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Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2025 May 22 1231 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

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

Сонячні протони

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

	10 см потік	Ap
22 May 2025	120	010
23 May 2025	121	030
24 May 2025	122	008

Сонячно-активні області та спалахи

Solar flaring activity over the last 24 hours has been low, with only one C-class flare. The strongest flare was a C2.6 flare (SIDC Flare 4431) peaking at 18:07 UTC on May 21, associated with SIDC Sunspot Group 504 (NOAA Active Region 4095, magnetic type beta- gamma). There are currently eight numbered active regions on the solar disk. The most complex one is SIDC Sunspot Group 504 (NOAA Active Region 4095). SIDC Sunspot Group 497 (NOAA Active Region 4089) has decayed into plage. SIDC Sunspot Group 505 (magnetic type beta) has rotated on disk from the east limb, in the southeast quadrant. The solar flaring activity is expected to be low to moderate over the next 24 hours, with C-class flares expected and a chance for M-class flares.

Корональні викиди маси

A Coronal Mass Ejection (CME), SIDC CME 503, was observed in LASCO/C2 coronagraph imagery around 14:06 UTC on May 21, propagating to the west. It is likely a backsided event and it is not expected to impact Earth. A filament eruption was observed in SDO/AIA 304 data around 18:45 UTC on May 21, near SIDC Sunspot Group 502 (NOAA Active Region 4094). No associated CME was observed in the available coronagraph imagery. No other Earth-directed CMEs were observed in the available coronagraph imagery.

Корональні діри

A northern, equatorial, positive polarity coronal hole (SIDC Coronal Hole 115) is crossing the central meridian. An associated, mild high-speed stream may arrive at Earth starting from May 25. The elongated, mid-latitude, positive polarity coronal hole (SIDC Coronal Hole 104) continues to cross the central meridian since May 15.

Сонячний вітер

The solar wind conditions (ACE and DSCOVR) were enhanced during the past 24 hours, most likely due to the continuous influence of a high- speed stream from the southern, positive polarity coronal hole (SIDC Coronal Hole 104). The solar wind speed decreased from around 620 km/s to around 515 km/s. The interplanetary magnetic field values ranged from 4 nT to 9 nT. The Bz component ranged between -3 nT and 6 nT. The interplanetary magnetic field angle phi was predominantly in the positive sector. Further enhancements in the solar wind conditions may be expected over the next 24 hours, due to the possible arrival of a glancing blow associated with the Coronal Mass Ejection observed around 00:24 UTC on May 19 (SIDC CME 500), and the continuous influence of the high-speed stream from the southern, positive polarity coronal hole (SIDC Coronal Hole 104).

Геомагнетизм

Geomagnetic conditions globally were quiet levels (NOAA Kp 1+ to 2+) over the past 24 hours. Geomagnetic conditions locally were at quiet levels (K BEL 2) over the past 24 hours. Active to minor storm conditions, with a chance for isolated moderate storm intervals (NOAA Kp 4 to 6) are expected over the next 24 hours due to the possible arrival of a glancing blow associated with the Coronal Mass Ejection observed around 00:24 UTC on May 19 (SIDC CME 500), and the continuous influence of the high-speed stream from the southern, positive polarity coronal hole (SIDC Coronal Hole 104).

Рівні потоку протонів

The greater than 10 MeV proton flux was below the 10 pfu threshold over the past 24 hours. It is expected to remain below the threshold level over the next 24 hours, pending no further eruptive activity from SIDC Sunspot Group 504 (NOAA Active Region 4095, magnetic type beta-gamma).

Потоки електронів на геостаціонарній орбіті

The greater than 2 MeV electron flux measured by GOES 18 was over the 1000 pfu threshold between 17:00 UTC and 23:30 UTC on May 21. The greater than 2 MeV electron flux measured by GOES 19 was close to the 1000 pfu threshold but remained below it in the past 24 hours. The greater than 2 MeV electron flux is expected to be above the 1000 pfu threshold over the next 24 hours. The 24-hour electron fluence is presently at normal levels and is expected to remain so over the next 24 hours.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 103, за даними 15 станцій.

Сонячні індекси за 21 May 2025

Число Вольфа, Катанія	///
Сонячний потік 10 см	119
AK Chambon La Forêt	014
AK Wingst	014
Розрахунковий індекс Ap	016
Розрахункова міжнародна кількість сонячних плям	098 - За даними 26 станцій

Зведення помітних подій

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

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