Перегляд архіву середа, 24 травня 2023

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2023 May 24 1232 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

Quiet (A<20 and K<4)

Сонячні протони

Quiet

	10 см потік	Ap
24 May 2023	154	010
25 May 2023	148	020
26 May 2023	146	015

Сонячно-активні області та спалахи

Solar flaring activity over the past 24 hours remained at moderate levels with a single low M-class flare, namely an impulsive M1.0 with peak time 09:58 UTC on May 24th produced by NOAA AR 3311 (beta-gamma-delta). This region was the main driver for the flaring activity and previously produced an impulsive M3.1 flare with peak time 12:13 UTC on May 23rd. It remains the most complex region on the visible solar disc and has significantly increased its number of trailing spots. Isolated C-class flaring was produced by NOAA AR 3305 from behind the west limb, by plage region NOAA 3314 and by a rotating region at the east limb. NOAA AR 3310 (beta) is the second largest region on the visible disc, which has also some increment in the number of trailing spots. Nevertheless the region remained quiet. The new active region in the south-east quadrant, NOAA 3315 (beta), has been silent. The solar flaring activity is expected to remain at low to moderate levels over the next days with chances for an isolated X-class flaring from NOAA AR 3311.

Корональні викиди маси

A fast full halo coronal mass ejection (CME) was observed in the LASCO/C2 chronograph imagery at 10:24 UTC on May 23rd. A type IV fast radio burst emission was first detected at 11:20 UTC the same day. The CME appears back-sided, possibly related to activity from an active region behind the east limb. No impact on Earth is expected. No other Earth-directed CMEs have been detected in the available coronagraph imagery.

Сонячний вітер

Over the past 24 hours the solar wind parameters (ACE and DSCOVR) Solar wind parameters reflected the continuous influence of a high speed stream (HSS) from a negative polarity coronal hole. The solar wind velocity varied in the range of 503 km/s to 636 km/s. The interplanetary magnetic field was weak with a maximum value of 5.6 nT and a minimum Bz of -5.3 nT. The B field was predominantly in the negative sector (directed towards the Sun). The solar wind conditions are expected to remain elevated over the next days with the ongoing HSS passage and possible glancing blow arrival late on May 25th and May 26th.

Геомагнетизм

The geomagnetic conditions over the past 24 hours were quiet to active. Mostly quiet to active geomagnetic conditions are expected over the next 24 hours with remaining chances for isolated minor storms under the ongoing high speed stream influence and due to a possible glancing blow ICME passage late on May 25th and May 26th.

Рівні потоку протонів

Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so with possible enhancements in case of increased levels of solar activity over the next days

Потоки електронів на геостаціонарній орбіті

The greater than 2 MeV electron flux has crossed the 1000 pfu threshold for prolonged periods of time. The greater than 2 MeV electron flux is expected to remain at that enhanced levels in the upcoming days. The 24h electron fluence was at the border of nominal levels to moderate levels and is expected to be at moderate levels over the next days.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 140, за даними 16 станцій.

Сонячні індекси за 23 May 2023

Число Вольфа, Катанія	156
Сонячний потік 10 см	155
AK Chambon La Forêt	019
AK Wingst	016
Розрахунковий індекс Ap	015
Розрахункова міжнародна кількість сонячних плям	123 - За даними 24 станцій

Зведення помітних подій

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

Весь час у UTC

<< На сторінку денного огляду