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Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2024 Apr 22 1245 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
22 Apr 2024	212	007
23 Apr 2024	212	008
24 Apr 2024	212	010

Сонячно-активні області та спалахи

Solar flaring activity was at moderate levels in the past 24 hours with background high C-class flaring and multiple M-class flares. There are around 19 numbered active regions on the visible solar disc with NOAA AR 3639 (beta-gamma), NOAA AR 3645 (beta- gamma) and NOAA AR 3647 (beta-delta) being the largest and most complex ones. The strongest activity was an impulsive M3.4 flare with start time 21:44 UTC, end time 21:57 UTC and peak time 21:52 UTC on April 21st produced by NOAA AR 3638 (beta-gamma). This region was responsible for most of the moderate flaring activity. Isolated low M-class flaring was produced by NOAA AR 3645, which has grown in size and complexity. NOAA AR 3647 (beta-delta) has exhibited further growth and produced multiple C-class flaring. NOAA AR 3655 (beta) produced isolated low flaring activity. The remaining active regions are relatively simple simple (magnetic type alpha or beta) and did not show any significant flaring activity. The solar flaring activity is expected to remain at moderate levels over the next days with likely further M-class flaring and small chance for X-class flaring.

Корональні викиди маси

No Earth-directed coronal mass ejections (CMEs) have been detected in the available coronagraph imagery over the past 24 hours. A Type II radio burst with estimated velocity of 278 km/s was observed at 22:09 UTC on April 21st, possibly related to the M3.4 flaring produced by NOAA AR 3638. No Earth-directed CME is currently associated to this event. A filament eruption to the east of the central meridian and might be associate with a narrow southward CME. Current analysis suggests no impact on Earth.

Корональні діри

An equatorial positive polarity coronal hole is currently residing on the central meridian. The high speed stream emanating from it might arrive to Earth on April 25th.

Сонячний вітер

Over the past 24 hours the solar wind parameters (ACE and DSCOVR) have recovered from the waning influence of a previous ICME arrival. The solar wind velocity was in the range of 377 km/s to 539 km/s. The interplanetary magnetic field was slightly elevated, reaching a maximum 7.69 nT with a minimum Bz of -6.23 nT. The B field phi angle was predominantly in the negative sector (directed towards the Sun). The solar wind conditions are expected to remain at slow solar wind conditions in the next hours with possible elevations from a mild high speed stream arrival from a negative polarity coronal hole or any potential ICME arrival later on April 22-23rd. Further mild high speed stream from a positive polarity coronal hole might arrive to Earth on April 25th - April 26th.

Геомагнетизм

The geomagnetic conditions over the past 24 hours were quiet to active. Mostly quiet to unsettled geomagnetic conditions are expected throughout April 22nd and 23rd with possible isolated active conditions and less likely minor storm levels pending an expected high speed stream arrival from a negative polarity coronal hole or any potential glancing blow ICME arrival from the multiple CMEs reported over last week.

Рівні потоку протонів

Over the past 24 hours the greater than 10 MeV GOES proton flux was at background levels and is expected to continue so over the next days, pending any fast eruptive solar activity.

Потоки електронів на геостаціонарній орбіті

The greater than 2 MeV GOES 16 electron flux as measured by GOES 16 was below the 1000 pfu threshold and is expected to remain so in the upcoming days. The greater than 2 MeV GOES 16 electron flux as measured by GOES 18 briefly exceeded 1000 pfu threshold around 17 UTC and midnight UTC on April 21st. The greater than 2 MeV GOES 16 electron flux as measured by GOES 18 might briefly cross the 1000 pfu threshold again in the next 24 hours. The 24h electron fluence was at nominal level and is expected to remain so in the next days.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 269, за даними 10 станцій.

Сонячні індекси за 21 Apr 2024

Число Вольфа, Катанія	///
Сонячний потік 10 см	///
AK Chambon La Forêt	///
AK Wingst	///
Розрахунковий індекс Ap	///
Розрахункова міжнародна кількість сонячних плям	222 - За даними 22 станцій

Зведення помітних подій

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

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