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    #61
    Propagation is likely to be mostly normal with a chance that propagation crossing high latitudes may be mildly degraded during Saturday December 23rd by Frank Donovan, W3LPL
    __________________________________________________ _____________

    My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs included this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

    NWRA’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

    SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

    SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

    N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

    KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

    Mid-latitude northern hemisphere sunrise is 88 minutes later and sunset is 76 minutes earlier than it was on September 23rd. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

    There is a chance of isolated minor daytime radio blackouts caused by M-class solar flares through Saturday.

    The 2200Z Penticton 10.7 cm solar flux index was 195 and is likely to remain about the same through Saturday. The solar flux index is updated daily at 1800, 2000 and 2200Z at:
    http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

    SILSO’s latest Estimated International Sunspot Number is 160 and is likely to remain about the same through Saturday. The solar visible disk has one very large, one large, five medium and two tiny active regions containing 43 sunspots with a total sunspot area of 1285 micro-hemispheres (about six times the surface area of the Earth).
    http://www.sidc.be/spaceweatherservi...tions/solarmap

    Solar wind speed is likely to return to a slow solar wind regime at 400 km/second or less through late Friday due to waning coronal hole high speed stream effects. Coronal hole high speed stream effects are likely to weakly enhance the solar wind through midday Saturday.

    Geomagnetic activity is likely to be mostly quiet to unsettled through Thursday improving to mostly quiet on Friday. Coronal hole high speed stream effects are likely to produce unsettled to active geomagnetic activity through midday Saturday, declining to quiet to unsettled after midday Saturday.

    160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be normal through Saturday.

    40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal with a chance of mild degradation on Saturday. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal with a chance of mild degradation on Saturday.

    30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal with a chance of mild degradation on Saturday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

    20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal with a chance of mild degradation on Saturday.

    17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal with a chance of mild degradation on Saturday. 17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal with a chance of mild degradation on Saturday.

    12 and 10 meter long distance propagation is likely to mostly normal with a chance of mild degradation on Saturday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal with a chance of mild degradation on Saturday.

    We are in the winter solstice season when geomagnetic disturbances are about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent than during the equinox seasons.

    There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

    Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

    SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
    http://www.swpc.noaa.gov/products/ge...-activity-plot

    SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

    GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
    https://spaceweather.gfz-potsdam.de/...index-forecast

    SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

    The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

    Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
    73 Al 4L5A

    Comment

    •  

      #62
      Propagation is likely to be mostly normal but propagation crossing high latitudes is likely to be mildly degraded from midday Monday through midday Tuesday January 2nd by Frank Donovan, W3LPL
      __________________________________________________ _____________

      My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs included this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

      NWRA’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

      SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

      The Penticton solar flux index is updated daily at 1800, 2000 and 2200Z at:
      http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

      SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

      SWPC’s four day solar wind prediction is updated daily at http://www.swpc.noaa.gov/products/ws...ind-prediction

      N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

      KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

      Mid-latitude northern hemisphere sunrise is 4 minutes later and sunset is 7 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

      Minor daytime radio blackouts caused by M-class solar flares are probable through Tuesday. There is a chance of strong to severe X-class solar flares through Tuesday.

      The 2200Z Penticton 10.7 cm solar flux index was 146 and is likely to remain about the same through Tuesday.

      SILSO’s latest Estimated International Sunspot Number is 55 and is likely to remain about the same through Tuesday. The solar visible disk has three medium and two tiny active regions containing 15 sunspots with a total sunspot area of 380 micro-hemispheres (about twice the surface area of the Earth).
      http://www.sidc.be/spaceweatherservi...tions/solarmap

      Solar wind speed is likely to increase to about 450 km/second due to waning coronal hole high speed stream effects due to Coronal hole high speed stream effects through Tuesday.

      Geomagnetic activity is likely to be mostly quiet to unsettled through midday Monday. Coronal hole high speed stream effects are likely to produce unsettled to active conditions through midday Tuesday improving to mostly quiet through late Tuesday as coronal hole high speed stream activity wanes.

      160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be normal through Tuesday.

      40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mild degraded on Monday and mostly normal on Tuesday. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Tuesday.

      30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal with periods of mild degradation from midday Monday through midday Tuesday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

      20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal with periods of mild degradation from midday Monday through midday Tuesday

      17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal with periods of mild degradation from midday Monday through midday Tuesday. 17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Tuesday.

