QRZ.RU EXPRESS от 6 мая 2022

Опубликовано: 2022 May 05 1232 UTC
SIDC URSIGRAM 20505
Состояние солнечной активности на 05 May 2022, 1230UT
Прогноз сделан для периода с 1230UT, 05 May 2022 до 07 May 2022)
SOLAR FLARES : C-class flares expected, (probability >=50%)
Геомагнитное поле: Спокойное состояние (A<20 and K<4)
Солнечные протоны: Спокойное состояние
Прогноз на 05 May 2022: плотность потока солнечного излучения: 130, A-индекс: 006
Прогноз на 06 May 2022: плотность потока солнечного излучения: 133, A-индекс: 006
Прогноз на 07 May 2022: плотность потока солнечного излучения: 136, A-индекс: 010
Комментарий (на английском языке): There are four active region on the visible disk. NOAA AR 3006 and 3004 are the most magnetically important. The flare of highest X-ray input over the past 24 hours is the M1.6-class flare, with peak time 4 May 20:27UT. The rest of the regions were relatively quiet and stable. The flaring activity is expected to be at moderate levels with C-class flares expected, M-class flares probable and X-class flares possible. From the Coronal Mass Ejections observed, none have been confirmed to be Earth directed. The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2MeV electron flux exceeded the 1000 pfu threshold and is expected to exceed threshold over the next 24 hours. The 24h electron fluence was at normal to moderate levels and is expected to be at normal to moderate levels over the next 24 hours. The solar wind speed (as recorded by ACR) fluctuated around 350 km/s. The total magnetic field magnitude fluctuated around 5nT. The interplanetary magnetic field phi angle was predominantly in the negative sector (directed towards the Sun). The solar wind speed is expected to continue to remain in the slow solar wind regime for the next 48 hours. Geomagnetic conditions were quiet to unsettled (K Dourbes=3). Geomagnetic conditions are expected to be quiet over the next 48 hours.Сегодняшнее значение числа солнечных пятен (International Sunspot Number): 076,
получено на основе анализа результатов 16 станций наблюдения.
Солнечные индексы за 04 May 2022
Число Вольфа по данным обсерватории Катания (IT9): 115
Плотность потока излучения: 130
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): 077,
получено на основе анализа результатов 28 станций наблюдения.
Прошедшие события на Солнце:
DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES
04 1625 1632 1640 S16W11 M1.1 1N 96/3004
04 1940 1948 2003 ////// M1.5 ///3006
04 2009 2027 2036 ////// M1.6 96/3004