Arşiv Perşembe, 6 Haziran 2024 görüntüleniyor

SIDC'den güneş ve jeomanyetik aktivite hakkında günlük bülten

Yayınlandı: 2024 Jun 06 1231 UTC

SIDC Tahmini

Güneş patlamaları

M-class flares expected (probability >=50%)

Jeomanyetizma

Quiet (A<20 and K<4)

Güneş protonları

Quiet

	10cm akı	Ap
06 Jun 2024	195	007
07 Jun 2024	193	007
08 Jun 2024	193	016

Güneş Aktif Bölgeleri ve parlama

Solar flaring activity was low over the past 24 hours. The largest flare was a C9.5-flare, with peak time 00:14 UTC on June 06 from beyond the east limb. There are currently 12 numbered active regions on the visible disk. NOAA AR 3697 is the most complex AR (beta-gamma-delta) but only produced C-class flaring in the last 24 hours. The solar flaring activity is expected to be at moderate levels over the coming day with C-class flares expected and M-class flares likely and a chance of X-class flares.

Koronal Kütle Atılımı

No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images. The CME of June 04 05:12 UTC has been further analyzed and is not believed to have an earth directed component.

Güneş rüzgarı

The solar wind at the Earth was slow, with speeds up to 430 km/s and interplanetary magnetic field around 6nT and Bz reaching minimum value of -5nT. The possible arrival of high-speed stream from the coronal hole that crossed the central meridian late June 04 is expected on June 08.

Jeomanyetizma

Geomagnetic conditions were quiet to unsettled both globally and locally (NOAA Kp 3-, Local K Bel 2). Geomagnetic conditions are expected to remain quiet to unsettled in the next 24h, and may reach active levels on June 08 due to a high speed stream arrival.

Proton akı seviyeleri

Over the past 24 hours, the greater than 10 MeV GOES proton flux remained below the 10 pfu threshold and is expected to remain so over the next day. There is a slight chance that the proton flux may increase due to strong flaring from NOAA AR 3697.

Jeostatik yörüngedeki elektron akıları

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

Bugünün tahmini uluslararası güneş lekesi sayısı (ISN): 1 Tahmini gunes lekesi sayisi, 2 Istasyon sayisi.

05 Jun 2024 için güneş endeksleri

Kurt numarası Catania	///
10cm güneş akısı	195
AK Chambon La Forêt	014
AK Wingst	008
Tahmini Ap	009
Tahmini uluslararası güneş lekesi sayısı	182 - 24 istasyonlarına göre

Dikkat çeken olayların özeti

Güneş Etkileri Veri Analiz Merkezi tarafından sağlanmıştır© - SIDC - SpaceWeatherLive tarafından işlendi

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