      12 and 10 meter long distance propagation is likely to be mostly normal with periods of mild degradation from midday Monday through midday Tuesday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal throughTuesday.

      We are in the winter solstice season when geomagnetic disturbances are about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent than during the equinox seasons.

      There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

      Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

      SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
      http://www.swpc.noaa.gov/products/ge...-activity-plot

      SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

      GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
      https://spaceweather.gfz-potsdam.de/...index-forecast

      SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

      The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

      Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
      73 Al 4L5A

      Comment

      •  

        #63
        Propagation is likely to be mostly normal but propagation crossing high latitudes is likely to be mildly degraded through midday Wednesday January 2nd by Frank Donovan, W3LPL
        __________________________________________________ _____________

        My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs included this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

        Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

        SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

        The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
        http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

        SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

        SWPC’s four day solar wind prediction is updated daily at http://www.swpc.noaa.gov/products/ws...ind-prediction

        N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

        KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

        Mid-latitude northern hemisphere sunrise is 4 minutes later and sunset is 8 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

        Minor daytime radio blackouts caused by M-class solar flares are likely with a chance of strong to severe radio blackouts caused by X-class solar flares through Wednesday.

        The 2200Z Penticton 10.7 cm solar flux index was 135 and is likely to remain about the same through Wednesday.

        SILSO’s latest Estimated International Sunspot Number is 51 and is likely to remain about the same through Wednesday. The solar visible disk has two medium and one tiny active region containing 14 sunspots with a total sunspot area of 210 micro-hemispheres (about the same as the surface area of the Earth).
        http://www.sidc.be/spaceweatherservi...tions/solarmap

        Coronal hole high speed stream and CME effects are likely to produce high speed solar wind well above 500 km/second before 0800Z Tuesday, gradually waning to below 500 km/second by midday Wednesday.

        Coronal hole high speed stream and CME effects are likely to produce geomagnetic activity at minor storm levels through midday Tuesday, improving to unsettled to active conditions through midday Wednesday. Mostly quiet geomagnetic conditions are likely after midday Wednesday as coronal high speed stream and CME effects gradually wane.

        160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be normal through Wednesday.

        40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mildly degraded on Tuesday then mostly normal on Wednesday. Short path propagation between North America and east Asia after about 0800Z is likely to be mildly degraded on Tuesday and mostly normal on Wednesday.

        30 meter propagation crossing the auroral ovals and polar regions is likely to be mildly degraded through midday Wednesday then mostly normal through late Wednesday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

        20 meter propagation crossing the auroral ovals and polar regions is likely to be mildly degraded through midday Wednesday then mostly normal through late Wednesday.

        17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mildly degraded through midday Wednesday then mostly normal through late Wednesday. 17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mildly degraded on Tuesday and mostly normal on Wednesday.

        12 and 10 meter long distance propagation is likely to be mildly degraded through midday Wednesday then mostly normal through late Wednesday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mildly degraded on Tuesday and mostly normal on Wednesday.

        We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

        There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

        Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

        SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
        http://www.swpc.noaa.gov/products/ge...-activity-plot

        SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

        GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
        https://spaceweather.gfz-potsdam.de/...index-forecast

        SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

        The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

        Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
        73 Al 4L5A

        Comment

        •  

          #64
          Propagation is likely to be mostly normal with a chance that propagation crossing high latitudes may be mildly degraded through Thursday January 3rd by Frank Donovan, W3LPL
          __________________________________________________ _____________

          My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs included this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

          Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

          SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

          The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
          http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

          SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

          SWPC’s four day solar wind prediction is updated daily at http://www.swpc.noaa.gov/products/ws...ind-prediction

          N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

          KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

          Mid-latitude northern hemisphere sunrise is 4 minutes later and sunset is 9 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

          Minor daytime radio blackouts caused by M-class solar flares are likely with a chance of strong to severe daytime radio blackouts caused by X-class solar flares through Thursday.

          The 2200Z Penticton 10.7 cm solar flux index was 142 and is likely to remain about the same through Thursday.

          SILSO’s latest Estimated International Sunspot Number is 64 and is likely to remain about the same through Thursday. The solar visible disk has one large, one medium and two tiny active regions containing 19 sunspots with a total sunspot area of 300 micro-hemispheres (about 50% larger than the surface area of the Earth).
          http://www.sidc.be/spaceweatherservi...tions/solarmap

          Lingering coronal hole high speed stream effects are likely to maintain solar wind at about 400 km/second through midday Wednesday, gradually slowing to background levels well below 400 km/second by Thursday.

