Просмотр архива за среда, 4 ноября 1998

Отчет о солнечной активности

Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Отчет о солнечно-геофизической активности 1998 Nov 04 2200 UTC
Подготовлено NOAA © SWPC и представлено SpaceWeatherLive.com

Совместный отчет USAF/NOAA о солнечной и геофизической активности

Количество SD 308 на уровне 2200Z 04 NOV 1998

IA. Анализ активных солнечных регионов и активности от 03 - 2100Z до 04 - 2100Z

SOLAR ACTIVITY WAS LOW. OVERALL THE AMOUNT OF ACTIVITY HAS INCREASED APPRECIABLY SINCE YESTERDAY. REGION 8375 (N18W07) HAS BEEN THE MOST ACTIVE REGION PRODUCING SIX C-CLASS FLARES AS WELL AS SEVERAL OPTICAL SUBFLARES AND ONE 1N OPTICAL FLARE. A FULL HALO CME WAS OBSERVED BY THE LASCO/SOHO SATELLITE AT 04/0418UT. THIS WAS IN CONJUNCTION WITH A C5/SF PRODUCED BY REGION 8375. REGION 8375 IS THE LARGEST AND MOST COMPLEX REGION ON THE SUN. CURRENTLY A DAI, BETA-GAMMA SPOT GROUP. THIS REGION HAS INCREASED SLIGHTLY IN SIZE AND THE SPOT COUNT HAS INCREASED FROM 22 TO 28. OTHER ACTIVE REGIONS ARE 8376 (S27E15), 8378 (N14E63) AND 8379 (S18W28) ALL OF WHICH PRODUCED AN OPTICAL SUBFLARE. REGION 8379 IS A NEW NUMBERED REGION WITH A 5 SPOT CRO, BETA SPOT GROUP. ONE OTHER REGION WAS NUMBERED: 8380 (S20E65) WITH AN AXX, ALPHA SPOT.
IB. Прогноз солнечной активности
SOLAR ACTIVITY IS EXPECTED TO REMAIN LOW WITH POSSIBLE ISOLATED M-CLASS FLARING FROM REGION 8375.
IIA. Обзор геофизической активности от 03 - 2100Z до 04 - 2100Z
THE GEOMAGNETIC FIELD HAS BEEN QUIET.
IIB. Прогноз геофизической активности
THE GEOMAGNETIC FIELD IS EXPECTED TO BE QUIET TO UNSETTLED WITH POSSIBLE ACTIVE PERIODS. THE CAUSE FOR THE POTENTIAL INCREASE IN GEOMAGNETIC ACTIVITY IS DUE TO A PARTIAL HALO CME THAT WAS OBSERVED BY THE LASCO/SOHO SATELLITE ON 02/1354UT. THIS WAS IN CONJUNCTION WITH A C1/N1 FLARE IN REGION 8376 LOCATED AT S25E44 AT THAT TIME. THE FULL HALO CME OBSERVED TODAY AT 04/0418UT COULD POSSIBLY CAUSE GEOMAGNETIC ACTIVITY LATE ON NOVEMBER 6TH OR ON NOVEMBER 7TH.
III. Вероятность события от 05 - NOV до 07 - NOV
M-класс30%30%30%
X-класс10%10%10%
Протон01%01%01%
PCAFGREEN
IV. Радиоизлучение λ = 10,7см
  Наблюдаемый       04 NOV 141
  Прогнозируемый   05 NOV-07 NOV  145/150/150
  среднее значение за последние 3 месяца        04 NOV 132
V. Геомагнитные индексы
OBSERVED AFR/AP 03 NOV  005/005
ESTIMATED AFR/AP 04 NOV  ???/???
PREDICTED AFR/AP 05 NOV-07 NOV  020/???-020/???-010/???
VI. Вероятность геомагнитной активности с 05 - NOV до 07 - NOV
A. Средние широты
Активно35%35%15%
Слабый шторм15%15%05%
Большой шторм01%01%01%
B. Высокие широты
Активно50%50%20%
Слабый шторм25%25%15%
Большой шторм01%01%01%
From [email protected] Wed Nov 4 17:41:46 1998 Received: by proton.sel.noaa.gov (1.37.109.18/16.2) id AA229939306; Wed, 4 Nov 1998 17:41:46 -0500 Return-Path: Date: Wed, 4 Nov 1998 22:40:04 GMT From: Space Environment Center Message-Id: <[email protected]> To: [email protected] Subject: RSGA Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII Content-Transfer-Encoding: 7bit Sender: [email protected] Precedence: bulk :Product: Report of Solar-Geophysical Activity :Issued: 1998 Nov 04 2240 UT # Prepared jointly by the U.S. Dept. of Commerce, NOAA, #Space Environment Center and the U.S. Air Force. # JOINT USAF/NOAA REPORT OF SOLAR AND GEOPHYSICAL ACTIVIT : : : : : : : CORRECTED COPY : : : : : : : : : : : : : : Количество SD 308 на уровне 2200Z 04 NOV 1998

