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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2014 Mar 15 1259 UTC

SIDC Forecast

Valid from 1230 UTC, 15 Mar 2014 until 17 Mar 2014
Brillamenti solari

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

Geomagnetism

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

Protoni solari

Quiet

10cm fluxAp
15 Mar 2014143005
16 Mar 2014143007
17 Mar 2014145007

Bulletin

There were five C flares on the Sun during the past 24 hours, released by NOAA AR 12003 and 12002. The brightest flare was a C5.0 flare produced by NOAA AR 12003 peaking at 09:40 UT on March 15. In the next 48 hours, the probability for C flares is high (90%) and for M flares around 35%, mainly from NOAA AR 12003 and 12002. In the past 24 hours, solar wind speed as observed by ACE decreased from about 450 km/s to about 400 km/s, while the magnitude of the Interplanetary Magnetic Field (IMF) dropped from about 8.5 to 4.5 nT. The effects of the coronal hole high speed stream have subsided. In the past 24 hours, quiet geomagnetic levels were registered (K Dourbes between 0 and 3; NOAA Kp between 1 and 2). Quiet geomagnetic conditions (K Dourbes < 4) are expected on March 15 and 16. Quiet to active conditions (K Dourbes < 5) are possible on March 17, due to a coronal hole high speed stream.

Today's estimated international sunspot number (ISN): 078, based on 11 stations.

Solar indices for 14 Mar 2014

Wolf number Catania///
10cm solar flux144
AK Chambon La Forêt010
AK Wingst005
Estimated Ap005
Estimated international sunspot number077 - Based on 32 stations

Noticeable events summary

DayBeginMaxFineLocStrengthOP10cmCatania/NOAARadio burst types
Nessuna

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

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