Prohlížíte si archiv úterý 6. dubna 2021

Daily bulletin on solar and geomagnetic activity from the SIDC

Vydáno: 2021 Apr 06 1233 UTC

SIDC Forecast

Valid from 1230 UTC, 06 Apr 2021 until 08 Apr 2021
Sluneční erupce

Quiet conditions (<50% probability of C-class flares)

Geomagnetism

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

Sluneční protony

Quiet

10cm fluxAp
06 Apr 2021072008
07 Apr 2021072006
08 Apr 2021072005

Bulletin

The solar activity has been very low over the past 24 hours. Active Region NOAA 12813 (Mag. type:Axx) is further decaying, with a smaller, spotless, region present in the South-Eastern part of the visible disk. The solar activity is expected to remain at low levels over the next 24 hours.

No Earth-directed coronal mass ejections were observed in the available coronagraph imagery.

The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold. It is expected to remain so during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.

The solar wind speed has fluctuated between 300 and 345 km/s over the past 24 hours. The total magnetic field strength has fluctuated between 3 nT and 9 nT. The Bz component decreased sharply to about -7 nT around April 5 09:30UT, smoothly increasing for the rest of the 24-hour window. The interplanetary magnetic field phi angle was predominantly in the positive sector (directed away from the Sun). The values recorded for the solar wind parameters indicate the possible passage of a magnetic cloud, starting around April 5 09:30UT. We are therefore anticipating the influence from the high speed stream associated with the southern positive Coronal Hole, which was on Central Meridian on April 3, over the next 24 hours. As a response, over the next 24 hours the solar wind parameters are expected to increase.

Geomagnetic conditions were mostly at quiet levels with isolated unsettled periods (NOAA Kp 0-3 and local K Dourbes 0-2) over the past 24 hours. Quiet to unsettled conditions are expected for the next 24-hour period, with a very slight chance of active conditions, due to the arrival of the aforementioned high-speed stream.

Today's estimated international sunspot number (ISN): 006, based on 27 stations.

Solar indices for 05 Apr 2021

Wolf number Catania///
10cm solar flux072
AK Chambon La Forêt007
AK Wingst004
Estimated Ap004
Estimated international sunspot number011 - Based on 25 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-záblesk18. 04. 2025M4.4
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 2025120.1 -14.1
Posledních 30 dnů116.4 -25.9

Tento den v historii*

Sluneční erupce
12022M3.7
22001M2.91
32024M2.1
42022M1.67
52021M1.1
DstG
12002-126G3
22024-117G3
31957-111G3
41977-91G2
51981-81G2
*od roku 1994

Sociální sítě