Prohlížíte si archiv pondělí 30. září 2024

Daily bulletin on solar and geomagnetic activity from the SIDC

Vydáno: 2024 Sep 30 1259 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
30 Sep 2024200011
01 Oct 2024200011
02 Oct 2024199007

Solar Active Regions and flaring

The solar flaring activity was at moderate level during the last 24 hours, with few C-class flares and three M-class flares. The strongest flare was GOES M1.8 flare from NOAA active region (AR) 3842 which peaked at 14:24 UTC on Sep 29. During the flare, the source region (AR 3842) of the flare had beta-gamma configuration of its photospheric magnetic field. NOAA AR 3842 is the most complex region on the disk (beta-gamma-delta magnetic field configuration). The solar flaring activity is expected to be at low to moderate levels over the next 24 hours, possibly with few M-class flares and a small chance for X-class flares.

Vyhazování koronální hmoty

Presently available observations indicate a coronal mass ejection (CME) on the East limb, which was first observed on SOHO/LASCO coronograph images starting around 03:12 UTC on Sep 30 (detected by CACTUS tool), with an angular width of about 104 deg. This CME was having the source region close to the East limb, although very faint on- disk CME signatures are also observed. Accordingly, glancing blow related to this shock could be expected, with a very low probability, on Oct 03. No other Earth-directed CMEs were detected in the available coronagraph observations during the last 24 hour.

Solární bouře

Over the past 24 hours, the solar wind parameters were disturbed under the influence of high speed streams (HSSs) from the negative polarity coronal hole which crossed the central meridian on Sep 26. The solar wind speed ranged between 310 km/s to 530 km/s. The North- South component (Bz) ranged between -12 and 13 nT. The interplanetary magnetic field ranged from 2 nT to 15 nT. In the next 24 hours, we expect a gradual transition from fast to slow solar wind.

Geomagnetism

Geomagnetic conditions were globally and locally at quiet to active conditions (NOAA Kp and K BEL 1 to 4), due to the arrival of high speed sptream from the coronal hole which crossed the central meridian on Sep 26. Quiet to active conditions are expected in the next 24 hours.

Proton flux levels

The greater than 10 MeV GOES proton flux was below the threshold level over the past 24 hours. It is expected to remain so during the next 24 hours.

Electron fluxes at geostationary orbit

The greater than 2 MeV electron flux, as measured by the GOES-16 satellite, was below the threshold level over the past 24 hours and is expected to remain so in the coming 24 hours. The 24h electron fluence is presently at normal level, and it is expected to remain so in the next 24 hours.

Today's estimated international sunspot number (ISN): 177, based on 11 stations.

Solar indices for 29 Sep 2024

Wolf number Catania///
10cm solar flux197
AK Chambon La Forêt019
AK Wingst016
Estimated Ap017
Estimated international sunspot number159 - Based on 23 stations

Noticeable events summary

DayBeginMaxKonecLocStrengthOP10cmCatania/NOAARadio burst types
29124912531258S11E25M1.0SF--/----
29140914241431S15E51M1.71F--/3842III/1
29143114411446----M1.7--/3842

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

Všechny časy v UTC

<< Přejít na stránku s denním přehledem

Poslední zprávy

Podpora SpaceWeatherLive.com!

Mnoho lidí přichází do SpaceWeatherLive, aby sledovali aktivitu Slunce nebo pokud je vidět polární záři, ale s větším provozem přicházejí i vyšší náklady na server. Zvažte dar, pokud vás baví SpaceWeatherLive, abychom mohli udržovat web online!

Darovat SpaceWeatherLive Pro
Podpořte naše zboží SpaceWeatherLive
Podívejte se na naše zboží

Fakta o počasí ve vesmíru

Poslední X-záblesk28. 03. 2025X1.1
Poslední M-záblesk05. 04. 2025M1.0
Poslední geomagnetická bouře06. 04. 2025Kp5 (G1)
Dny bez skvrn
Poslední den bez skvrn08. 06. 2022
Průměrný měsíční počet slunečních skvrn
března 2025134.2 -20.4
dubna 2025148.7 +14.5
Posledních 30 dnů132.7 -9.9

Tento den v historii*

Sluneční erupce
12006M1.39
22002M1.38
31997C9.01
42002C8.7
52002C6.29
DstG
12000-292G4
21995-149G4
31977-95G3
41989-85G1
51960-76G1
*od roku 1994

Sociální sítě