Перегляд архіву четвер, 11 травня 2023

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2023 May 11 1239 UTC

Прогноз SIDC

Сонячні спалахи

M-class flares expected (probability >=50%)

Геомагнетизм

Moderate (ISES: Major) magstorm expected (A>=50 or K=6)

Сонячні протони

Quiet

	10 см потік	Ap
11 May 2023	172	034
12 May 2023	170	029
13 May 2023	168	015

Бюлетень

Solar flaring activity was at moderate levels over the past 24 hours. The largest flares of the period were an M2.2 flare, peaking at 14:21 UTC May 10, from NOAA AR 3296 and another M2.2 flare, peaking at 09:01 UTC May 11, associated with NOAA AR 3294. The second of which was also associated with a Type II radio emission. NOAA AR 3296 remained the most active region on the disk, but simplified slightly. NOAA AR 3294 C-class flares were also produced by NOAA AR 3293 (which has now decayed into a plage region). NOAA AR 3297 also reduced in complexity. Two new small regions emerged in the eastern hemisphere both of which were quiet. The solar flaring activity is expected to be at moderate levels over the next 24 hours with M-class flares likely and a chance for X-class flares.

No new Earth directed Coronal Mass Ejections (CMEs) were detected in the available coronagraph imagery.

The greater than 10 MeV proton flux displayed a gradually decreasing trend and is now below the 10pfu threshold since around 04:00 UTC May 11. It is expected that the proton flux will be below this threshold for the next days. The greater than 2 MeV electron flux was below the 1000 pfu threshold and is expected to increase slightly but will likely remain below this threshold over the next days. The 24h electron fluence was at nominal levels and is expected to remain at nominal levels over the next 24 hours.

The solar wind conditions (ACE and DSCOVR) reflected the ongoing ICME passage. The solar wind speed gradually decreased from 690 km/s to 500 km/s. The total interplanetary magnetic field gradually decreased from 11 nT to 6nT. Bz had a minimum value of -4 nT. The interplanetary magnetic field was predominantly in the positive sector (directed away from the Sun). The solar wind conditions are expected to become enhanced again from late on May 11, due to the predicted arrival of the shock from the partial halo CME from May 09, possibly combined with the influence form a small positive coronal hole which began to traverse the central meridian on May 08.

The geomagnetic conditions reached minor storm conditions globally (NOAA KP = 5) and active conditions locally (K Bel = 4). Unsettled to active conditions are expected for the rest of May 11, with minor to moderate storm conditions possible from late on May 11 and on May 12, due to the expected arrival of the partial halo CME observed on May 09.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 159, за даними 12 станцій.

Сонячні індекси за 10 May 2023

Число Вольфа, Катанія	///
Сонячний потік 10 см	170
AK Chambon La Forêt	028
AK Wingst	027
Розрахунковий індекс Ap	027
Розрахункова міжнародна кількість сонячних плям	165 - За даними 18 станцій

Зведення помітних подій

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

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