QRZ.RU EXPRESS от 11 февраля 2026

Опубликовано: 10 февраля 2026 в 1238 UTC
SIDC URSIGRAM 60210
Состояние солнечной активности на 10 февраля 2026, 1237UT
Прогноз SIDC
SOLAR FLARES : C-class flares expected, (probability >=50%)
Геомагнитное поле: Спокойное состояние (A<20 and K<4)
Солнечные протоны: Спокойное состояние
Прогноз на 10 февраля 2026: Солнечный поток в диапазоне 10см: 133 / AP-индекс: 008
Прогноз на 11 февраля 2026: Солнечный поток в диапазоне 10см: 129 / AP-индекс: 012
Прогноз на 12 февраля 2026: Солнечный поток в диапазоне 10см: 124 / AP-индекс: 011
Комментарий (на английском языке): Solar Active Regions and flaring: Solar flaring activity was low over the past 24 hours, with only C-class flares identified. The largest flare was a C9.2 flare (SIDC Flare 6999) peaking on February 09 at 23:02 UTC, which was produced by SIDC Sunspot Group 762 (NOAA Active Regions 4342, 4374). A total of 8 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 784 (NOAA Active Region 4366) is the largest region on disk, the most magnetically complex (Beta-Gamma-Delta) and produced most of the flaring activity in the last 24 hours. This region is rotating over the western limb off the visible solar disk. 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. Coronal mass ejections: No Earth directed CMEs were observed in the past 24 hours. Solar wind: Slow solar wind conditions were recorded over the past 24 hours. The solar wind speed ranged from 360 km/s to 474km /s. The total interplanetary magnetic field ranged from 5 to 9 nT, with the Bz reaching a minimum of -7 nT. The phi-angle was mainly in the negative sector (directed towards the Sun), with periods in the positive sector. In the next 24 hours, a slow solar wind regime is expected. Geomagnetism: The geomagnetic conditions were quiet globally (Kp 1-2) and quiet to unsettled locally (K BEL 1-3) in the last 24 hours. Quiet to unsettled conditions are expected in the next 24 hours. Proton flux levels: The greater than 10 MeV GOES proton flux was at background levels and is expected to remain at background levels over the next 24 hours. Electron fluxes at GEO: The greater than 2 MeV electron flux, as measured by the GOES-19 satellite was above the 1000 pfu threshold between 12:55 UTC and 19:15 UTC on February 09. The 2 MeV electron flux is expected to cross the threshold again during the next 24 hour. The 24-hour electron fluence was at moderate levels and is expected to remain at moderate levels over the next 24 hours.Сегодняшнее значение числа солнечных пятен (International Sunspot Number): 113,
получено на основе анализа результатов 03 станций наблюдения.
Солнечные индексы за 09 Feb 2026
Число Вольфа по данным обсерватории Катания (IT9): 156
Солнечный поток в диапазоне 10см: 144
A-индекс по данным обсерватории Chambon-la-Foret (F): 012
A-индекс по данным обсерватории Wingst (DL): 008
Планетарный А-индекс Ap: 007
Вчерашнее значение числа солнечных пятен (International Sunspot Number): 117,
получено на основе анализа результатов 10 станций наблюдения.
Прошедшие события на Солнце:
DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES
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