Viewing archive of Tuesday, 24 February 2015

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2015 Feb 24 1259 UTC

SIDC Forecast

Valid from 1230 UTC, 24 Feb 2015 until 26 Feb 2015
Solar flares

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

Geomagnetism

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

Solar protons

Quiet

10cm fluxAp
24 Feb 2015117028
25 Feb 2015117015
26 Feb 2015117007

Bulletin

Solar activity has been low. A C1.4 flare was detected today peaking at 10:57 UT, related to a filament eruption on the southeast limb of the Sun. No coroagraph data is available yet to observe an associated CME. The visible active regions have simple magnetic configuration (beta) and are not expected to produce more than C-class flaring. An active region rotating now over the east limb may increase activity levels in the coming hours. Geomagnetic activity reached active levels locally (K at Dourbes = 4, with Kp reaching 5) due to the fast solar wind from a coronal hole. Unsettled to active conditions can be expected in the next 24h.

Today's estimated international sunspot number (ISN): 037, based on 07 stations.

Solar indices for 23 Feb 2015

Wolf number Catania///
10cm solar flux117
AK Chambon La Forêt048
AK Wingst018
Estimated Ap020
Estimated international sunspot number038 - Based on 18 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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