Перегляд архіву понеділок, 21 червня 2021

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2021 Jun 21 1301 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
21 Jun 2021	077	003
22 Jun 2021	080	005
23 Jun 2021	085	006

Бюлетень

Solar activity has been very low over the past 24 hours. Catania region 7 (NOAA AR 12833) is rotating on the western solar hemisphere. Two active regions (NOAA AR 12830 and NOAA AR 12831) are about to rotate on the visible disk. The solar activity is expected to remain at low levels over the next 24 hours.

No Earth-directed coronal mass ejections were 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 above the 1000 pfu alert threshold, were it is expected to remain during the next 24 hours. The 24h electron fluence was at moderate levels and is expected to remain at those levels over the next 24 hours.

The solar wind speed slightly decreased from 432 to 345 km/s over the past 24 hours. The total magnetic field strength fluctuated between 3 and 6 nT. The values of the Bz component varied between -4 and +3 nT. The interplanetary magnetic field phi angle was predominantly on the negative sector (directed towards the Sun). Any effects from the high speed stream from the extention of the northern negative polarity Coronal Hole (CH) or the southern positive CH could be expected, but possibly not in the next 24 hours.

Geomagnetic conditions were at quiet to unsettled levels (NOAA Kp 0-3) over the past 24 hours. Quiet conditions are expected over the next 24 hours.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 013, за даними 15 станцій.

Сонячні індекси за 20 Jun 2021

Число Вольфа, Катанія	///
Сонячний потік 10 см	076
AK Chambon La Forêt	009
AK Wingst	006
Розрахунковий індекс Ap	005
Розрахункова міжнародна кількість сонячних плям	014 - За даними 27 станцій

Зведення помітних подій

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

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