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OVERVIEW & FORECAST

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Day 1 To 3
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Weekly Forecast

During the past 24 hours, solar activity was moderate. Eight sunspot active regions were on the visble disk with three M-class flares produced. The solar wind speed decreased to about 400 km/s. The geomagnetic field was quiet to unsettled.
	Published:	2026-02-09 00:30 UTC
	Forecaster:	012/041

Within the next three days, solar activity is expected to be quiet to moderate with chances for M-class and above flares. The geomagnetic field is expected to be mainly quiet to unsettled.
	Published:	2026-02-09 00:30 UTC
	Forecaster:	012/041

During the last week, solar activity was extremely high on 1 Feb, high on 2-5 Feb and low for the rest of the time. Fifteen active sunspot regions (AR4349, AR4357-AR4360, AR4362-AR4363, AR4365-AR4372) were on the visible disk with 6 X-class and 61 M-Class flares produced. No solar proton event occured. The F10.7 index ranged from 128 sfu to 178 sfu. Due to the continuous effect of the recurrent coronal hole high speed stream, the geomagnetic field reached active levels for 3 hours on 30 Jan. Due to the arrival of the CME which associated with X8.1 flare on 2 Feb, the solar wind speed reached a peak value of 610 km/s, and the geomagnetic field reached minor storm levels for 6 hours and active levels for 9 hours on 4-5 Feb. The geomagnetic field was quiet to unsettled on the rest of the time. The greater than 2 MeV electron flux at geosynchronous orbit maintained at minor storm levels during 30 Jan - 4 Feb.
	Published:	2026-02-06 06:30 UTC
	Forecaster:	027/026

Within the next week, solar activity is expected to be mainly moderate with chances for M-class and above flares. The geomagnetic field is expected to reach isolated active levels on 6-7 Feb due to the effect of the recurrent coronal hole high speed stream. It will be mainly quiet to unsettled for the rest of the time.
	Published:	2026-02-06 06:30 UTC
	Forecaster:	027/026

ALERTS


	Space environment alerts have been issued today.


	02:48 UTC 09 Feb 2026	12:57 UTC 08 Feb 2026	11:59 UTC 08 Feb 2026	11:21 UTC 08 Feb 2026	22:20 UTC 05 Feb 2026

LATEST DATA



		The magnetic map of the activity area is generated based on the full day longitudinal magnetic field data of the Huairou Solar Observatory in Beijing.				This full-disk Hα image of sun is observed with the 20cm Full-Disc Hα Telescope located at Huairou Solar Observatory Station of Beijing in China.



		Observatories of cosmic ray in SEPC include Beijing station monitoring Neutron intensity variations and Guangzhou station monitoring the intensity variations of East, West, South, North and Vertical components of muon.				This model is an improved geomagnetic K-index current reporting model based on the evaluation of Takahashi, a commonly used international Kp index current reporting model, and its application to Chinese geomagnetic stations.

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	24-hr Max:M2.8
	Peak Time:2026 Feb 09 02:27 UTC

	Updated:2026 Feb 09 06:47 UTC
	>>more data<<


	Current 5-min:1.865e-1 /cm².sr.s
	24-hr Max:2.733e-1 /cm².sr.s

	Updated:2026 Feb 09 06:40 UTC
	>>more data<<


	Speed:419.7 km/sec
	Density:0.6 protons/cm³

	Updated:2026 Feb 09 06:57 UTC
	>>more data<<


	Current:Kp=1
	24-hr Max:Kp=3

	Updated:2026 Feb 09 06:00 UTC
	>>more data<<


	Current 5-min:5.330e+2 /cm².sr.s
	Integral Flux:8.512e+7 /cm².sr.day

	Updated:2026 Feb 09 06:40 UTC
	>>more data<<


	10.7cm Flux:167 sfu

	Update:2026 Feb 08 UTC
	>>more data<<


	SSN:118

	Update:2026 Feb 08 UTC
	>>more data<<