          Lingering coronal hole high speed stream effects are likely to maintain mostly quiet to unsettled activity through midday Wednesday, improving to mostly quiet conditions through Thursday as coronal high speed stream effects wane.

          160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be normal through Thursday.

          40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal through Thursday. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Thursday.

          30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Thursday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

          20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Thursday.

          17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Thursday. 17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Thursday.

          12 and 10 meter long distance propagation is likely to be mostly normal through Thursday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Thursday.

          We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

          There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

          Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

          SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
          http://www.swpc.noaa.gov/products/ge...-activity-plot

          SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

          GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
          https://spaceweather.gfz-potsdam.de/...index-forecast

          SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

          The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

          Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
          73 Al 4L5A

          Comment

          •  

            #65
            Propagation is likely to be mostly normal but there is a chance that propagation crossing high latitudes may be mildly degraded through Friday January 5th by Frank Donovan, W3LPL
            __________________________________________________ _____________

            My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs included this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

            Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

            SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

            The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
            http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

            SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

            SWPC’s four day solar wind prediction is updated daily at http://www.swpc.noaa.gov/products/ws...ind-prediction

            N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

            KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

            Mid-latitude northern hemisphere sunrise is 4 minutes later and sunset is 10 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

            Minor daytime radio blackouts caused by M-class solar flares are likely with a chance of strong daytime radio blackouts caused by X-class solar flares through Friday.

            The 2200Z Penticton 10.7 cm solar flux index was 140 and is likely to remain about the same through Friday.

            SILSO’s latest Estimated International Sunspot Number is 58 and is likely to remain about the same through Friday. The visible solar disk has one large, one medium and two tiny active regions containing 23 sunspots with a total sunspot area of 350 micro-hemispheres (about twice the surface area of the Earth).
            http://www.sidc.be/spaceweatherservi...tions/solarmap

            Lingering coronal hole high speed stream effects are likely to maintain the solar wind speed above 400 km/second through Friday.

            Lingering coronal hole high speed stream effects are likely to maintain mostly quiet to unsettled geomagnetic activity through Thursday, improving to mostly quiet conditions through Friday as coronal high speed stream effects wane.

            160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be normal through Friday.

            40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal through Friday. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Friday.

            30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Friday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

            20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Friday.

            17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Friday. 17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Friday.

            12 and 10 meter long distance propagation is likely to be mostly normal through Friday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Friday.

            We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

            There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

            Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

            SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
            http://www.swpc.noaa.gov/products/ge...-activity-plot

            SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

            GFZ-Potsdam’s three-day Planetary K Index Forecast is updated every three hours at:
            https://spaceweather.gfz-potsdam.de/...index-forecast

            SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

            The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

            Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
            73 Al 4L5A

            Comment

            •  

              #66
              Propagation is likely to be mostly normal but there is a chance that propagation crossing high latitudes may be mildly degraded through early Tuesday January 9th by Frank Donovan, W3LPL
              __________________________________________________ _____________

              My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs included at the end forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

              The 2200Z Penticton 10.7 cm solar flux index was 170 and is likely to remain about the same through Tuesday.

              SILSO’s latest Estimated International Sunspot Number is 169 and is likely to remain about the same through Tuesday. The visible solar disk has one large, six medium and three tiny active regions containing 71 sunspots with a total sunspot area of 800 micro-hemispheres (about four times the surface area of the Earth).
              http://www.sidc.be/spaceweatherservi...tions/solarmap

              We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

              Solar wind speed is likely to increase to above 400 km/second after midday Monday due to coronal hole high speed stream effects, declining to below 400 km/second before midday Tuesday as coronal hole high speed stream effects wane.

              Quiet to unsettled geomagnetic activity is likely through early Tuesday, declining to mostly quiet before midday Tuesday as coronal hole high speed stream effects wane.

              There is a chance of minor daytime radio blackouts caused by M-class solar flares and a slight chance of strong daytime radio blackouts caused by X-class solar flares through Tuesday.

              160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be normal through Tuesday.

              40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal through Tuesday. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Tuesday.

              30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Tuesday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

              20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Tuesday.

              17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Tuesday. 17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Tuesday.

              12 and 10 meter long distance propagation is likely to be mostly normal through Tuesday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Tuesday.

