Перегляд архіву четвер, 1 жовтня 2015

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2015 Oct 01 1230 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

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

Сонячні протони

Warning condition (activity levels expected to increase, but no numeric forecast given)

	10 см потік	Ap
01 Oct 2015	120	011
02 Oct 2015	110	011
03 Oct 2015	110	006

Бюлетень

Solar flaring activity is gradually decreasing, with only one M1 (with peak at 13:20 UT) and eight C-class flares, mainly from NOAA active region 2422. NOAA 2422 is slightly decaying but still retains a complex magnetic configuration. NOAA 2427 has slightly grown, but did produce much activity. A series of CMEs were launched on September 30 of which at least two were related to a prominence eruption at the southwest limb. SDO/AIA and PROBA2/SWAP data indicate that solar material starts to lift late September 29/early morning September 30 and part of it falls back south and another part falls to the north. The southern part produces a CME with first measurement in LASCO/C2 at 10:00 UT and shortly after that the NW part produces a CME as well. These two CMEs visually merge later on. They mainly propagate to the West with a speed of 330 km/s (CACTus estimate), but it is not excluded that a glancing arrives at Earth late October 4. The CME activity did cause a rise in the proton flux (at >10MeV) to about 1pfu, though the flux values have not reached the event threshold. Proton flux values are gradually decreasing again. More C-class flares are expected, with a 25% chance for M-class flares.

The slow wind speed was low (with values around 300 km/s) till around 11 UT when the speed slightly increased to about 330 km/s. The phi angle has been varying from negative (towards) to positive (away) orientation. At 11 UT, the interplanetary magnetic field magnitude reached a peak of 10 nT. The geomagnetic conditions are quiet (K<3) to unsettled (K=3) and are mainly expected to remain so. There is a some chance for isolated time slots of active conditions (K=4).

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 092, за даними 20 станцій.

Сонячні індекси за 30 Sep 2015

Число Вольфа, Катанія	///
Сонячний потік 10 см	131
AK Chambon La Forêt	006
AK Wingst	003
Розрахунковий індекс Ap	002
Розрахункова міжнародна кількість сонячних плям	/// - За даними /// станцій

Зведення помітних подій

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

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