Space Environment Prediction Center





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	Cosmic Ray
	Station K Indices
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	Coronal Hole Index
	Solar Active Regions
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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. There was no active region on the visible disk, without C-class and above flare produced. The solar wind speed maintained at about 340 km/s. The geomagnetic field was quiet to unsettled.
	Published:	2018-07-17 00:18 UTC
	Forecaster:	035/012

Within the next three days, solar activity is expected to be very low. The geomagnetic field will be quiet to unsettled.
	Published:	2018-07-17 00:18 UTC
	Forecaster:	035/012

During last week, solar activity was at very low to low levels. There was no active region on the visible disk, with only one C1.6 flare produced from eastward limb on 6 July. The F10.7 index ranged from 72 sfu to 73 sfu. Due to the continous effect of the coronal hole high speed stream, the solar wind speed reached a peak of 524 km/s on 7 Jul. The geomagnetic field was at quiet to unsettled levels.
	Published:	2018-07-13 03:57 UTC
	Forecaster:	010/029

Within the next week, solar activity is expected to be mainly very low. Due to the effect of the coronal hole high speed stream, the geomagnetic field is expected to reach active levels on 15 Jul. It will be quiet to unsettled for the rest of time.
	Published:	2018-07-13 03:57 UTC
	Forecaster:	010/029

ALERTS


	No space environment alerts have been issued today.


	19:00 UTC 05 Jul 2018	00:15 UTC 04 Jul 2018	01:15 UTC 03 Jul 2018	01:15 UTC 02 Jul 2018	01:15 UTC 01 Jul 2018

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:A4.1
	Peak Time:2018 Jul 16 18:19 UTC

	Updated:2018 Jul 17 15:27 UTC
	>>more data<<


	Current 5-min:3.260e-1 /cm².sr.s
	24-hr Max:5.440e-1 /cm².sr.s

	Updated:2018 Jul 17 15:20 UTC
	>>more data<<


	Speed:446 km/sec
	Density:6.4 protons/cm³

	Updated:2018 Jul 17 15:22 UTC
	>>more data<<


	Current:Kp=2
	24-hr Max:Kp=3

	Updated:2018 Jul 17 12:00 UTC
	>>more data<<


	Current 5-min:3.840e+0 /cm².sr.s
	Integral Flux:3.806e+5 /cm².sr.day

	Updated:2018 Jul 17 15:20 UTC
	>>more data<<


	10.7cm Flux:72 sfu

	Update:2018 Jul 16 UTC
	>>more data<<


	SSN:0

	Update:2018 Jul 16 UTC
	>>more data<<