Перегляд архіву понеділок, 9 серпня 2021

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2021 Aug 09 1236 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

Quiet (A<20 and K<4)

Сонячні протони

Quiet

	10 см потік	Ap
09 Aug 2021	074	010
10 Aug 2021	074	013
11 Aug 2021	074	005

Бюлетень

Over the past 24 hours, a C1.3 class flare has taken place, originating from Catania region 29. The solar activity is expected to remain at low levels, with a small change of C class flares over the next 24 hours.

No Earth-directed coronal mass ejections have been observed in the available coronagraphic imagery.

The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, while the 24h electron fluence was at nominal levels over the past 24 hours. They are expected to likely remain so during the next 24 hours.

Over the past 24 hours the solar wind speed fluctuated between 330 and 390 km/s. The total magnetic field strength had values between 1 and 8 nT, while its Bz component varied between -6 and 5 nT. The interplanetary magnetic field phi angle was predominantly on the positive sector (directed away from the Sun), until Aug 9 08:00UT when it switched to the negative sector. Over the next 24 hours, solar wind conditions could possibly be slightly enhanced, due to the expected high speed stream associated with the negative polarity coronal hole crossing central meridian Aug 5.

Geomagnetic conditions were at quiet to unsettled levels (NOAA Kp 1-2 and K Dourbes 1-3) over the past 24 hours. Quiet to active conditions are expected over the next 24 hours.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 010, за даними 20 станцій.

Сонячні індекси за 08 Aug 2021

Число Вольфа, Катанія	///
Сонячний потік 10 см	074
AK Chambon La Forêt	009
AK Wingst	006
Розрахунковий індекс Ap	005
Розрахункова міжнародна кількість сонячних плям	000 - За даними 24 станцій

Зведення помітних подій

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

Весь час у UTC

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