Het archief bekijken van zaterdag 29 mei 2021

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2021 May 29 1232 UTC

SIDC Prognose

Geldig van 1230 UTC, 29 May 2021 tot 31 May 2021
Zonnevlammen

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

Geomagnetisme

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

Proton Flux monitor

Warning condition (activity levels expected to increase, but no numeric forecast given)

10cm fluxAp
29 May 2021076012
30 May 2021076006
31 May 2021075004

Bulletin

Beta-gamma region NOAA 2824 has released four C flares during the past 24 hours. The brightest flare was a C9.4 flare peaking at 23:13 UT on May 28. This flare was associated with a dimming detected by Solar Demon and a CME towards the West first observed in LASCO C2 imagery at 23:12 UT. The chance for a C flare in the next 24 hours is estimated at 85%, while the chance for an M flare is estimated at 35%.

Analysis of LASCO C2 and COR2 A images suggests the CME mentioned above has a speed around 840 km/s and a half cone angle of about 50 degrees. There is a slight chance it will deliver a glancing blow to Earth, with estimated arrival time 13h UT on May 31.

A proton event started around 0h UT on May 29, related to the C9.4 flare and associated CME. The greater than 10 MeV proton flux reached a maximum of about 16 pfu around 03:20 UT. Proton flux levels went below the 10 pfu threshold around 05:50 UT and are decreasing further. The proton event is finished, but there is a chance for further proton events in the next 48 hours. The greater than 2 MeV electron flux was at nominal 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 fluence was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.

The solar wind speed as registered by DSCOVR varied between about 365 km/s and 460 km/s in the past 24 hours, with current values around 425 km/s. The Interplanetary Magnetic Field (IMF) was oriented away from the Sun and its magnitude varied between about 3 and 9 nT. Bz was never below -5 nT for extended intervals. Solar wind conditions are expected to gradually decline on May 29 and 30.

Quiet geomagnetic conditions (K Dourbes between 0 and 2; NOAA Kp between 0 and 1) were registered in the past 24 hours. Active geomagnetic intervals (K Dourbes = 4) are possible on May 29, with a slight chance for minor storm geomagnetic levels (K Dourbes = 5). Quiet to unsettled levels (K Dourbes < 4) are expected on May 30 and 31.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 012, gebaseerd op 21 stations.

Zon indexen voor 28 May 2021

Wolfgetal Catania///
10cm zonneflux077
AK Chambon La Forêt005
AK Wingst003
Geschatte Ap002
Geschat internationaal zonnevlekkengetal028 - Gebaseerd op 30 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
Geen

Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive

Alle tijden in UTC

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Op basis van de huidige parameters is er nu geen kans op poollicht in België en Nederland

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De snelheid van de zonnewind is gematigd hoog (536.6 km/sec.)
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C7.43

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