Prohlížíte si archiv středa 13. září 2017

Daily bulletin on solar and geomagnetic activity from the SIDC

Vydáno: 2017 Sep 13 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 13 Sep 2017 until 15 Sep 2017
Sluneční erupce

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

Geomagnetism

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

Sluneční protony

Proton event in progress (>10 MeV)

10cm fluxAp
13 Sep 2017077023
14 Sep 2017076015
15 Sep 2017075008

Bulletin

Strongest flare observed in the last 24 hours was the C1.6 flare (peaked at 19:20 UT on September 12), which originated from the Catania sunspot group 55 (NOAA AR 2680). The flare was, similarly to the C-class flare from this active region reported yesterday, associated with the EIT wave, coronal dimming, and rather slow and narrow CME (with projected speed of 350 km/s and angular width of about 100 degree). This CME will not arrive at the Earth. We might expect more isolated C-class flares in the coming hours (probability is about 25%), in particular from the Catania sunspot group 55 (NOAA AR 2680). The particle event, associated with the X8.2 flare is still on going, but the level of the proton fluxes is decreasing, and presently only fluxes with >10 MeV are slightly above the event threshold.

The sudden jump of the solar wind speed (up to maximum value of 650 km/s) and simultaneous increase of the density and interplanetary magnetic field magnitude (up to 16 nT) observed at about 19:26 UT on September 12 indicated arrival of the decayed CME-driven shock wave associated with the X8.2 flare observed on September 10. The shock was followed by the post- shock sheath region. The solar wind speed decreased rather fast and it is presently about 460 km/s.The interplanetary magnetic field magnitude is about 5 nT. The longer intervals of the southward Bz component and fast solar wind induced minor geomagnetic storm conditions starting at about 21:00 UT on September 12 and lasting until about 03 UT on September 13 (local station at Dourbes reported K=5 and NOAA reported Kp=5). The fast solar wind, associated with the low latitude coronal hole in the northern hemisphere which reached the central meridian on September 10, is expected to arrive at the Earth today. We expect quiet to active conditions within next 24 hours due to arrival of the fast solar wind.

Today's estimated international sunspot number (ISN): 018, based on 19 stations.

Solar indices for 12 Sep 2017

Wolf number Catania012
10cm solar flux076
AK Chambon La Forêt031
AK Wingst019
Estimated Ap021
Estimated international sunspot number012 - Based on 30 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-záblesk08. 04. 2025M1.5
Poslední geomagnetická bouře06. 04. 2025Kp5 (G1)
Dny bez skvrn
Poslední den bez skvrn08. 06. 2022
Průměrný měsíční počet slunečních skvrn
března 2025134.2 -20.4
dubna 2025141.4 +7.2
Posledních 30 dnů137.9 +0.4

Tento den v historii*

Sluneční erupce
12013M9.34
22024M5.47
32001M3.41
42000M1.63
52000M1.5
DstG
12001-271G4
21990-190G3
31978-114G4
41982-110G2
51959-88G1
*od roku 1994

Sociální sítě