              There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

              Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

              Mid-latitude northern hemisphere sunrise is 4 minutes later and sunset is 12 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

              Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

              SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

              The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
              http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

              SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

              SWPC’s four day solar wind prediction is updated a few times per week at http://www.swpc.noaa.gov/products/ws...ind-prediction

              N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

              KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

              SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
              http://www.swpc.noaa.gov/products/ge...-activity-plot

              SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

              GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
              https://spaceweather.gfz-potsdam.de/...index-forecast

              SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

              The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

              Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation and www.solarham.net
              73 Al 4L5A

              Comment

              •  

                #67
                Propagation is likely to be mostly normal through late Thursday but there is a chance that propagation crossing high latitudes may be mildly degraded through early Wednesday January 10th by Frank Donovan, W3LPL
                __________________________________________________ _____________

                My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs included at the end forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

                The 2200Z Penticton 10.7 cm solar flux index was 174 and is likely to remain about the same through Wednesday.

                SILSO’s latest Estimated International Sunspot Number is 161 and is likely to remain about the same through Wednesday. The visible solar disk has one large, five medium and three tiny active regions containing 62 sunspots with a total sunspot area of 700 micro-hemispheres (about four times the surface area of the Earth).
                http://www.sidc.be/spaceweatherservi...tions/solarmap

                We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

                Solar wind speed is likely to remain slightly elevated at less than 400 km/second through early Wednesday due to weak coronal hole high speed stream effects, declining to about 350 km/second through late Thursday as coronal hole high speed stream effects further weaken.

                Mostly quiet geomagnetic activity is likely, with a chance of isolated unsettled conditions due to weak coronal hole high speed stream effects through early Wednesday. Mostly quiet conditions are likely to continue through late Thursday as coronal hole high speed stream effects further weaken.

                There is a chance of minor daytime radio blackouts caused by M-class solar flares and a slight chance of strong daytime radio blackouts caused by X-class solar flares through Thursday.

                160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be normal through late Thursday.

                40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal through Thursday. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Thursday.

                30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through late Thursday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

                20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through late Thursday.

                17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through late Thursday.17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through late Thursday.

                12 and 10 meter long distance propagation is likely to be mostly normal through late Thursday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through late Thursday.

                There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

                Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

                Mid-latitude northern hemisphere sunrise is 4 minutes later and sunset is 13 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

                Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

                SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

                The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
                http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

                SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

                SWPC’s four day solar wind prediction is updated about every five days at http://www.swpc.noaa.gov/products/ws...ind-prediction

                N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

                KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

                SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
                http://www.swpc.noaa.gov/products/ge...-activity-plot

                SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

                GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
                https://spaceweather.gfz-potsdam.de/...index-forecast

                SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

                The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

                Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation and www.solarham.net
                73 Al 4L5A

                Comment

                •  

                  #68
                  Propagation is likely to be mostly normal through Friday January 12th by Frank Donovan, W3LPL
                  __________________________________________________ _____________

                  My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs at the end of this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

                  The 2200Z Penticton 10.7 cm solar flux index was 176 and is likely to remain about the same through Friday.

                  SILSO’s latest Estimated International Sunspot Number is 149 and is likely to remain about the same through Thursday. The visible solar disk has one large, seven medium and three tiny active regions containing 73 sunspots with a total sunspot area of 1060 micro-hemispheres (about five times the surface area of the Earth).
                  http://www.sidc.be/spaceweatherservi...tions/solarmap

                  We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

                  Solar wind speed is likely to remain slightly elevated at about 400 km/second through early Wednesday due to weak coronal hole high speed stream effects, declining to about 350 km/second through Friday as coronal hole high speed stream effects further weaken.

                  Mostly quiet geomagnetic activity is likely through Friday.

                  There is a chance of minor daytime radio blackouts caused by M-class solar flares through Friday.

                  160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be mostly normal through Friday.

                  40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal through Friday.. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Friday.

                  30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Friday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

                  20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Friday.

                  17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Friday.17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Friday.

                  12 and 10 meter long distance propagation is likely to be mostly normal through Friday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Friday.

