Viewing archive of Sunday, 9 February 2014

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2014 Feb 09 1455 UTC

SIDC Forecast

Valid from 1230 UTC, 09 Feb 2014 until 11 Feb 2014
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

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

10cm fluxAp
09 Feb 2014168014
10 Feb 2014164005
11 Feb 2014160006

Bulletin

The solar flaring activity continues to decrease. The strongest flare of the past 24 hours was the C8.6 flare peaking yesterday at 18:33 UT in the Catania sunspot group 28 (NOAA AR 1967). All other flares did not reach the C3 level. Catania sunspot groups 27 and 28 (NOAA ARs 1968 and 1967 respectively) are currently situated at the west solar limb, maintaining respectively beta-gamma and beta-gamma-delta configurations of the photospheric magnetic field. Due to position of these groups at the west limb, a major CME in one of them may lead to a proton event, so we maintain the warning condition. We expect flaring activity to continue on the C-level, with an isolated M-class flare being unlikely. The Earth is now exiting the trailing part of the ICME that followed the shock arrival on February 7. The ICME triggered active (K = 4) to minor storm (K = 5) conditions according to IZMIRAN and NOAA respectively. The solar wind speed is currently around 420 km/s, and the interplanetary magnetic field magnitude is around 8 nT. We expect quiet geomagnetic conditions, with isolated intervals of active conditions (K = 4) being possible but unlikely.

Today's estimated international sunspot number (ISN): 106, based on 09 stations.

Solar indices for 08 Feb 2014

Wolf number Catania///
10cm solar flux172
AK Chambon La Forêt037
AK Wingst027
Estimated Ap027
Estimated international sunspot number099 - Based on 12 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

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

Oulu, Kuopio
Trondheim
Arkhangelsk, Vorkuta
Luleå, 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 (-6.65nT).

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