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| During the last week, solar activity was low on 12-13 Sep and very low for the rest of the time. Seven active sunspot regions (AR4521, AR4524-AR4525, AR4523-AR4530) were on the visible disk without any M-class or above flares produced. No Solar Proton Event occurred. The F10.7 index decreased from 114 sfu to 97 sfu. Due to the effects of a recurrent coronal hole high speed stream, the solar wind speed increased to a peak of about 600 km/s and the geomagnetic field was at active levels for 6 hours on 14-16 Sep and 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 11 and 14 Sep. | |
| Within the next week, solar activity is expected to be very low to low with chances for C-class flares. The geomagnetic field is expected to reach active levels to minor storm levels on 24 Sep due to the effect of a recurrent coronal hole high speed stream. It is expected to be mainly at quiet to unsettled levels for the rest of the time. | | Published: 2026-09-18 06:30 UTC Forecaster: 039/022 |
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| During the last week, solar activity was very low on 18 Sep and low for the rest of the time. Eleven active sunspot regions (AR4532-AR4542) were on the visible disk without any M-class or above flares produced. No Solar Proton Event occurred. The F10.7 index ranged from 96 sfu to 121 sfu. Due to the effects of a recurrent coronal hole high speed stream, the solar wind speed increased to a peak of about 440 km/s and the geomagnetic field was at active levels for 6 hours on 24 Sep and quiet to unsettled levels for the rest of the time. | |
| Within the next week, solar activity is expected to be very low to low with chances for C-class flares. The geomagnetic field is expected to reach active levels to minor storm levels on 25-26 Sep due to the continuous effect of a recurrent coronal hole high speed stream. It is expected to be mainly at quiet to unsettled levels for the rest of the time. | | Published: 2026-09-25 06:30 UTC Forecaster: 042/012 |
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| During the last week, solar activity remained at a low level. Eleven active sunspot regions (AR4533-AR4539, AR4542-AR4545) were on the visible disk without any M-class or above flares produced. No Solar Proton Event occurred. The F10.7 index decreased from 105 sfu to 92 sfu. Due to the effect of the recurrent coronal hole high speed stream, the solar wind speed reached a peak of about 550 km/s and the geomagnetic field was at active levels for 24 hours on 25-27 Sep. It was quiet to unsettled for the rest of time. The greater than 2 MeV electron flux at geosynchronous orbit reached minor storm levels on 27-30 Sep. | |
| Within the next week, solar activity is expected to be very low to low with chances for C-class flares. The geomagnetic field is expected to reach isolated minor storm levels on 2 Oct due to the arrival of a CME observed on 28 Sep, and reach minor storm levels on 3-4 Oct due to the effects of a coronal hole high speed stream. It is expected to be mainly 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 6-8 Oct. | | Published: 2026-10-02 06:30 UTC Forecaster: 026/010 |
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| During the last week, solar activity was high on 8 Oct, moderate on 5-6 Oct, low on 7 Oct and very low for the rest of time. Seven active sunspot regions (AR4535, AR4545-AR4550) were on the visible disk with 4 M-class flares produced. No Solar Proton Event occurred. The F10.7 index increased from 92 sfu to 119 sfu. Due to the effect of the coronal hole high speed stream, the solar wind speed reached a peak of about 600 km/s and the geomagnetic field was at moderate storm levels for 3 hours, minor storm levels for 12 hours and active levels for 18 hours on 4-5 Oct. It was quiet to unsettled for the rest of time. The greater than 2 MeV electron flux at geosynchronous orbit reached minor storm levels on 6-8 Oct. | |
| Within the next week, solar activity is expected to be moderate to low with chances for M-class flares. The geomagnetic field is expected to reach isolated active to minor or moderate storm levels on 9-11 Oct due to the arrival of the CMEs observed on 6-8 Oct, and reach active or minor storm levels on 12-14 Oct due to the effects of the recurrent coronal hole high speed stream. | | Published: 2026-10-09 06:30 UTC Forecaster: 027/022 |
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| During the last week, solar activity was high on 10 Oct, moderate on 9 Oct, low for the rest of time. Eleven active sunspot regions (AR4545, AR4548-AR4549, AR4551-AR4558) were on the visible disk with 3 M-class flares produced. No Solar Proton Event occurred. The F10.7 index fluctuated between 121 sfu and 136 sfu. Due to the co-effects of several CMEs on 7-8 and the recurrent coronal hole high speed stream, the solar wind speed reached a peak of about 890 km/s and the geomagnetic field reached major strom levels for 6 hours, minor storm levels for 3 hours and active levels for 9 hours on 9-11 Oct. It was quiet to unsettled 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 reach active or minor storm levels on 22-23 Oct due to the effect of the recurrent coronal hole high speed stream. | | Published: 2026-10-16 06:30 UTC Forecaster: 042/025 |
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