                  There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

                  Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

                  Mid-latitude northern hemisphere sunrise is 4 minutes later and sunset is 13 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

                  Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

                  SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

                  The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
                  http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

                  SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

                  SWPC’s four day solar wind prediction is updated about every five days at http://www.swpc.noaa.gov/products/ws...ind-prediction

                  N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

                  KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

                  SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
                  http://www.swpc.noaa.gov/products/ge...-activity-plot

                  SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

                  GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
                  https://spaceweather.gfz-potsdam.de/...index-forecast

                  SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

                  The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

                  Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
                  73 Al 4L5A

                  Comment

                  •  

                    #69
                    Propagation is likely to be mostly normal through Saturday January 13th by Frank Donovan, W3LPL
                    __________________________________________________ _____________

                    My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs at the end of this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

                    The 2200Z Penticton 10.7 cm solar flux index was 190 and is likely to remain about the same through Saturday.

                    SILSO’s latest Estimated International Sunspot Number is 164 and is likely to remain about the same through Saturday. The visible solar disk has three large, five medium and two tiny active regions containing 83 sunspots with a total sunspot area of 1200 micro-hemispheres (about six times the surface area of the Earth).
                    http://www.sidc.be/spaceweatherservi...tions/solarmap

                    We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

                    Solar wind speed is likely to remain elevated above 450 km/second until about midday Thursday due to weak coronal hole high speed stream effects, declining to less than 400 km/second through Saturday as coronal hole high speed stream effects weaken.

                    Mostly quiet geomagnetic activity is likely through Saturday.

                    There is a chance of minor daytime radio blackouts caused by M-class solar flares through Saturday.

                    160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be mostly normal through Saturday.

                    40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal through Saturday.. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Saturday.

                    30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Saturday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

                    20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Saturday.

                    17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Saturday.17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Saturday.

                    12 and 10 meter long distance propagation is likely to be mostly normal through Saturday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Saturday.

                    There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

                    Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

                    Mid-latitude northern hemisphere sunrise is 3 minutes later and sunset is 14 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

                    Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

                    SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

                    The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
                    http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

                    SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

                    SWPC’s four day solar wind prediction is updated about every five days at http://www.swpc.noaa.gov/products/ws...ind-prediction

                    N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

                    KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

                    SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
                    http://www.swpc.noaa.gov/products/ge...-activity-plot

                    SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

                    GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
                    https://spaceweather.gfz-potsdam.de/...index-forecast

                    SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

                    The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

                    Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
                    73 Al 4L5A

                    Comment

                    •  

                      #70
                      Propagation is likely to be mostly normal through Sunday January 14th by Frank Donovan, W3LPL
                      __________________________________________________ _____________

                      My propagation forecast derived from today's NOAA/SWPC web pages and twelve other online sources (the URLs at the end of this forecast) is published five days a week (M-F) in The Daily DX. All days and times in this forecast are in UTC (Zulu) time.

                      The 2200Z Penticton 10.7 cm solar flux index was 188 and is likely to remain about the same through Sunday.

                      SILSO’s latest Estimated International Sunspot Number is 170 and is likely to remain about the same through Sunday. The visible solar disk has one large, six medium and two tiny active regions containing 61 sunspots with a total sunspot area of 810 micro-hemispheres (about four times the surface area of the Earth).
                      http://www.sidc.be/spaceweatherservi...tions/solarmap

                      We are in the winter solstice season when geomagnetic disturbances are less severe and about half as likely as during the equinox seasons and geomagnetically quiet periods are much more frequent and long lasting than during the equinox seasons.

                      Solar wind speed is likely to remain elevated above 450 km/second through Sunday due to coronal hole high speed stream effects.

                      Mostly quiet geomagnetic activity is likely through Sunday.

                      There is a chance of minor daytime radio blackouts caused by M-class solar flares through Sunday.

                      160 and 80 meter propagation from North America to VK/ZL and the South Pacific is likely to be mostly normal through Sunday.

                      40 meter short path propagation from North America to south Asia after about 2200Z is likely to be mostly normal through Sunday.. Short path propagation between North America and east Asia after about 0800Z is likely to be mostly normal through Sunday.

                      30 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Sunday. 30 meter propagation is always mildly to moderately degraded within several hours of local noon by E-region blanketing of long distance low angle F2 propagation.

                      20 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Sunday.

                      17 and 15 meter propagation crossing the auroral ovals and polar regions is likely to be mostly normal through Sunday.17 and 15 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Sunday.

                      12 and 10 meter long distance propagation is likely to be mostly normal through Sunday. 12 and 10 meter long path propagation from North America to southeast and east Asia from about 1200Z to 1400Z is likely to be mostly normal through Sunday.

