Viewing archive of Monday, 4 February 2013

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2013 Feb 04 1228 UTC

SIDC Forecast

Valid from 1230 UTC, 04 Feb 2013 until 06 Feb 2013
Solar flares

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

Geomagnetism

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

Solar protons

Quiet

10cm fluxAp
04 Feb 2013114005
05 Feb 2013115012
06 Feb 2013115013

Bulletin

Four C-class flares were detected during the past 24 hours, and the strongest one was C8.4 flare peaking at 06:10 UT, on February 3. The C-class flares are possible, in particular from the Catania sunspot group 79 (NOAA AR 1667). The interplanetary magnetic field magnitude is about 5 nT. The Earth is currently under the influence of a slow solar wind with the speed of 350 km/s. The low-latitude coronal hole in the northern hemisphere has passed the central meridian and we expect arrival of the fast solar wind late on February 5. We expect quiet to possibly active geomagnetic conditions in the next 48 hours.

Today's estimated international sunspot number (ISN): 022, based on 07 stations.

Solar indices for 3 Feb 2013

Wolf number Catania///
10cm solar flux111
AK Chambon La Forêt008
AK Wingst006
Estimated Ap005
Estimated international sunspot number053 - Based on 15 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmRadio burst typesCatania/NOAA
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

Arkhangelsk, Vorkuta
The direction of the interplanetary magnetic field is slightly South (-6.4nT).

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