Просмотр архива за четверг, 19 июня 2003
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 2003 Jun 19 2200 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.comСовместный отчет USAF/NOAA о солнечной и геофизической активности
Количество SD 170 на уровне 2200Z 19 Jun 2003
IA. Анализ активных солнечных регионов и активности от 18 - 2100Z до 19 - 2100Z
Solar activity decreased to very low levels. Flare
activity was limited to several B-class flares. Region 386 (S07E30)
lost penumbral coverage over the period although it does retain a
delta magnetic structure in the dominant lead spot. Region 387
(N18E49) grew in both penumbral coverage and magnetic complexity
since yesterday, a gamma structure is now evident in the trailing
portion of the spot group. Newly numbered Region 388 (S03E08)
produced a minor B-class flare early in the period.
IB. Прогноз солнечной активности
Solar activity is expected to be at
moderate levels. Region 386 remains capable of producing an
isolated major flare.
IIA. Обзор геофизической активности от 18 - 2100Z до 19 - 2100Z
The geomagnetic field was at predominantly active levels today.
Minor storm conditions were observed at both middle and high
latitudes between 19/0000 and 0300Z due to the influence of a
recurrent high speed coronal hole stream. The greater than 10 MeV
proton flux exceeded event threshold at 18/2050Z (reached a max of
24 pfu at 19/0450Z), ended at 19/1900Z and after careful review the
event is believed to have been the result of the M6.8 x-ray flare
from June 17. The greater than 2 MeV electron flux reached moderate
levels today.
IIB. Прогноз геофизической активности
The geomagnetic field is
expected to be at predominantly unsettled to active levels through
the interval. Minor storm conditions may exist due to a transient
passage during the first half of day one in response to the M6.8
x-ray flare from June 17.
III. Вероятность события от 20 - Jun до 22 - Jun
M-класс | 50% | 50% | 50% |
X-класс | 15% | 15% | 15% |
Протон | 25% | 15% | 15% |
PCAF | green
|
IV. Радиоизлучение λ = 10,7см
Наблюдаемый 19 Jun 123
Прогнозируемый 20 Jun-22 Jun 125/125/125
среднее значение за последние 3 месяца 19 Jun 124
V. Геомагнитные индексы
Наблюдаемый Afr/Ap 18 Jun 036/054
По оценкам Afr/Ap 19 Jun 023/025
Прогнозируемый Afr/Ap 20 Jun-22 Jun 020/025-020/025-012/020
VI. Вероятность геомагнитной активности с 20 - Jun до 22 - Jun
A. Средние широты |
Активно | 40% | 40% | 25% |
Слабый шторм | 15% | 15% | 10% |
Большой шторм | 10% | 10% | 05% |
B. Высокие широты |
Активно | 50% | 50% | 40% |
Слабый шторм | 20% | 20% | 15% |
Большой шторм | 10% | 10% | 10% |
PLAIN
GOES Protons:
To ensure continued operational monitoring of important energetic particle data, it is necessary to reassign primary/secondary designations for the GOES Space Environment Monitor (SEM) detectors. GOES 11 (113W) is now the primary satellite for protons. GOES 12 will continue as the primary satellite for magnetometer, X-ray, and electron measurements. GOES 10 (135W) will be the secondary satellite for all SEM sensors - magnetometer, X-ray, and energetic particles. Because of the degraded state of the proton data on GOES-10, its designation as the secondary source for proton data is a short-term solution. More permanent solutions have been identified and are being evaluated. Users will be notified when we define and schedule a permanent fix. Further details can be found at http://www.sec.noaa.gov/GOES.html.
K-Indices:
On 16 June, it was determined that a scaling problem exists with the Boulder magnetometer instrument. While this problem, and its fix are being investigated the primary instrument for Boulder K-indices has been switched to the Boulder USGS (via Domsat) magnetometer, effective 1500 UTC on 16 June.
99999
Все время в UTC
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