Просмотр архива за среда, 10 ноября 2004
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 2004 Nov 10 2220 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.comСовместный отчет USAF/NOAA о солнечной и геофизической активности
Количество SD 315 на уровне 2200Z 10 Nov 2004
IA. Анализ активных солнечных регионов и активности от 09 - 2100Z до 10 - 2100Z
Solar activity continued at high levels this period.
The very active Region 696 (N08W62) produced an X2/3b Tenflare with
protons at 10/0213Z. Strong Type II and IV radio sweeps and moderate
centimetric radio bursts also accompanied this flare. LASCO imagery
showed a very fast asymetrical full halo CME with a plane-of-sky
speed estimated at 2000 km/s. Region 696 continues to gradually
decrease in area, but maintains a significant delta configuration.
The rest of the visible disk was quiet and stable.
IB. Прогноз солнечной активности
Solar activity is expected to be
moderate to high. Region 696, though in decay, maintains potential
for major flare activity. This region will rotate around the west
limb on 13 November and as a result, solar activity levels are
expected to significantly decline.
IIA. Обзор геофизической активности от 09 - 2100Z до 10 - 2100Z
The geomagnetic field ranged from active to severe storm levels.
Yesterday's strong shock at 09/1852Z was followed by a short period
of strong southward Bz to near 40 nT, before rotating northward for
approximately five hours. At 10/0100Z, the solar wind exceeded 800
km/s and Bz rotated southward again, ranging from -15 to -25 nT for
over nine hours. The geomagnetic field response was severe at all
latitudes. The period ended at minor storm levels with solar wind
speed declining to near 600 km/s. A new influx of high energy
protons followed the X2 flare at 10/0213Z. A greater than 10 MeV
peak flux of 424 pfu was observed at 10/1655Z. A greater than 100
Mev proton event also occurred in association with the X2 flare. It
began on 10/0320Z, peaked at 2.1 pfu at 10/0340Z, and ended at
10/1250Z. The greater that 2 MeV electron flux was at high levels.
IIB. Прогноз геофизической активности
The geomagnetic field is
expected to range from unsettled to severe storm levels on 11 and 12
November. The two halo CMEs observed on 09 and 10 November are
expected to impact the geomagnetic field on 11 November. Both of
these fast CMEs had a strong westward component; however, their
combined effects may produce major or even severe storm periods. On
12 November, field conditions are expected to return to mostly
unsettled to minor storm levels, with occasional major storm periods
at high latitudes. Unsettled to active conditions are expected on 13
November. The greater than 10 MeV proton event currently in progress
is expected to end by 12 November.
III. Вероятность события от 11 - Nov до 13 - Nov
| M-класс | 70% | 65% | 60% |
| X-класс | 20% | 15% | 10% |
| Протон | 99% | 25% | 15% |
| PCAF | in progress
|
IV. Радиоизлучение λ = 10,7см
Наблюдаемый 10 Nov 105
Прогнозируемый 11 Nov-13 Nov 100/095/090
среднее значение за последние 3 месяца 10 Nov 109
V. Геомагнитные индексы
Наблюдаемый Afr/Ap 09 Nov 047/120
По оценкам Afr/Ap 10 Nov 100/200
Прогнозируемый Afr/Ap 11 Nov-13 Nov 075/125-030/050-020/030
VI. Вероятность геомагнитной активности с 11 - Nov до 13 - Nov
| A. Средние широты |
| Активно | 25% | 40% | 30% |
| Слабый шторм | 50% | 25% | 20% |
| Большой шторм | 25% | 15% | 10% |
| B. Высокие широты |
| Активно | 20% | 40% | 40% |
| Слабый шторм | 40% | 30% | 20% |
| Большой шторм | 40% | 20% | 10% |
Все время в UTC
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