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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2014 Apr 20 1445 UTC

SIDC Předpověď

Sluneční erupce

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

Geomagnetismus

Minor storm expected (A>=30 or K=5)

Sluneční protony

Warning condition (activity levels expected to increase, but no numeric forecast given)

	10cm tok	Ap
20 Apr 2014	169	028
21 Apr 2014	172	012
22 Apr 2014	173	005

Bulletin

Twelve active regions were reported by NOAA today. Three of them (NOAA ARs 2034, 2035, and 2036) have beta-gamma configuration of the photospheric magnetic field. These three active regions and four others were responsible for numerous C-class flares yesterday and today. None of them was associated with an Earth-directed CME. The strongest flare of the past 24 hours was the C6.4 flare peaking at 08:13 UT today in the NOAA AR 2032 at the west solar limb. We expect further flaring activity on the C-level, with a good chance for an M-class event. After the arrival of the shock produced by the halo CME on April 18 (see below), the proton flux at energies above 10 MeV decreased to values below the threshold of the proton event. The proton flux, however, remains high, and in case of another solar eruption with associated SEPs, the event threshold could be easily crossed. We therefore issue a warning condition for a proton event. An interplanetary shock-like structure was detected this morning. ACE recorded jumps of solar wind speed, temperature, and the interplanetary magnetic filed (IMF) magnitude at 10:23 UT. SOHO/CELIAS detected a jump in density at 10:22 UT, but the jump in speed was detected only 20 to 30 minutes later. Therefore, this discontinuity does not seem to be a typical ICME- driven fast forward shock as ACE did not detect a jump in density at all, and jumps in density and the solar wind speed detected by SOHO/CELIAS were not simultaneous. There is, however, very little doubt that this is a start of an ICME corresponding to the halo CME observed on the Sun on April 18. During the intervals of the strongest IMF magnitude in the post-shock solar wind flow (up to 22 nT), the north-south IMF component Bz was either northward or close to zero. Unsettled geomagnetic conditions (K = 3) were reported by Dourbes and NOAA, and active conditions (K = 4) were reported by IZMIRAN. Currently the IMF magnitude is around 12 nT and the solar wind speed is around 650 km/s, so minor geomagnetic storm conditions (K = 5) are still possible.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 138, na základě 17 stanic.

Solární indexy za 19 Apr 2014

Wolfovo číslo Catania	///
10cm sluneční tok	169
AK Chambon La Forêt	///
AK Wingst	014
Odhadovaný Ap	014
Odhadovaný mezinárodní počet slunečních skvrn	129 - Na základě 16 stanic

Souhrn významných událostí

Poskytuje Centrum pro analýzu dat o solárních vlivech© - SIDC - Zpracováno SpaceWeatherLive

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