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ARCHIVE

DAILY REPORTS

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During the past 24 hours, solar activity was low. Nine active sunspot regions were on the visble disk without any M-class or above flares produced. The solar wind speed maintained at about 430 km/s, and the geomagnetic field was quiet. The greater than 2 MeV electron flux at geosynchronous orbit reached moderate storm levels.
Within the next three days, solar activity is expected to be low to moderate with a chance for M-class and above flares. The geomagnetic field is expected to reach isolated active to minor storm levels due to the effects of CME on 3 Oct. The greater than 2 MeV electron flux at geosynchronous orbit will maintain at minor storm levels on 7 Oct.
	Published:	2025-10-06 23:51 UTC
	Forecaster:	022

During the past 24 hours, solar activity was low. 7 active sunspot regions were on the visble disk without M-class or above flares produced. Due to the effect of CME from 3 Oct, the solar wind speed maintained at about 410 km/s, and the geomagnetic field reached active level for 3 hours and was quiet to unsettled for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit reached minor storm level.
Within the next three days, solar activity is expected to be mainly low with little chance for M-class flares. The geomagnetic field is expected to reach isolated active levels on 8 Oct due to the effect of CME on from 3 Oct and isolated active levels on 10 Oct due to the effect of coronal hole high speed stream. The greater than 2 MeV electron flux at geosynchronous orbit will maintain at minor storm levels on 8-10 Oct.
	Published:	2025-10-08 00:11 UTC
	Forecaster:	026

During the past 24 hours, solar activity was low. 5 active sunspot regions were on the visble disk without M-class or above flares produced. Due to the continuous effect of CME from 3 Oct, the solar wind speed maintained at about 310 km/s to 400 km/s. The geomagnetic field reached active level for 3 hours and was quiet to unsettled for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit maintained at minor storm level.
Within the next three days, solar activity is expected to be mainly low. The geomagnetic field is expected to reach isolated minor storm levels on 11 Oct due to the effect of recurrent coronal hole high speed stream, mainly quiet to unsettled for the rest of the time.
	Published:	2025-10-08 23:56 UTC
	Forecaster:	026/027

During the past 24 hours, solar activity was moderate. Six active sunspot regions were on the visble disk with one M2 flare produced. The solar wind speed maintained at about 320 km/s. The geomagnetic field was quiet. The greater than 2 MeV electron flux at geosynchronous orbit maintained at minor storm level.
Within the next three days, solar activity is expected to be mainly low. The geomagnetic field is expected to reach isolated minor storm levels on 11-12 Oct due to the effect of the recurrent coronal hole high speed stream, and mainly quiet to unsettled for the rest of the time.
	Published:	2025-10-09 23:42 UTC
	Forecaster:	027/016

During the past 24 hours, solar activity was low. Six active sunspot regions were on the visble disk without M-class flare produced. The solar wind speed increased to about 370 km/s. The geomagnetic field reached active levels for 3 hours and was quiet to unsettled for the rest of the time.
Within the next three days, solar activity is expected to be mainly low. The geomagnetic field is expected to reach active to minor storm levels due to the effect of the recurrent coronal hole high speed stream.
	Published:	2025-10-10 23:47 UTC
	Forecaster:	016/042

During the past 24 hours, solar activity was low. Seven active sunspot regions were on the visble disk without M-class flare produced. The solar wind speed increased to about 540 km/s. The geomagnetic field reached minor storm levels for 3 hours, active levels for 6 hours and was quiet to unsettled for the rest of the time.
Within the next three days, solar activity is expected to be mainly low. The geomagnetic field is expected to reach active to minor storm levels on 12-13 Oct due to the effect of the recurrent coronal hole high speed stream. It will be quiet to unsettled on 14 Oct. The greater than 2 MeV electron flux at geosynchronous orbit will reach minor storm level on 14 Oct.
	Published:	2025-10-11 23:56 UTC
	Forecaster:	042/039

