QRZ.RU EXPRESS от 6 января 2026

Опубликовано: 05 января 2026 в 1231 UTC
SIDC URSIGRAM 60105
Состояние солнечной активности на 05 января 2026, 1230UT
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 05 января 2026: Солнечный поток в диапазоне 10см: 156 / AP-индекс: 017
Прогноз на 06 января 2026: Солнечный поток в диапазоне 10см: 158 / AP-индекс: 017
Прогноз на 07 января 2026: Солнечный поток в диапазоне 10см: 158 / AP-индекс: 017
Комментарий (на английском языке): Solar Active Regions and flaring: Solar flaring activity was low over the past 24 hours, with several C-class flares recorded. The largest flare was a C3.0 flare (SIDC Flare 6582) peaking on January 05 at 09:20 UTC, associated with SIDC Sunspot Group 722 (NOAA Active Region 4334; magnetic type alpha). There are currently seven numbered active regions on the visible solar disk. SIDC Sunspot Group 745 (NOAA Active Region 4325, magnetic type beta-gamma) remains the largest and most complex active region, but produced only low-level C-class flaring. Low flaring activity was also produced by SIDC Sunspot Group 744 (NOAA Active Region 4324; magnetic type alpha) and by SIDC Sunspot Group 754 (NOAA Active Region 4336; magnetic type beta). The remaining active regions are relatively simple (magnetic type alpha or beta) and did not produce any significant flaring activity. Solar flaring activity is expected to be low over the next 24 hours, with C-class flares expected and a M-class flares possible. Coronal mass ejections: No Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images over the past 24 hours. Solar wind: A shock was registered in the solar wind data around 20:40 UTC on January 01, likely associated with a CME that lifted off the solar surface at around 18:00 on January 01 (SIDC CME 618). The interplanetary magnetic field quickly jumped from 440 to 470 km/s. The southward component of the interplanetary magnetic field reached minimum values -10 nT. Solar wind conditions are expected to remain slightly elevated on January 05 due to the ICME passage, before gradually returning to slow solar wind conditions. Geomagnetism: Geomagnetic conditions reached active levels globally (NOAA Kp = 4, 4+) between 03:00 and 09:00 UTC on January 5 due to the ICME arrival. Locally over Belgium, quiet to unsettled conditions were observed (K-Bel = 1 to 3). Mostly quiet to unsettled geomagnetic conditions are expected over the next 24 hours, with a chance of isolated active periods. Proton flux levels: The greater than 10 MeV proton flux, as measured by the GOES-19 satellite, was at background levels over the past 24 hours and is likely to remain so in the next 24 hours. Electron fluxes at GEO: The greater than 2 MeV electron flux, as measured by GOES-18 and GOES-19 satellites, exceeded the 1000 pfu threshold. The greater than 2 MeV electron flux may exceed the 1000 pfu threshold over the next 24 hours. The electron fluence was at moderate levels and is expected to be at normal to moderate levels for the next 24 hours.Сегодняшнее значение числа солнечных пятен (International Sunspot Number): 106,
получено на основе анализа результатов 10 станций наблюдения.
Солнечные индексы за 04 Jan 2026
Число Вольфа по данным обсерватории Катания (IT9): ///
Солнечный поток в диапазоне 10см: 157
A-индекс по данным обсерватории Chambon-la-Foret (F): 016
A-индекс по данным обсерватории Wingst (DL): 005
Планетарный А-индекс Ap: 005
Вчерашнее значение числа солнечных пятен (International Sunspot Number): 115,
получено на основе анализа результатов 18 станций наблюдения.
Прошедшие события на Солнце:
DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES
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