Просмотр архива за суббота, 10 марта 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 Mar 10 2200 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.comСовместный отчет USAF/NOAA о солнечной и геофизической активности
Количество SD 070 на уровне 2200Z 10 Mar 2012
IA. Анализ активных солнечных регионов и активности от 09 - 2100Z до 10 - 2100Z
Solar activity was high. Region 1430 (N21W42) produced
a C8 flare at 10/1552Z and Region 1429 (N18W26) produced a long
duration M8 flare at 10/1744Z with an associated Tenflare (459 sfu)
and a Type IV radio sweep. Both flares had associated CMEs. The
first CME appeared in SOHO/LASCO C2 imagery at 10/1624Z with
the majority of the ejecta off the NW limb. The second CME,
associated with the M8 flare, first appeared in C2 imagery at
10/1800Z. Further analysis will be done as imagery becomes
available, however initial analysis indicated the event produced a
full-halo CME with an estimated plane-of-sky speed between 1200 -
1400 km/s. Region 1429 remained a large Ekc spot class with a
Beta-Gamma-Delta magnetic class. A new region appeared on the ENE
limb near Region 1432 (N16E52). Close proximity to the limb made a
detailed analysis of this new region difficult.
IB. Прогноз солнечной активности
Solar activity is expected to be at
moderate to high levels for the forecast period (11 - 13 March).
IIA. Обзор геофизической активности от 09 - 2100Z до 10 - 2100Z
The geomagnetic field was at quiet to minor storm levels with periods
of major storming at higher latitudes between 10/0600 - 1200Z.
Activity was due to the continued effects of the 07 March CME.
Solar wind speed at the ACE spacecraft has gradually decreased from
approximately 580 km/s to near 450 km/s. The greater than 10 MeV
and greater than 100 Mev proton events are on going. The greater
than 2 MeV electron flux at geosynchronous orbit was at high levels
throughout the period.
IIB. Прогноз геофизической активности
The geomagnetic field is
expected to be quiet to unsettled early on day 1 (11 March) until
the arrival of the 09 March CME followed by todays CME associated
with the M8 flare. Models show an arrival of the first CME early to
midday on 11 March which is expected to cause minor to major storm
conditions with isolated severe storm periods likely. Initial
estimates on the second CME indicate an arrival late on day 1.
Activity is expected to continue into day 2 (12 March) with minor to
major storm conditions with isolated severe storm periods possible.
Conditions are expected to decrease to unsettled to active levels by
day 3 (13 March).
III. Вероятность события от 11 - Mar до 13 - Mar
M-класс | 80% | 80% | 80% |
X-класс | 40% | 40% | 40% |
Протон | 99% | 99% | 60% |
PCAF | red
|
IV. Радиоизлучение λ = 10,7см
Наблюдаемый 10 Mar 149
Прогнозируемый 11 Mar-13 Mar 155/155/155
среднее значение за последние 3 месяца 10 Mar 125
V. Геомагнитные индексы
Наблюдаемый Afr/Ap 09 Mar 057/094
По оценкам Afr/Ap 10 Mar 013/018
Прогнозируемый Afr/Ap 11 Mar-13 Mar 047/085-024/040-007/012
VI. Вероятность геомагнитной активности с 11 - Mar до 13 - Mar
A. Средние широты |
Активно | 30% | 25% | 15% |
Слабый шторм | 35% | 30% | 05% |
Большой шторм | 35% | 25% | 01% |
B. Высокие широты |
Активно | 05% | 15% | 25% |
Слабый шторм | 15% | 25% | 15% |
Большой шторм | 75% | 55% | 10% |
Все время в UTC
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