Просмотр архива за суббота, 2 мая 1998
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 1998 May 02 2200 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.comСовместный отчет USAF/NOAA о солнечной и геофизической активности
Количество SD 122 на уровне 2200Z 02 MAY 1998
IA. Анализ активных солнечных регионов и активности от 01 - 2100Z до 02 - 2100Z
SOLAR ACTIVITY HAS BEEN HIGH FOR THE PAST 24 HOURS.
REGION 8210 (S17W21) PRODUCED AN X1/3B TENFLARE (1300 FLUX UNITS)
THAT REACHED MAXIMUM AT 02/1342 UT. IT WAS ACCOMPANIED BY A
PARTIAL-HALO CORONAL MASS EJECTION (REPORTED BY SOHO/LASCO
OPERATIONS), SIGNIFICANT RADIO BURSTS ACROSS THE SPECTRUM AND A TYPE
IV SWEEP. THE CME WAS CONCENTRATED OFF THE NW LIMB AND THE MEASURED
SPEED WAS APPROXIMATELY 750 KM/S. REGION 8210 ALSO PARTICIPATED IN
AN M1 X-RAY EVENT ON 01/2254 UT SHARED WITH REGION 8214 (N27E19).
THIS EARLIER EVENT MAY ALSO BE ASSOCIATED WITH A PARTIAL-HALO CME
CONCENTRATED OFF THE NE LIMB. REGION 8210 IS EXTREMELY MAGNETICALLY
COMPLEX, AND REGIONS 8210 AND 8214 ARE BOTH CONTINUING TO GROW IN
SIZE AND SPOT COUNT. NEW REGION 8217 (S17E77), A SIMPLE A-TYPE
GROUP, WAS NUMBERED TODAY. THERE ARE CONTINUING INDICATIONS OF
ACTIVE REGIONS BEYOND THE EAST LIMB THAT WILL BE ROTATING ONTO THE
DISK IN THE NEXT FEW DAYS.
IB. Прогноз солнечной активности
SOLAR ACTIVITY IS EXPECTED TO PERSIST
AT MODERATE TO HIGH LEVELS. REGION 8210 RETAINS THE EXTREME MAGNETIC
COMPLEXITY ASSOCIATED WITH MAJOR X-RAY EVENTS, AND THE PROBABILITY
OF SIGNIFICANT ACTIVITY FROM REGION 8214 IS INCREASING AS IT
CONTINUES TO DEVELOP.
IIA. Обзор геофизической активности от 01 - 2100Z до 02 - 2100Z
GEOMAGNETIC ACTIVITY REACHED PERIODS AT MAJOR STORM LEVELS DURING THE
PAST 24 HOURS. THE STORM SUDDEN COMMENCEMENT OCCURRED AT 01/2158 UT.
IT IS PRESUMED TO HAVE ORIGINATED WITH A MAJOR SOLAR EVENT ON 29
APRIL. PRECEDING THE SSC, THE PASSAGE OF AN INTERPLANETARY SHOCK WAS
OBSERVED IN ACE SOLAR WIND DATA AT APPROXIMATELY 01/2124 UT. A
GREATER THAN 100 MEV SATELLITE PROTON EVENT BEGAN 02/1405 AND
REACHED 7.6 PFU AT 1540 UT. A GREATER THAN 10 MEV SATELLITE PROTON
EVENT BEGAN AT 02/1420UT AND REACHED 150 PFU AT 1650 UT. BOTH
EVENTS ARE STILL IN PROGRESS AT REPORT ISSUE TIME. A POLAR CAP
ABSORPTION EVENT IS IN PROGRESS, AS WELL AS A FORBUSH DECREASE OF
APPROXIMATELY 5 PERCENT.
IIB. Прогноз геофизической активности
GEOMAGNETIC ACTIVITY IS
EXPECTED TO DECLINE TOWARD GENERALLY UNSETTLED TO ACTIVE CONDITIONS
TOMORROW, BUT A NEW STORM COMMENCEMENT IS EXPECTED AFTER MIDDAY ON
04 MAY FROM THE X-CLASS SOLAR ACTIVITY ON 02 MAY. MAJOR STORM
CONDITIONS ARE PROBABLE ON 05 MAY. THE SATELLITE PROTON EVENT AT
GREATER THAN 10 MEV ENERGIES IS EXPECTED TO PERSIST THROUGH 04 MAY,
AND COULD CONTINUE LONGER IF NEW SOLAR ACTIVITY OCCURS.
III. Вероятность события от 03 - MAY до 05 - MAY
| M-класс | 50% | 50% | 50% |
| X-класс | 30% | 30% | 30% |
| Протон | 30% | 30% | 30% |
| PCAF | IN PROGRESS
|
IV. Радиоизлучение λ = 10,7см
Наблюдаемый 02 MAY 117
Прогнозируемый 03 MAY-05 MAY 130/140/150
среднее значение за последние 3 месяца 02 MAY 104
V. Геомагнитные индексы
OBSERVED AFR/AP 01 MAY 008/008
ESTIMATED AFR/AP 02 MAY 045/060
PREDICTED AFR/AP 03 MAY-05 MAY 020/035-020/020-050/050
VI. Вероятность геомагнитной активности с 03 - MAY до 05 - MAY
| A. Средние широты |
| Активно | 30% | 25% | 10% |
| Слабый шторм | 25% | 15% | 20% |
| Большой шторм | 11% | 21% | 60% |
| B. Высокие широты |
| Активно | 25% | 35% | 10% |
| Слабый шторм | 30% | 20% | 20% |
| Большой шторм | 16% | 11% | 60% |
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