                      There is a very slight chance of brief geographically focused 6 meter above-the-MUF trans-Atlantic F2 propagation from about 1300-1500Z between mid-latitude U.S states and western Europe, this above-the-MUF propagation path may be skewed towards the east. There is a very slight chance of brief geographically focused 6 meter F2 propagation enhanced by TEP over Africa from the mid-latitude US states to the Indian Ocean, equatorial and southern Africa (e.g., 3B8. 3B9, 7Q, D2, FR, V5, ZD7 and ZS) from about 1500-1800Z. There is a very slight chance of widespread F2 trans-equatorial propagation (TEP) from mid-latitude U.S. states to South America from about 2100-0100Z. There is a very slight chance of above-the-MUF F2 propagation enhanced by oblique-TEP from the mid-latitude US states to the south Pacific (e.g., 5W, E5, FK, ZL7 and VK/ZL) from about 2200-0100Z. There is a very slight chance that more northerly U.S. stations may couple into TEP and oblique-TEP via geographically focused brief intervals of above-the-MUF F2 propagation. TEP may be significantly enhanced from late afternoon through early evening during the onset of strong to severe solar flares and geomagnetic storms then significantly degrading after initial enhancement. See K6MIO’s excellent article on 6 meter TEP, oblique-TEP, TEP-related and mid-latitude sporadic-E linking to TEP beginning on page 9 at: http://www.oh3ac.fi/QEX-2016-11.pdf

                      Southward orientation (-Bz) of the north-south component of the interplanetary magnetic field (IMF) plays a crucial but unpredictable role in triggering all geomagnetic storms. Brief minor to moderate geomagnetic storms may be gradually triggered when the IMF persists in a southward orientation (-Bz) with IMF field strength of about 5 nanoteslas for several hours coincident with the effects of an Earth directed coronal hole high speed stream. More frequent, longer duration, minor to severe geomagnetic storms may be triggered suddenly and unpredictably when the IMF persists in a southward orientation (-Bz) with IMF field strength mildly stronger than 5 nanoteslas for at least a few hours coincident with the effects of an Earth directed CME and solar wind speed exceeding 500 km/second.

                      Mid-latitude northern hemisphere sunrise is 3 minutes later and sunset is 14 minutes later than it was on December 21st. Sunrise is about two hours earlier and sunset is about two hours later at the 300 km altitude of the F2 region than it is at ground level.

                      Northwest Research Associate’s Table of Space Weather Indices is updated 40 minutes after every hour at https://spawx.nwra.com/spawx/env_latest.html

                      SILSO’s Estimated International Sunspot Number is updated continuously at www.sidc.be/silso/DATA/EISN/EISNcurrent.png

                      The Penticton 10.7 cm solar flux index is updated daily at 1800, 2000 and 2200Z at:
                      http://www.spaceweather.gc.ca/foreca...-5-flux-en.php

                      SWPC’s Estimated Planetary Kp Index is updated every three hours at https://services.swpc.noaa.gov/image...on-k-index.png

                      SWPC’s four day solar wind prediction is updated about every five days at http://www.swpc.noaa.gov/products/ws...ind-prediction

                      N0NBH’s Current HF Band Conditions Report is updated regularly at www.hamqsl.com/solar.html

                      KC2G’s Near-Real-Time Maps and Data about HF propagation are generated every 15 minutes, from near real time data usually only 5 to 20 minutes old at https://prop.kc2g.com

                      SWPC’s Real Time 24 hour Geomagnetic Data including Bz orientation, IMF field strength, solar wind speed and near real time 30 minute forecasts are updated frequently at:
                      http://www.swpc.noaa.gov/products/ge...-activity-plot

                      SIDC’s Daily Bulletin on Solar and Geomagnetic Activity is updated daily at 1230Z at http://www.sidc.be/spaceweatherservi...uct/meu/latest

                      GFZ-Potsdam’s three-day GFZ Planetary K Index Forecast is updated every three hours at:
                      https://spaceweather.gfz-potsdam.de/...index-forecast

                      SWPC’s Solar Activity Forecast and Discussion is updated daily at 0030Z and 1230Z at: www.swpc.noaa.gov/products/forecast-discussion

                      The Australian Space Forecast Centre’s Summary and Forecast is updated daily at 2330Z at: www.sws.bom.gov.au/Space_Weather/1/1

                      Perhaps the most useful HF propagation pages for DXers can be found at: http://dx.qsl.net/propagation
                      73 Al 4L5A

                      Comment

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