QRZ.RU EXPRESS от 17 января 2026

Опубликовано: 16 января 2026 в 1231 UTC
SIDC URSIGRAM 60116
Состояние солнечной активности на 16 января 2026, 1230UT
Прогноз SIDC
Солнечные вспышки. Ожидаются вспышки класса M (вероятность >=50%)
Геомагнитное поле: Спокойное состояние (A<20 and K<4)
Солнечные протоны: Спокойное состояние
Прогноз на 16 января 2026: Солнечный поток в диапазоне 10см: 140 / AP-индекс: 017
Прогноз на 17 января 2026: Солнечный поток в диапазоне 10см: 144 / AP-индекс: 012
Прогноз на 18 января 2026: Солнечный поток в диапазоне 10см: 150 / AP-индекс: 010
Комментарий (на английском языке): Solar Active Regions and flaring: Solar flaring activity was low over the past 24 hours with only C-class flares. The largest flare was a C6.6 flare peaking on January 16 at 09:09 UTC, originated from SIDC Sunspot Group 766 (NOAA Active Region 4345). SIDC Sunspot Group 740 (NOAA Active Region 4341) is the most complex active region (Beta-Gamma-Delta). Solar activity is expected to be moderate over the next 24 hours, with C-class flares expected and M-class flares likely. Coronal mass ejections: No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images. Coronal holes: SIDC Coronal Hole 146 (a large equatorial coronal hole with a positive polarity) has reached the central meridian. High Speed Stream from this coronal hole is expected to impact earth late on the 18th of Januari. Solar wind: Fast solar wind conditions were recorded over the past 24 hours. The solar wind velocity reached 700 km/s, but is currently gradually reducing to 588 km/s. The interplanetary magnetic field reached 13 nT, with the Bz reaching a minimum value of -10 nT. Solar wind conditions are expected to remain enhanced over the next 24 hours. Geomagnetism: Over the past 24 hours geomagnetic conditions were mainly unsettled both locally and globally (Kp3, Kbel 3) but with a isolated active period globally (Kp 4-) on 16 Jan 03:00 to 06:00 UTC. Unsettled geomagnetic conditions are expected over the next day. 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 until Jan 15 23:55 UTC and has since then dropped below the threshold and is expected to remain so in the upcoming day. The 24h electron fluence was at moderate level and is expected to return to normal level in the next day.Сегодняшнее значение числа солнечных пятен (International Sunspot Number): 138,
получено на основе анализа результатов 09 станций наблюдения.
Солнечные индексы за 15 Jan 2026
Число Вольфа по данным обсерватории Катания (IT9): ///
Солнечный поток в диапазоне 10см: 139
A-индекс по данным обсерватории Chambon-la-Foret (F): 019
A-индекс по данным обсерватории Wingst (DL): 012
Планетарный А-индекс Ap: 011
Вчерашнее значение числа солнечных пятен (International Sunspot Number): 094,
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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