Space Environment Prediction Center





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	Station K Indices
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	Coronal Hole Index
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OVERVIEW & FORECAST

Daily Review
Day 1 To 3
Weekly Review
Weekly Forecast

During the past 24 hours, solar activity was very low without C-class and above flare produced. There was no active region on the visible disk. The solar wind speed maintained at about 360 km/s. The geomagnetic field was quiet to unsettled.
	Published:	2019-10-16 00:23 UTC
	Forecaster:	035/012

Within the next three days, solar activity is expected to be very low. The geomagnetic field is expected to be mainly quiet.
	Published:	2019-10-16 00:23 UTC
	Forecaster:	035/012

During last week, solar activity was very low. There was no active region on the visible disk, without C-class and above flare produced. The F10.7 index ranged from 67 sfu to 68 sfu. The solar wind speed increased to about 500 km/s on 10 Oct. The geomagnetic field was active levels for 9 hours on 9-10 Oct. The geomagentic field was quiet to unsettled during other periods. The greater than 2 MeV electron flux at geosynchronous orbit reached minor storm levels on 4 Oct.
	Published:	2019-10-11 02:37 UTC
	Forecaster:	015/029

Within the next week, solar activity is expected to be very low. Due to the effect of a recurrent coronal hole high speed stream, the geomagnetic field is expected to reach active levels on 14-15 Oct. It will be quiet to unsettled during other periods.
	Published:	2019-10-11 02:37 UTC
	Forecaster:	015/029

ALERTS


	No space environment alerts have been issued today.


	01:15 UTC 05 Oct 2019	00:15 UTC 04 Oct 2019	01:15 UTC 03 Oct 2019	01:15 UTC 02 Oct 2019	01:15 UTC 01 Oct 2019

LATEST DATA



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

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		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.				The Ionosphere GPS observation network , monitoring the ionospheric scintillation and GPS-TEC with time resolutions of 1 minute and 30 seconds, is located at Fuzhou, Xiamen, Guangzhou, Nanning and Hainan.

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	24-hr Max:A7.3
	Peak Time:2019 Oct 16 08:05 UTC

	Updated:2019 Oct 16 08:34 UTC
	>>more data<<


	Current 5-min:1.530e-1 /cm².sr.s
	24-hr Max:5.870e-1 /cm².sr.s

	Updated:2019 Oct 16 08:25 UTC
	>>more data<<


	Speed:372 km/sec
	Density:2.3 protons/cm³

	Updated:2019 Oct 16 08:31 UTC
	>>more data<<


	Current:Kp=2
	24-hr Max:Kp=2

	Updated:2019 Oct 16 06:00 UTC
	>>more data<<


	Current 5-min:2.690e+1 /cm².sr.s
	Integral Flux:7.917e+6 /cm².sr.day

	Updated:2019 Oct 16 08:25 UTC
	>>more data<<


	10.7cm Flux:67 sfu

	Update:2019 Oct 15 UTC
	>>more data<<


	SSN:0

	Update:2019 Oct 15 UTC
	>>more data<<