During the past 24 hours, solar activity was low. Seven active sunspot regions were on the visble disk without M-class flare produced. Due to the continuous effect of the recurrent coronal hole high speed stream, the solar wind speed increased to about 730 km/s. The geomagnetic field reached minor storm levels for 3 hours, active levels for 21 hours.
Within the next three days, solar activity is expected to be low to moderate. The geomagnetic field is expected to reach active levels on 13-14 Oct due to the continuous effect of the recurrent coronal hole high speed stream. Due to the effect of CME from 11 Oct, it will reach active levels on 15 Oct. The greater than 2 MeV electron flux at geosynchronous orbit will reach active level on 14-15 Oct.
	Published:	2025-10-13 00:00 UTC
	Forecaster:	039/041

WEEKLY REPORTS

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During the last week, solar activity was moderate on 22-26, 28 Aug and low for the rest of time. Eighteen active sunspot regions (AR4187-AR4204) were on the visible disk with sixteen M-class flares produced. The greater than 10 MeV proton flux at geosynchronous orbit reached the threshold of minor solar proton event levels on 26-27 Aug with a peak of 14 pfu. The F10.7 index increased from 136 sfu to 232 sfu. The geomagnetic field was at quiet to unsettled levels.
Within the next week, solar activity is expected to be low to moderate with chances for M-class flares. The geomagnetic field is expected to be mainly quiet to unsettled.
	Published:	2025-08-29 02:32 UTC
	Forecaster:	012/029

During the last week, solar activity was moderate on 29-30 Aug, 4 Sep and low for the rest of time. Seventeen active sunspot regions (AR4191, AR4196-AR4202, AR4204-AR212) were on the visible disk with five M-class flares produced. No solar proton event levels happened. The F10.7 index decreased from 232 sfu to 172 sfu. The geomagnetic field was at moderate storm levels for 3 hours, minor storm levels for 9 hours, active levels for fifteen hours, due to the effect of the halo CME on 30 Aug, it was quiet to unsettled levels for the rest of time.
Within the next week, solar activity is expected to be low to moderate with chances for M-class flares. The geomagnetic field is expected to be mainly at quiet to unsettled levels with isolated minor storm levels on 5-7 Sep and active levels on 8-10 Sep due to the effect of the recurrent coronal hole high speed stream and the CME on 4 Sep. it will be quiet to unsettled levels for the rest of time.
	Published:	2025-09-05 02:11 UTC
	Forecaster:	026/040

During the last week, solar activity was moderate on 5-6 Sep, and low for the rest of time. Thirteen active sunspot regions (AR4197, AR4199, AR4201-AR4202, AR4206-AR4207, AR4210-AR4216) were on the visible disk with two M-class flares produced. No solar proton event levels happened. The F10.7 index decreased from 149 sfu to 115 sfu. Due to the effect of the recurrent coronal hole high speed stream and CME of 4 Sep, the solar wind speed reached a peak value of 670 km/s, the geomagnetic field was at minor storm levels for 3 hours, active levels for fifteen hours on 6 Sep. The geomagnetic field was at moderate storm levels for 3 hours, active levels for twelve hours on 8-11 Sep, it was quiet to unsettled levels for the rest of time.
Within the next week, solar activity is expected to be low to moderate with chances for M-class flares. The geomagnetic field is expected to be mainly at quiet to unsettled levels with isolated active to minor storm levels on 13-15 Sep due to the effect of the recurrent coronal hole high speed stream.
	Published:	2025-09-12 03:50 UTC
	Forecaster:	026/012

