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Daily bulletin on solar and geomagnetic activity from the SIDC

Emesso: 2014 Jul 01 1236 UTC

SIDC Forecast

Brillamenti solari

Active (M-class flares expected, probability >=50%)

Geomagnetism

Quiet (A<20 and K<4)

Protoni solari

Quiet

	10cm flux	Ap
01 Jul 2014	152	005
02 Jul 2014	160	003
03 Jul 2014	165	003

Bulletin

The strongest flare during the last 24 hours was an M1.4 flare peaking on 1 July at 11:23UT and originating from filamentary activity between small sunspot regions NOAA 2102 and 2106. Most of the C-class flares also originated from NOAA 2106. NOAA 2104 and 2107 are the largest and magnetically most complex sunspot regions, but produced only one C-class flare each, the strongest a C6.6 peaking at 07:37UT this morning and having its source in NOAA 2107. No coronagraphic images are available yet to evaluate any of the CMEs that may be associated to the recent flaring activity. The other CMEs had their source on the Sun's farside or were directed away from Earth. There's a good chance for further M-class flaring. Solar wind speed hovered around 350 km/s while Bz oscillated between -5 and +5 nT. Quiet geomagnetic conditions were observed and are expected to remain so.

Today's estimated international sunspot number (ISN): 101, based on 18 stations.

Solar indices for 30 Jun 2014

Wolf number Catania	///
10cm solar flux	141
AK Chambon La Forêt	009
AK Wingst	008
Estimated Ap	008
Estimated international sunspot number	/// - Based on /// stations

Noticeable events summary

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

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