Prohlížíte si archiv čtvrtek 18. ledna 2024

Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2024 Jan 18 1232 UTC

SIDC Předpověď

Sluneční erupce

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

Geomagnetismus

Quiet (A<20 and K<4)

Sluneční protony

Quiet

	10cm tok	Ap
18 Jan 2024	174	007
19 Jan 2024	174	007
20 Jan 2024	174	007

Slunečně aktivní oblasti a vzplanutí

Solar flaring activity over the past 24 hours was at low levels. The C5.4-class flare was the larger flare and was produced by the bipolar NOAA Active Region 3553 (magnetic complexity beta). NOAA Active Region 3555 is currently the most complex region with a magnetic complexity beta-gamma, but does not show any significant flaring activity. The solar flaring activity is likely to be at low levels over the coming days with C-class flares and possible M-class flares.

Vyhazování koronální hmoty

Based on currently available coronagraph images several coronal mass ejections (CMEs) were observed. No Earth directed coronal mass ejections have been identified in the last 24 hours.

Koronální díra

The small midlatitude coronal hole in the northern hemisphere (with positive magnetic polarity) is now on the solar meridian. It’s a high-speed stream may impact the solar condition near Earth in 2-3 days.

Solární bouře

Slow solar wind conditions were recorded over the past 24 hours. The solar wind speed as measured by DSCOVR ranged between 300 km/s and 500 km/s. The total interplanetary magnetic field was below 7 nT, and the Bz (north-south) component fluctuating between -6 nT and 5 nT. Slow solar wind conditions are expected for the next 24 hours.

Geomagnetismus

The geomagnetic conditions over the past 24 hours were quiet (NOAA-Kp and K-Bel 1-2). Mostly quiet conditions are expected in the next 24 hours.

Úrovně protonového toku

The greater than 10 MeV protons flux where at background levels. It is expected to be at background levels in the next 24 hours.

Elektronové toky na geostacionární oběžné dráze

The greater than 2 MeV GOES 16 electron flux was below the 1000 pfu threshold and is expected to remain so in the next 24 hours. The 24h electron fluence was at nominal level and is expected to remain so in the next 24 hours.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 128, na základě 14 stanic.

Solární indexy za 17 Jan 2024

Wolfovo číslo Catania	///
10cm sluneční tok	174
AK Chambon La Forêt	007
AK Wingst	004
Odhadovaný Ap	002
Odhadovaný mezinárodní počet slunečních skvrn	143 - Na základě 09 stanic

Souhrn významných událostí

Poskytuje Centrum pro analýzu dat o solárních vlivech© - SIDC - Zpracováno SpaceWeatherLive

Všechny časy v UTC

<< Přejít na stránku s denním přehledem