Viewing archive of Tuesday, 7 February 2017

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2017 Feb 07 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 07 Feb 2017 until 09 Feb 2017
Solar flares

Quiet conditions (<50% probability of C-class flares)

Geomagnetism

Active conditions expected (A>=20 or K=4)

Solar protons

Quiet

10cm fluxAp
07 Feb 2017073017
08 Feb 2017075019
09 Feb 2017077017

Bulletin

NOAA AR 2634 evolved into a beta magnetic field configuration and is the only visible active region on the solar disk. There have been no C-class flares in past 24 h. C-class flares are possible.

No Earth directed Coronal Mass Ejections (CMEs) have been detected. Solar protons have remained at background levels over the past 24 h.

Geomagnetic conditions have reached K=4 overnight due to the longlasting effect of a fading high speed stream (HSS) with speeds between 550 and 600 km/s. Solar wind speed is now at 500 km/s with interplanetary magnetic fields of 4 nT. Another HSS from a small equatorial positive polarity coronal is expected to affect the Earth within 24 h. Geomagnetic conditions up to K = 5 can be expected.

Today's estimated international sunspot number (ISN): 012, based on 08 stations.

Solar indices for 06 Feb 2017

Wolf number Catania///
10cm solar flux073
AK Chambon La Forêt022
AK Wingst015
Estimated Ap015
Estimated international sunspot number012 - Based on 20 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
None

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

All times in UTC

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Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Gillam, MB, Iqaluit, NU
Nuuk
Reykjavik
The direction of the interplanetary magnetic field is slightly South (-6.61nT).
The maximum X-ray flux of the past two hours is:
C6.12

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