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Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2021 Oct 19 1243 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
19 Oct 2021	077	014
20 Oct 2021	078	017
21 Oct 2021	080	008

Бюлетень

Solar activity was at very low levels. NOAA Active Region (AR) 2886 (Catania sunspot region 64) has rotated further onto the disk and has a simple magnetic configuration (Alpha). The small sunspot (Catania sunspot region 63) that emerged yesterday has since decayed. 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 (DSCOVR) showed an enhancement in the Interplanetary Magnetic Field (IMF) over the past 24 hours. The total magnetic field reached a maximum value of 12 nT. The Bz varied between -8 and +10 nT. The solar wind speed ranged between 340 km/s and 390 km/s. The solar wind speed and magnetic field are expected to be enhanced on Oct 19 and 20, due to the influence of the High Speed Stream (HSS) associated with the with the small positive Coronal Hole (CH) and subsequently the larger 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 and 1-3, respectively) over the past 24 hours. Geomagnetic conditions are expected to be unsettled to active on Oct 19 to 20, due to the arrival of the aforementioned HSS.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 010, за даними 07 станцій.

Сонячні індекси за 18 Oct 2021

Число Вольфа, Катанія	023
Сонячний потік 10 см	///
AK Chambon La Forêt	///
AK Wingst	///
Розрахунковий індекс Ap	///
Розрахункова міжнародна кількість сонячних плям	016 - За даними 24 станцій

Зведення помітних подій

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

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