QRZ.RU EXPRESS от 13 января 2026

Опубликовано: 12 января 2026 в 1231 UTC
SIDC URSIGRAM 60112
Состояние солнечной активности на 12 января 2026, 1230UT
Прогноз SIDC
SOLAR FLARES : C-class flares expected, (probability >=50%)
Геомагнитное поле: Возмущенное (A>=20, K=4)
Солнечные протоны: Спокойное состояние
Прогноз на 12 января 2026: Солнечный поток в диапазоне 10см: 112 / AP-индекс: 022
Прогноз на 13 января 2026: Солнечный поток в диапазоне 10см: 114 / AP-индекс: 031
Прогноз на 14 января 2026: Солнечный поток в диапазоне 10см: 114 / AP-индекс: 012
Комментарий (на английском языке): Solar Active Regions and flaring: Solar flaring activity was moderate over the past 24 hours. The largest flare was a M3.3 flare (SIDC Flare 6631) peaking on January 11 at 23:14 UTC, originated from a region from behind the east limb. A total of 4 numbered sunspot groups are currently on the disk, all having alpha or beta magnetic configuration and have produced only C-class flaring. 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 new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images. The halo CME detected in SOHO/LASCO-C2 data from 23:36 UTC 11 JAN 2026, is backsided and not expected to arrive to the Earth. Solar wind: Solar wind conditions were slightly elevated with speeds around 540 km/s. The interplanetary magnetic field was around 10nT, with the Bz reaching a minimum value of -10 nT. Solar wind conditions are expected to remain slightly elevated due to the ongoing ICME passage, and the possible arrival of high-speed streams from negative polarity coronal holes (SIDC Coronal Hole 137 and SIDC Coronal Hole 142). Geomagnetism: Geomagnetic conditions reached minor storm levels globally and locally (Kp 5, K5) between 12:00 and 21:00 UTC on January 11 Mostly unsettled to active geomagnetic conditions are expected over the next day due to the ongoing ICME passage and possible HSS arrival. Proton flux levels: The greater than 10 MeV proton flux remained below the 10 pfu threshold and is expected to remain so over the next days. Electron fluxes at GEO: The greater than 2 MeV electron flux exceeded slightly the 1000 pfu threshold on 11 JAN between 21:35 UTC and 12 JAN 01:30 UTC and is currently slightly above the threshold since 10:45 UTC. The greater than 2 MeV electron flux is expected to have short crossings over the 1000 pfu threshold over the next 24 hours. The electron fluence was at normal levels and is expected to be at normal levels over the next 24 hours.Сегодняшнее значение числа солнечных пятен (International Sunspot Number): 049,
получено на основе анализа результатов 08 станций наблюдения.
Солнечные индексы за 11 Jan 2026
Число Вольфа по данным обсерватории Катания (IT9): ///
Солнечный поток в диапазоне 10см: 111
A-индекс по данным обсерватории Chambon-la-Foret (F): 047
A-индекс по данным обсерватории Wingst (DL): 032
Планетарный А-индекс Ap: 035
Вчерашнее значение числа солнечных пятен (International Sunspot Number): 065,
получено на основе анализа результатов 15 станций наблюдения.
Прошедшие события на Солнце:
DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES
11 2153 2314 0031 ////// M3.3 ///////