Prohlížíte si archiv čtvrtek 19. září 2024

Daily bulletin on solar and geomagnetic activity from the SIDC

Vydáno: 2024 Sep 19 1236 UTC

SIDC Forecast

Sluneční erupce

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

Geomagnetism

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

Sluneční protony

Quiet

10cm fluxAp
19 Sep 2024162016
20 Sep 2024164011
21 Sep 2024164014

Solar Active Regions and flaring

Solar flaring activity over the past 24 hours remained at low levels with background C-class flaring. There are seven numbered regions on the visible solar disc with NOAA AR 3825 (beta- gamma-delta) remaining the largest and most complex region. Most of the flaring activity was produced by NOAA AR 3824 (beta-gamma), which is now approaching the west limb, NOAA AR 3825 and NOAA AR 3829 (beta). The solar flaring activity is likely to be predominantly at low levels over the coming days with 50% chances of M-class flares and 15% chances for isolated X-class flaring.

Vyhazování koronální hmoty

No Earth-directed coronal mass ejections (CMEs) have been detected in the available coronagraph imagery over the past 24 hours.

Solární bouře

Over the past 24 hours the solar wind parameters (ACE and DSCOVR) were slightly perturbed. The interplanetary magnetic field reached 9.4 nT with Bz as low as - 8.8 nT. The solar wind velocity varied in the range of 375 km/s to 532 km/s. The B field phi angle remained predominantly in the positive sector (directed away from the Sun). The solar wind conditions are expected to continue to be slightly perturbed in the upcoming days under the possible influence of two mild high speed stream arrivals.

Geomagnetism

The geomagnetic conditions over the past 24 hours were predominantly quiet to active with an isolated minor geomagnetic storm registered by the global Kp index between 00:00 and 03:00 UTC on Sept 18th. Mostly quiet to active geomagnetic conditions with small chances for further isolated minor storms are expected over the next days.

Proton flux levels

Over the past 24 hours the greater than 10 MeV GOES proton flux has returned to nominal levels and is expected to remain so over the next 24 hours.

Electron fluxes at geostationary orbit

The greater than 2 MeV electron flux as measured by GOES 16 and GOES 18 was below the 1000 pfu threshold over the past 24 hours and is expected to remain so over the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so in the next 24 hours.

Today's estimated international sunspot number (ISN): 108, based on 23 stations.

Solar indices for 18 Sep 2024

Wolf number Catania///
10cm solar flux163
AK Chambon La Forêt019
AK Wingst012
Estimated Ap011
Estimated international sunspot number109 - Based on 24 stations

Noticeable events summary

DayBeginMaxKonecLocStrengthOP10cmCatania/NOAARadio burst types
Žádný

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

Všechny časy v UTC

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Fakta o počasí ve vesmíru

Poslední X-záblesk28. 03. 2025X1.1
Poslední M-záblesk08. 04. 2025M1.5
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Dny bez skvrn
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Průměrný měsíční počet slunečních skvrn
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Posledních 30 dnů137.9 +0.4

Tento den v historii*

Sluneční erupce
12013M9.34
22024M5.47
32001M3.41
42000M1.63
52000M1.5
DstG
12001-271G4
21990-190G3
31978-114G4
41982-110G2
51959-88G1
*od roku 1994

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