Viewing archive of Sunday, 12 January 2014

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2014 Jan 12 1245 UTC

SIDC Forecast

Valid from 1230 UTC, 12 Jan 2014 until 14 Jan 2014
Solar flares

Eruptive (C-class flares expected, probability >=50%)

Geomagnetism

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

Solar protons

Warning condition (activity levels expected to increase, but no numeric forecast given)

10cm fluxAp
12 Jan 2014160016
13 Jan 2014150012
14 Jan 2014150004

Bulletin

In total 8 C flares occurred during the past 24 hours. A C6.5 and C6.0 flare were the strongest events. Both erupted from Catania sunspot group 98 (NOAA AR 1944). Also Catania sunspot group 9 (NOAA AR 1950) was responsible for two C flares. More C flares are expected within the next 48 hours with a chance of 90%. Chances for M flares are estimated at 40% and for X flares at 10%. We issue a warning condition for a proton event, due to position of NOAA AR 1944 which is rotating towards the west limb. No geo-effective CMEs were observed. The solar wind, measured by ACE, showed signatures of the arrival of the coronal hole high speed stream. Solar wind speed increased from about 400 km/s to 500 km/s. The magnitude of the interplanetary magnetic field reached a maximum of 9 nT and the Bz component varied between +8 and -8 nT. Geomagnetic conditions were quiet to unsettled. Quiet to active conditions are expected during the next 24 hours.

Today's estimated international sunspot number (ISN): 098, based on 18 stations.

Solar indices for 11 Jan 2014

Wolf number Catania///
10cm solar flux166
AK Chambon La Forêt009
AK Wingst004
Estimated Ap004
Estimated international sunspot number102 - Based on 21 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 moderate possibility for aurora to appear at the following high latitude regions in the near future

Rovaniemi, Sodankylä
Murmansk
Kiruna, Luleå

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

Tórshavn
Oulu, Kuopio
Bergen, Trondheim
Arkhangelsk
Sundsvall, Umeå

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

Tampere
Petrozavodsk
The direction of the interplanetary magnetic field is slightly South (-6.08nT).

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