QRZ.RU EXPRESS от 14 января 2026

Опубликовано: 13 января 2026 в 1231 UTC
SIDC URSIGRAM 60113
Состояние солнечной активности на 13 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 13 января 2026: Солнечный поток в диапазоне 10см: 113 / AP-индекс: 023
Прогноз на 14 января 2026: Солнечный поток в диапазоне 10см: 114 / AP-индекс: 012
Прогноз на 15 января 2026: Солнечный поток в диапазоне 10см: 114 / AP-индекс: 007
Комментарий (на английском языке): Solar Active Regions and flaring: Solar flaring activity was low over the past 24 hours. The largest flare was a C1.9 flare peaking on January 13 at 10:18 UTC, originated from a region from behind the east limb. A total of 3 numbered sunspot groups are currently on the disk, all having alpha or beta magnetic configuration. 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 CME detected in LASCO C2 data on JAN 12 2026 05:48 UTC, directed to the north east, is back sided and is not expected to impact Earth. Solar wind: Fast solar wind conditions were recorded over the past 24 hours. The solar wind velocity varied between 520 to 590 km/s. The interplanetary magnetic field was around 8nT, with the Bz reaching a minimum value of -6 nT. Solar wind conditions are expected to remain elevated due to the continuation of the high-speed streams from negative polarity coronal holes (SIDC Coronal Hole 137 and SIDC Coronal Hole 142). Geomagnetism: Geomagnetic conditions reached active levels globally and locally (Kp 4, K bel 4) between Jan 12 21:00 UTC and Jan 13 03:00 UTC. Mostly unsettled to active geomagnetic conditions are expected over the next day due to the ongoing high speed stream. 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 was above the 1000 pfu threshold for the past 24 hours and is expected to remain so in the upcoming days. The 24h electron fluence was at moderate level and is expected to remain so in the next days.Сегодняшнее значение числа солнечных пятен (International Sunspot Number): 048,
получено на основе анализа результатов 06 станций наблюдения.
Солнечные индексы за 12 Jan 2026
Число Вольфа по данным обсерватории Катания (IT9): 044
Солнечный поток в диапазоне 10см: 113
A-индекс по данным обсерватории Chambon-la-Foret (F): 032
A-индекс по данным обсерватории Wingst (DL): 021
Планетарный А-индекс Ap: 023
Вчерашнее значение числа солнечных пятен (International Sunspot Number): 056,
получено на основе анализа результатов 12 станций наблюдения.
Прошедшие события на Солнце:
DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES
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