During the last week, solar activity was low. Fourteen active sunspot regions (AR4211, AR4213-4225) were on the visible disk with no M-class flares produced. No solar proton event occurred. The F10.7 index increased from 114 sfu to 150 sfu. Due to the effect of the recurrent coronal hole high speed stream, the solar wind speed reached a peak value of 800 km/s, the geomagnetic field was at major storm levels for 3 hours, minor storm levels for 18 hours and active levels for 21 hours during 14-16 Sep. It was at quiet to unsettled levels for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit maintained at minor storm levels on 16-18 Sep.
Within the next week, solar activity is expected to be low to moderate with a chance for M-class flares. Due to the effect of the recurrent coronal hole high speed stream, the geomagnetic field is expected to reach isolated active or minor storm levels on 22-23 Sep. It will be mainly quiet to unsettled for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit will maintain at minor storm levels on 19-21 Sep.
	Published:	2025-09-19 02:23 UTC
	Forecaster:	027/042

During the last week, solar activity was low to moderate. Fifteen active sunspot regions (AR4216-4217, AR4219-4231) were on the visible disk with 4 M-class flares produced. No solar proton event occurred. The F10.7 index varied between 160 sfu and 184 sfu. Due to the effect of a recurrent coronal hole high speed stream, the solar wind speed reached a peak value of 600 km/s during 22-23 Sep, and the geomagnetic field was at active levels for 3 hours. The geomagnetic field was at quiet to unsettled levels for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit maintained at minor storm levels on 19-21 Sep.
Within the next week, solar activity is expected to be low to moderate with a chance for M-class flares. The geomagnetic field is expected to be quiet to unsettled.
	Published:	2025-09-26 02:24 UTC
	Forecaster:	012/022

During the last week, solar activity was high on 28 Sep and moderate on 26-27 Sep and 29 Sep to 2 Oct. Neneteen active sunspot regions (AR4217, AR4224-4241) were on the visible disk with 15 M-class flares produced. No solar proton event occurred. The F10.7 index varied between 164 sfu and 187 sfu. Due to the effects of a recurrent coronal hole high speed stream and geomagnetism during the autumn equinoxe, the solar wind speed reached a peak value of 750 km/s during 29 Sep to 2 Oct, and the geomagnetic field reached major storm levels for 6 hours, moderate storm levels for 15 hours, minor storm levels for 42 hours and active levels for 18 hours. The geomagnetic field was at quiet to unsettled levels for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit reached minor storm levels on 2 Oct.
Within the next week, solar activity is expected to be mainly moderate with a chance for M-class and above flares. The geomagnetic field is expected to reach active or minor storm levels 3-7 Oct due to the continuous effects of coronal hole high speed streams and geomagnetism during the autumn equinoxe. The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach minor storm levels on 3-5 Oct.
	Published:	2025-10-03 02:34 UTC
	Forecaster:	012

During the last week, solar activity was moderate on 3 Oct and 9 Oct, and low for the rest of the time. Fifteen active sunspot regions (AR4230, AR4232-4233, AR4235-4236, AR4238, AR4241-4249) were on the visible disk with 3 M-class flares produced. No solar proton event occurred. The F10.7 index decreased from 170 sfu to 120 sfu. Due to the effects of the recurrent coronal hole high speed stream, the solar wind speed reached a peak value of 800 km/s during 3-4 Oct, and the geomagnetic field reached minor storm levels for 6 hours and active levels for 27 hours. Due to the effect of the CME on 3 Oct, the solar wind speed reached a peak value of 450 km/s during 7-8 Oct, and the geomagnetic field reached active levels for 6 hours. The geomagnetic field was at quiet to unsettled levels for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit reached minor storm levels on 3-5 Oct, 7-9 Oct and reached moderate storm levels on 6 Oct.
Within the next week, solar activity is expected to be mainly low with a chance for M-class flares. The geomagnetic field is expected to reach storm levels on 11-13 Oct due to the effect of the recurrent coronal hole high speed stream. It will be quiet to unsettled for the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit is expected to reach minor storm levels on 14-16 Oct.
	Published:	2025-10-10 02:57 UTC
	Forecaster:	016/027

SOLAR IMAGES

The active region magnetogram is created from the raw full-disk longitudinal magnetogram data, which is observed at Huairou Solar Observatory Station of Beijing in China.