Просмотр архива за суббота, 26 марта 2011
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 2011 Mar 26 2200 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.comСовместный отчет USAF/NOAA о солнечной и геофизической активности
Количество SD 085 на уровне 2200Z 26 Mar 2011
IA. Анализ активных солнечных регионов и активности от 25 - 2100Z до 26 - 2100Z
Solar activity was moderate due to an impulsive M1
X-ray event at 25/2322Z from Region 1176 (S16E16). Associated with
this event were Type II (673 km/s), Type IV and 10.7 cm (170 sfu)
radio signatures. Region 1176 remained mostly unchanged through the
period, though it increased in longitudinal extent, and is
classified as an F-type group. Region 1178 (S15E43) developed
penumbra in its trailer spots to become a D-type group. At about
26/0500Z, GOES-15 SXI BE12A imagery observed a large surge from
Region 1180 (N25E53) that appeared to continue for about six hours.
X-ray data was mostly unavailable during this event due to GOES-13
and GOES-15 eclipse phase. Associated with this event was a
fast-moving (approximately 850 km/s) partial-halo, asymmetric CME
first observed in LASCO C3 imagery at 26/0630Z and STEREO-A and B
COR2 imagery at 26/0709Z. Though this CME does not appear to have an
Earth-directed component, further analysis is required.
IB. Прогноз солнечной активности
Solar activity is expected to be low
for the next three days (27 - 29 March). A chance for M-class
activity exists on day one (27 March) becoming likely on days two
and three (28 - 29 March) with a slight chance for X-class activity
on 29 March. This expected increase in activity is due to the
complex nature of Region 1176 and the return of old Region 1166
(N10, L=110) on 27 March. On its last transit across the disk, old
Region 1166 produced four M-class events and one X-class event.
IIA. Обзор геофизической активности от 25 - 2100Z до 26 - 2100Z
The geomagnetic field was at quiet levels. ACE solar wind data
indicated a gradual decrease in wind velocities from a high of 460
km/s at 26/0243Z to a low of 360 km/s at 26/1841Z. IMF Bz was
predominately north through the period.
IIB. Прогноз геофизической активности
The geomagnetic field is
expected to be at mostly quiet levels for day one (27 March). By day
two (28 March), quiet to unsettled conditions, with isolated active
periods, are possible due to effects from the 24 March CME. Quiet
levels are expected to return on day three (29 March).
III. Вероятность события от 27 - Mar до 29 - Mar
| M-класс | 50% | 60% | 70% |
| X-класс | 05% | 05% | 10% |
| Протон | 01% | 01% | 01% |
| PCAF | green
|
IV. Радиоизлучение λ = 10,7см
Наблюдаемый 26 Mar 115
Прогнозируемый 27 Mar-29 Mar 120/125/125
среднее значение за последние 3 месяца 26 Mar 096
V. Геомагнитные индексы
Наблюдаемый Afr/Ap 25 Mar 002/003
По оценкам Afr/Ap 26 Mar 002/003
Прогнозируемый Afr/Ap 27 Mar-29 Mar 005/005-010/010-005/005
VI. Вероятность геомагнитной активности с 27 - Mar до 29 - Mar
| A. Средние широты |
| Активно | 10% | 20% | 10% |
| Слабый шторм | 01% | 05% | 01% |
| Большой шторм | 01% | 01% | 01% |
| B. Высокие широты |
| Активно | 15% | 25% | 15% |
| Слабый шторм | 01% | 10% | 01% |
| Большой шторм | 01% | 01% | 01% |
Все время в UTC
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