Viewing archive of Monday, 6 October 2014

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2014 Oct 06 1246 UTC

SIDC Forecast

Valid from 1230 UTC, 06 Oct 2014 until 08 Oct 2014
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
06 Oct 2014129008
07 Oct 2014126010
08 Oct 2014127006

Bulletin

Solar activity is low. The strongest flare reported during last 24 hours was the C1.5 flare with the peak time at 16:56 UT, on October 05. The flare originated from the Catania sunspot group 63 (NOAA AR 2177) currently situated close to the west solar limb. No Earth-directed CMEs were observed during last 24 hours. We expect C-class flares. An isolated M-class flare from the Catania sunspot group 64 (NOAA AR 2181) which has beta-gamma configuration of its photospheric magnetic field, is possible but not very probable. The solar wind speed is currently 400 km/s and the interplanetary magnetic field magnitude is about 4nT. The geomagnetic conditions are quiet and expected to remain so in the following 48 hours.

Today's estimated international sunspot number (ISN): 050, based on 09 stations.

Solar indices for 05 Oct 2014

Wolf number Catania///
10cm solar flux128
AK Chambon La Forêt012
AK Wingst006
Estimated Ap005
Estimated international sunspot number067 - Based on 15 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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