Prohlížíte si archiv čtvrtek 2. března 2023

Daily bulletin on solar and geomagnetic activity from the SIDC

Vydáno: 2023 Mar 02 1241 UTC

SIDC Forecast

Valid from 1230 UTC, 02 Mar 2023 until 04 Mar 2023
Sluneční erupce

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

Geomagnetism

Quiet (A<20 and K<4)

Sluneční protony

Quiet

10cm fluxAp
02 Mar 2023162006
03 Mar 2023162007
04 Mar 2023162007

Bulletin

The solar flaring activity was at low levels over the past 24 hours. The larger flare was a C9.2-class flare peaking at 04:50 UTC on February 02 occurring in the most complex region on disc, NOAA active region 3234 (with a magnetic complexity of beta-gamma-delta). The other region on the disc did not show any significant flaring activity. The flaring activity over the next 24 hours is expected to remain mostly at low levels with C-class flares and with some possibility of an M-class flare.

Several coronal mass ejections and flows were observed in the currently available SOHO/LASCO coronagraph imagery and automatically detected by the Cactus tool over the past 24 hours. No clear Earth-directed coronal mass ejections were identified.

The greater than 10 MeV protons flux was at the background levels over the past 24 hours. The proton flux is expected to be at the background levels over the next day. The greater than 2 MeV electron flux crossed the 1000 pfu threshold and is expected to remain elevated over the next days due to the enhanced solar wind conditions in the past days. The 24-hour electron fluence was at moderate levels and is expected to remind at moderate levels over the next 24 hours.

An equatorial coronal hole of negative polarity is currently transiting the central meridian. It is expected to enhance the solar wind conditions near Earth starting in about 3 days, starting on February 5.

The solar wind environment near Earth slowly returned to nominal values over the past 24 hours: The wind speed steadily decreased from 600 km/s to 480 km/s. The total interplanetary magnetic was below 7 nT, and the southward interplanetary magnetic component, Bz, fluctuated between -4 nT and 7 nT. The solar wind condition is expected to continue its decrease over the next 24 hours.

The geomagnetic conditions were quiet and is expected to remain quiet.

Today's estimated international sunspot number (ISN): 098, based on 15 stations.

Solar indices for 01 Mar 2023

Wolf number Catania///
10cm solar flux162
AK Chambon La Forêt011
AK Wingst009
Estimated Ap010
Estimated international sunspot number092 - Based on 28 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

<< 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-záblesk15. 04. 2025M1.2
Poslední geomagnetická bouře16. 04. 2025Kp8- (G4)
Dny bez skvrn
Poslední den bez skvrn08. 06. 2022
Průměrný měsíční počet slunečních skvrn
března 2025134.2 -20.4
dubna 2025120.5 -13.7
Posledních 30 dnů118.3 -22.1

Tento den v historii*

Sluneční erupce
12014X1.05
22016M9.63
32024M2.2
42022M1.9
52024M1.6
DstG
11965-162G4
22002-127G3
32001-114G3
41990-95G1
51957-89G2
*od roku 1994

Sociální sítě