Перегляд архіву середа, 20 жовтня 2021

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2021 Oct 20 1231 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

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

Сонячні протони

Quiet

	10 см потік	Ap
20 Oct 2021	076	010
21 Oct 2021	076	011
22 Oct 2021	077	006

Бюлетень

Solar activity was at very low levels. NOAA Active Region (AR) 2886 (Catania sunspot region 64) remained stable. A small region of flux emergence was observed to develop near N23E63. Solar activity is expected to be very low over the next 24 hours with a slight probability of C-class flares from NOAA AR 2866.

No Earth directed CMEs have been detected in the available coronagraph imagery.

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain below this level during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.

The solar wind speed (DSCOVR) ranged between 340 and 430 km/s. The total magnetic field reached a maximum value of 10 nT at the beginning of the period, before then decreasing to around 5 nT. The Bz varied between -8 and +8 nT. The interplanetary magnetic field phi angle was predominantly in the negative sector (directed towards from the Sun). The solar wind speed and magnetic field are expected to continue to be slightly enhanced on Oct 20 and 21, due to the influence of the High Speed Stream (HSS) associated with the with the negative polarity extension of the southern polar CH which began to cross the central meridian on Oct 16.

Geomagnetic conditions reached active levels (NOAA Kp and local K Dourbes recorded values of 1-4) over the past 24 hours. Geomagnetic conditions are expected to be unsettled to active on Oct 20 and 21, due to the influence of the aforementioned HSS and returning to quiet to levels from Oct 22.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 011, за даними 14 станцій.

Сонячні індекси за 19 Oct 2021

Число Вольфа, Катанія	011
Сонячний потік 10 см	076
AK Chambon La Forêt	020
AK Wingst	017
Розрахунковий індекс Ap	016
Розрахункова міжнародна кількість сонячних плям	011 - За даними 18 станцій

Зведення помітних подій

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

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