Просмотр архива за вторник, 24 января 2012
Отчет о солнечной активности
Любая солнечная вспышка, упомянутая в этом расчете, имеет масштабирующий коэффициент, применяемый Центром прогнозирования космической погоды (SWPC). Из-за него солнечные вспышки здесь на 42% слабее, чем в научных данных. Из наших архивов этот коэффициент был удален, чтобы показать реальные величины вспышек.
Отчет о солнечно-геофизической активности 2012 Jan 24 2200 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.comСовместный отчет USAF/NOAA о солнечной и геофизической активности
Количество SD 024 на уровне 2200Z 24 Jan 2012
IA. Анализ активных солнечных регионов и активности от 23 - 2100Z до 24 - 2100Z
Solar activity was at low levels. Low-level C-class
events were observed from Region 1401 (N16W53) and Region 1402
(N29W48). Region 1401 indicated slight decay while Region 1402
showed some growth in the trailer spots.
IB. Прогноз солнечной активности
Solar activity is expected to be low
during the period (25 - 27 January) with M-class activity likely
from Regions 1401 and 1402.
IIA. Обзор геофизической активности от 23 - 2100Z до 24 - 2100Z
The geomagnetic field was at quiet to active levels with isolated
minor to major storm periods. At 24/1431Z, an interplanetary shock
passage was recorded at the ACE satellite with a corresponding
sudden impulse of 22 nT observed at the Boulder magnetometer at
24/1504Z. At the time of the IP shock passage, Bt reached a maximum
of 37 nT at 24/1439Z while the Bz component of the interplanetary
magnetic field hit a maximum northward extent of 27 nT at 24/1436Z
and a maximum southward extent of -16 nT at 24/1807Z. Wind
velocity, as measured at the SOHO spacecraft, were observed at shock
passage near 750 km/s with post shock passage speeds near 650 km/s.
The greater than 100 MeV proton flux event that began at 23/0445Z,
reached a maximum of 2 pfu at 23/0750Z and ended at 23/2050Z. The
greater than 10 MeV proton flux event that began at 23/0530Z,
reached a new maximum of 6310 pfu at 24/1530Z and was still in
progress at the time of this writing.
IIB. Прогноз геофизической активности
The geomagnetic field is
expected to be at unsettled to minor storm levels, with isolated
major storm intervals, on day one (25 January) as effects from the
arrival of the 23 January CME persist. By day two (26 January), the
field is expected to be at mostly quiet levels as CME effects wane.
Quiet to unsettled levels, with isolated active periods, are
expected on day three (27 January) due to a recurrent coronal hole
high speed stream rotating into a geoeffective position. The
greater than 10 MeV proton flux event is expected to remain above
threshold through 26 January, falling to background levels by 27
January.
III. Вероятность события от 25 - Jan до 27 - Jan
| M-класс | 60% | 60% | 60% |
| X-класс | 10% | 10% | 10% |
| Протон | 99% | 99% | 50% |
| PCAF | in progress
|
IV. Радиоизлучение λ = 10,7см
Наблюдаемый 24 Jan 136
Прогнозируемый 25 Jan-27 Jan 140/140/135
среднее значение за последние 3 месяца 24 Jan 143
V. Геомагнитные индексы
Наблюдаемый Afr/Ap 23 Jan 007/011
По оценкам Afr/Ap 24 Jan 022/030
Прогнозируемый Afr/Ap 25 Jan-27 Jan 018/020-005/005-007/008
VI. Вероятность геомагнитной активности с 25 - Jan до 27 - Jan
| A. Средние широты |
| Активно | 35% | 10% | 25% |
| Слабый шторм | 20% | 05% | 05% |
| Большой шторм | 05% | 01% | 01% |
| B. Высокие широты |
| Активно | 40% | 15% | 35% |
| Слабый шторм | 25% | 05% | 15% |
| Большой шторм | 10% | 01% | 05% |
Все время в UTC
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