Het archief bekijken van dinsdag 25 juli 2023

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2023 Jul 25 1316 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Quiet

10cm fluxAp
25 Jul 2023166006
26 Jul 2023162011
27 Jul 2023155012

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity was moderate during the last 24 hours, with an M1 flare detected from NOAA Active Region (AR) 3376 (magnetic type Beta, Catania group 86) today 02:03 UTC. Most of the C-flaring activity came from NOAA AR 3373 (magnetic type Beta-Gamma, Catania group 81), while the brightest C-class flares came from NOAA AR 3380 (magnetic type Beta, Catania group 95), with two C3 flares today at 07:00 and 08:21 UTC. Further C-class flaring activity is expected, with a chance of an isolated M-class flare in the next 24 hours.

Coronale massa uitstoten

No Earth-directed Coronal Mass Ejections (CME) were observed in the last 24 hours. A halo CME can be seen in LASCO/SOHO coronograph data starting from yesterday 18:12 UTC, however this is a back- sided event.

Zonnewind

The Solar Wind (SW) conditions remain in a slow SW regime during the last 24 hours. The SW speed varied between 350 and 460 km/s in the last 24 hours. The total interplanetary magnetic field (Bt) varied between 3 and 7 nT and its North-South component (Bz) ranged between -6 and 6 nT. The interplanetary magnetic field phi angle was almost exclusively directed towards the Sun during the past 24 hours. A glancing blow from a Corona Mass Ejection (CME) is expected to arrive in the next 24 to 36 hours, however, it is not expected to have a major effect to the SW conditions.

Geomagnetisme

Geomagnetic conditions were both globally and locally unsettled for short periods (NOAA Kp 3- and K BEL 3) and for the rest of the time quiet (NOAA Kp 1 to 2+, K BEL 1 to 2) during the past 24 hours. They are expected to become unsettled to active in the next 24 hours.

Proton flux niveaus

A proton event was detected yesterday by the GOES-18 satellite lasting from 18:00 to 23:00 UTC. However, this event was weak and the 10 MeV proton flux reached but did not exceed the 1000 pfu threshold. The 10 MeV proton flux is expected to remain below the 1000 pfu threshold for the next 24 hours.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain below this threshold during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 136, gebaseerd op 17 stations.

Zon indexen voor 24 Jul 2023

Wolfgetal Catania158
10cm zonneflux165
AK Chambon La Forêt011
AK Wingst008
Geschatte Ap007
Geschat internationaal zonnevlekkengetal137 - Gebaseerd op 22 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
25013602030224N25W49M1.52N86/3376VI/2

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

Alle tijden in UTC

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