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Denní bulletin o sluneční a geomagnetické aktivitě ze SIDC

Vydáno: 2026 Feb 27 1231 UTC

SIDC Předpověď

Sluneční erupce

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

Geomagnetismus

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

Sluneční protony

Quiet

	10cm tok	Ap
27 Feb 2026	131	012
28 Feb 2026	133	026
01 Mar 2026	135	023

Slunečně aktivní oblasti a vzplanutí

Solar flaring activity was low over the past 24 hours, with only C-class flares. The strongest flare was a C6.3 flare from the east limb (SIDC Flare 7084) peaking at 19:09 UTC on February 26. There are currently three numbered active regions on the solar disk. The most complex one is SIDC Sunspot Group 803 (NOAA Active Region 4380, magnetic type beta-gamma), which has rotated on disc from the east limb, in the southeast quadrant. The solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a chance for M-class flares.

Vyhazování koronální hmoty

No Earth-directed Coronal Mass Ejections (CMEs) were observed in the available coronagraph imagery in the last 24 hours.

Solární bouře

Over the past 24 hours, the solar wind parameters (ACE and DSCOVR) are gradually returning to the slow solar wind regime, under the waning influence of the high-speed stream from the recurrent, negative polarity, equatorial, coronal hole (SIDC Coronal Hole 147). The solar wind speed decreased from approximately 530 km/s to the current value of approximately 450 km/s. The interplanetary magnetic field values were between 3 nT and 6 nT. The Bz component varied between -4 nT and 3 nT. The interplanetary magnetic field angle was mostly in the negative sector. Enhanced solar wind conditions may be possible over the next 24 hours, due to the possible arrival of a glancing blow associated with the Coronal Mass Ejection (SIDC CME 607) observed at 07:00 UTC on February 25.

Geomagnetismus

Geomagnetic conditions globally were mostly at quiet to unsettled levels (NOAA Kp 2 to 3). Geomagnetic conditions locally were mostly at quiet to unsettled levels (K BEL 2 to 3), with an interval of active conditions (KBEL 4) between 19:00 UTC and 22:00 UTC on February 26. Active to minor storm conditions may be possible over the next 24 hours, due to the possible arrival of a glancing blow associated with the Coronal Mass Ejection (SIDC CME 607) observed at 07:00 UTC on February 25.

Úrovně protonového toku

The greater than 10 MeV proton flux was below the 10 pfu threshold level over the past 24 hours. It is expected to remain below the threshold level over the next 24 hours.

Elektronové toky na geostacionární oběžné dráze

The greater than 2 MeV electron flux measured by GOES 18 and GOES 19 was mostly above the 1000 pfu threshold in the last 24 hours. The greater than 2 MeV electron flux is expected to remain around the 1000 pfu threshold levels in the next 24 hours. The 24-hour electron fluence is presently at moderate levels and is expected to remain so over the next 24 hours.

Dnešní odhadovaný mezinárodní počet slunečních skvrn (ISN): 040, na základě 18 stanic.

Solární indexy za 26 Feb 2026

Wolfovo číslo Catania	040
10cm sluneční tok	130
AK Chambon La Forêt	021
AK Wingst	019
Odhadovaný Ap	020
Odhadovaný mezinárodní počet slunečních skvrn	033 - Na základě 29 stanic

Souhrn významných událostí

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

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