Viewing archive of Sunday, 18 August 2013

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2013 Aug 18 1225 UTC

SIDC Forecast

Valid from 1230 UTC, 18 Aug 2013 until 20 Aug 2013
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
18 Aug 2013123007
19 Aug 2013120007
20 Aug 2013120012

Bulletin

NOAA AR 1818 produced a complex eruptive event on August 17, resulting in two M flares within one hour: a M3.3 peaking at 1824 UT and a M1.4 peaking at 1933 UT. This complex event was associated with a fast CME (~1000 km/s as seen from COR2 A). The bulk of the CME appears to go essentially westwards, with respect to the Earth, but we might cross the eastern flank of this CME on the second half of August 20. The 10 MeV proton flux rose slightly but didn't reach the event threshold. Flaring activity is expected to remain at eruptive levels for the next 48 hours, with C class flares likely from NOAA ARs 1818 and 1824, and a slight risk of an isolated M class flare from AR 1818. We expect essentially quiet geomagnetic conditions for the next 48 hours. There is a small chance of periods of enhanced activity (unsettled to active) on the second half of August 20, due to the CME of August 17.

Today's estimated international sunspot number (ISN): 074, based on 10 stations.

Solar indices for 17 Aug 2013

Wolf number Catania///
10cm solar flux125
AK Chambon La Forêt011
AK Wingst008
Estimated Ap008
Estimated international sunspot number071 - Based on 18 stations

Noticeable events summary

17 1816 1824 1835 ////// M3.3 B 110 ///1818 17 1849 1933 1954 ////// M1.4 150 ///1818 I/2 1I/2V/1
DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types

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

Norilsk, Vorkuta

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

Arkhangelsk

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

Surgut, Syktyvkar
The solar wind speed is currently moderately high (530.3 km/sec.)
The direction of the interplanetary magnetic field is slightly South (-5.06nT).

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