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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2024 Jan 13 1231 UTC

SIDC Předpověď

Sluneční erupce

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

Geomagnetismus

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

Sluneční protony

Quiet

	10cm tok	Ap
13 Jan 2024	180	008
14 Jan 2024	182	011
15 Jan 2024	182	007

Slunečně aktivní oblasti a vzplanutí

Solar flaring activity over the past 24 hours was at low levels. The largest flare was a C4.8-flare, with peak time at 17:22 UTC on January 12, associated with NOAA AR 3538 (beyond the west limb). There are currently 12 numbered active regions on the visible disk. Since yesterday, two active regions have rotated away over the west limb, four new active regions have been numbered in the eastern hemisphere, and one new active region has emerged in the south-west quadrant of the solar disk. NOAA AR 3541 (beta-gamma) is the most magnetically complex region on the disk, and together with NOAA AR 3538, NOAA AR 3539 (beta), NOAA AR 3548 (beta), and NOAA AR 3549 (beta), has produced most of the flaring activity in the past 24 hours. The solar flaring activity is likely to be at moderate levels over the coming days with C-class flares expected and M-class flares probable.

Vyhazování koronální hmoty

Based on currently available coronagraph images, a partial halo coronal mass ejection (CME), with angular width of about 120 degrees and directed towards the south-east, first appeared in SOHO/LASCO coronagraphs around 22:12 UTC on January 12. The plane-of-the-sky speed of the CME was around 700 km/s. The CME was associated with a filament eruption, observed at 22:00 UTC in SDO/AIA 304 near the south-east limb of the solar disk. No clear Earth-directed component has been identified. However, further analysis is on-going.

Koronální díra

A small mid-latitude coronal hole in the northern hemisphere (with positive magnetic polarity) started crossing the central meridian around 18:00 UTC on January 12. The associated high speed solar wind stream may reach Earth no earlier than January 15.

Solární bouře

Slow solar wind conditions were recorded over the past 24 hours. The solar wind speed as measured by DSCOVR ranged between 470 km/s and 500 km/s, while ACE data was unavailable at this time. The total interplanetary magnetic field fluctuated between 1 nT and 5 nT, with the Bz (north-south) component reaching a minimum value of -3 nT. The phi-angle transitioned from the negative (towards the Sun) to the positive sector (away from the Sun) around 14:53 UTC on January 12, and has remained mainly positive ever since. In the next 24 hours, we expect similar slow solar wind conditions, with a chance of disturbed conditions due to the possible arrival of the coronal mass ejection (CME) first observed on January 09 around 01:25 UTC.

Geomagnetismus

The geomagnetic conditions over the past 24 hours were globally and locally quiet (Kp 2 and K Bel 2). Due to the possible arrival of a coronal mass ejection from January 09, unsettled conditions with short periods of active conditions are possible in the next 24 hours.

Úrovně protonového toku

The greater than 10 MeV proton flux is at background level, and is expected to remain at background level in the past 24 hours. Due to the number of complex regions currently on the disk, however, we cannot exclude the possibility of new proton events in the next 24 hours

Elektronové toky na geostacionární oběžné dráze

The greater than 2 MeV GOES 16 electron flux was below the 1000 pfu threshold and is expected to remain so in the next 24 hours. The 24h electron fluence was at nominal level and is expected to remain so in the next 24 hours.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 150, na základě 04 stanic.

Solární indexy za 12 Jan 2024

Wolfovo číslo Catania	///
10cm sluneční tok	186
AK Chambon La Forêt	005
AK Wingst	003
Odhadovaný Ap	002
Odhadovaný mezinárodní počet slunečních skvrn	192 - Na základě 12 stanic

Souhrn významných událostí

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

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