Перегляд архіву субота, 21 листопада 2020

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2020 Nov 21 1234 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

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

Сонячні протони

Quiet

	10 см потік	Ap
21 Nov 2020	083	006
22 Nov 2020	087	022
23 Nov 2020	089	019

Бюлетень

Solar activity was at low levels with two C-class flares registered in the past 24 hours. A C1 flare (peak at 18:44 UTC) was produced from an active region behind the east limb and a C1.9 flare with peak time at 17:03UTC on Nov 20th was produced by active region NOAA 2783 (Hsx/alpha). A new unnamed and unclassified active region has formed in the north-east quadrant, approximately at N32E35. The solar activity is expected to remain at low levels with a 50% chance for C-class flares and a slight chance for an M class flare. No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery.

The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux remained under the 1000 pfu threshold. The 24h electron fluence was at nominal levels. Enhancements of the > 2MeV electron flux and fluence are foreseen within the next 24 hours related to the expected arrival of a high speed stream originating from coronal hole CH 96.

Over the past 24 hours the solar wind speed was relatively stable with maximal velocity remaining below 390 km/s (ACE and DSCOVR). The total magnetic field reached a maximal strength of 7 nT with Bz component varying between -6 nT and 6 nT. The phi angle showed long periods in the positive sectors and is currently fluctuating between the positive and negative sectors.

Geomagnetic activity was globally quiet with a single locally unsettled period when K Dourbes registered 3. Quiet to active geomagnetic conditions are expected for the next 24 hours due to the foreseen arrival of a high speed stream (HSS) originating from coronal hole CH 96 by the morning of Nov. 22nd. With the arrival of the HSS there are slight chances for a minor geomagnetic storm.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 021, за даними 14 станцій.

Сонячні індекси за 20 Nov 2020

Число Вольфа, Катанія	011
Сонячний потік 10 см	082
AK Chambon La Forêt	009
AK Wingst	008
Розрахунковий індекс Ap	007
Розрахункова міжнародна кількість сонячних плям	010 - За даними 30 станцій

Зведення помітних подій

Надано Центром Аналізу Даних Сонячного Впливу (SIDC)© - SIDC - Оброблено SpaceWeatherLive

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