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Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2025 Jul 27 1231 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

Quiet (A<20 and K<4)

Сонячні протони

Quiet

	10 см потік	Ap
27 Jul 2025	142	008
28 Jul 2025	141	008
29 Jul 2025	140	011

Сонячно-активні області та спалахи

Solar flaring activity was low over the past 24 hours, with only C-class flares. The strongest flare was a C3.3 flare (SIDC Flare 4949) peaking at 14:25 UTC on July 26, which was associated with SIDC Sunspot Group 576 (NOAA Active Region 4160, magnetic type alpha). There are currently eight numbered active regions on the solar disk. SIDC Sunspot Groups 564, 570, 572 (NOAA Active Regions 4149, 4153, 4155) are the most complex Groups with magnetic type beta. SIDC Sunspot Group 575 (NOAA Active Region 4159) has decayed into a plage region. SIDC Sunspot Group 571 (NOAA Active Region 4158) has rotated over the west limb. The solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a chance for M-class flares.

Корональні викиди маси

No Earth-directed Coronal Mass Ejections (CMEs) were observed in the available coronagraph imagery in the last 24 hours.

Корональні діри

A mid-latitude, negative polarity coronal hole (SIDC Coronal Hole 121) continues to cross the central meridian since June 26. An associated high-speed stream may arrive at Earth starting from July 29.

Сонячний вітер

Over the past 24 hours, the solar wind parameters (ACE) were initially enhanced, under the waning influence of the high-speed stream from the negative polarity coronal hole (SIDC Coronal Hole 116) and a possible, but less certain, ICME arrival associated with the Coronal Mass Ejection (SIDC CME 530) that lifted off around 08:00 UTC on July 23. Solar wind parameters are gradually returning to a slow solar wind regime. Solar wind speed values have decreased from around 570 km/s to around 430 km/s. The interplanetary magnetic field values were between 7 nT and 11 nT. The Bz component varied between -9 nT and 10 nT. The interplanetary magnetic field angle phi was in the negative sector until around 16:30 UTC on July 26, when it flipped to the positive sector. Mostly slow solar wind conditions are expected over the next 24 hours.

Геомагнетизм

Geomagnetic conditions globally were mostly at quiet to unsettled levels (NOAA Kp 1 to 3) and reached active levels (NOAA Kp 4) between 15:00 UTC and 18:00 UTC on July 26, due to a possible, but less certain, ICME arrival associated with Coronal Mass Ejection (SIDC CME 530) observed around 08:00 UTC on July 23. Geomagnetic conditions locally were mostly at quiet to unsettled levels (K BEL 1 to 3) and reached active levels (K BEL 4) between 12:00 UTC and 14:00 UTC and between 17:00 UTC and 20:00 UTC on July 26. Mostly quiet conditions, with possible unsettled intervals (NOAA Kp 1 to 3, K BEL 1 to 3), are expected globally and locally over the next 24 hours.

Рівні потоку протонів

The greater than 10 MeV proton flux was below the 10 pfu threshold level over the past 24 hours. It is expected to remain below the threshold level over the next 24 hours.

Потоки електронів на геостаціонарній орбіті

Over the past 24 hours, the greater than 2 MeV electron flux measured by GOES 19 was above the 1000 pfu threshold until around 20:00 UTC on July 26, when it fell below the threshold. The greater than 2 MeV electron flux measured by GOES 18 exceeded the 1000 pfu threshold between 15:30 UTC on July 26 and 03:00 UTC on July 27 and remained below the threshold for the rest of the last 24 hours. The greater than 2 MeV electron flux is expected to remain around the 1000 pfu threshold levels in the next 24 hours. The 24-hour electron fluence is presently at moderate levels and is expected to remain so over the next 24 hours.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 130, за даними 12 станцій.

Сонячні індекси за 26 Jul 2025

Число Вольфа, Катанія	///
Сонячний потік 10 см	143
AK Chambon La Forêt	018
AK Wingst	017
Розрахунковий індекс Ap	015
Розрахункова міжнародна кількість сонячних плям	153 - За даними 17 станцій

Зведення помітних подій

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

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