IA. Анализ активных солнечных регионов и активности от 03 - 2100Z до 04 - 2100Z

SOLAR ACTIVITY WAS LOW. OVERALL THE AMOUNT OF ACTIVITY HAS INCREASED APPRECIABLY SINCE YESTERDAY. REGION 8375 (N18W07) HAS BEEN THE MOST ACTIVE REGION PRODUCING SIX C-CLASS FLARES AS WELL AS SEVERAL OPTICAL SUBFLARES AND ONE 1N OPTICAL FLARE. A FULL HALO CME WAS OBSERVED BY THE LASCO/SOHO SATELLITE AT 04/0418UT. THIS WAS IN CONJUNCTION WITH A C5/SF PRODUCED BY REGION 8375. REGION 8375 IS THE LARGEST AND MOST COMPLEX REGION ON THE SUN. CURRENTLY A DAI, BETA-GAMMA SPOT GROUP. THIS REGION HAS INCREASED SLIGHTLY IN SIZE AND THE SPOT COUNT HAS INCREASED FROM 22 TO 28. OTHER ACTIVE REGIONS ARE 8376 (S27E15), 8378 (N14E63) AND 8379 (S18W28) ALL OF WHICH PRODUCED AN OPTICAL SUBFLARE. REGION 8379 IS A NEW NUMBERED REGION WITH A 5 SPOT CRO, BETA SPOT GROUP. ONE OTHER REGION WAS NUMBERED: 8380 (S20E65) WITH AN AXX, ALPHA SPOT.
IB. Прогноз солнечной активности
SOLAR ACTIVITY IS EXPECTED TO REMAIN LOW WITH POSSIBLE ISOLATED M-CLASS FLARING FROM REGION 8375.
IIA. Обзор геофизической активности от 03 - 2100Z до 04 - 2100Z
THE GEOMAGNETIC FIELD HAS BEEN QUIET.
IIB. Прогноз геофизической активности
THE GEOMAGNETIC FIELD IS EXPECTED TO BE QUIET TO UNSETTLED WITH POSSIBLE ACTIVE PERIODS. THE CAUSE FOR THE POTENTIAL INCREASE IN GEOMAGNETIC ACTIVITY IS DUE TO A PARTIAL HALO CME THAT WAS OBSERVED BY THE LASCO/SOHO SATELLITE ON 02/1354UT. THIS WAS IN CONJUNCTION WITH A C1/N1 FLARE IN REGION 8376 LOCATED AT S25E44 AT THAT TIME. THE FULL HALO CME OBSERVED TODAY AT 04/0418UT COULD POSSIBLY CAUSE GEOMAGNETIC ACTIVITY LATE ON NOVEMBER 6TH OR ON NOVEMBER 7TH.
III. Вероятность события от 05 - NOV до 07 - NOV
M-класс30%30%30%
X-класс10%10%10%
Протон01%01%01%
PCAFGREEN
IV. Радиоизлучение λ = 10,7см
  Наблюдаемый       04 NOV 141
  Прогнозируемый   05 NOV-07 NOV  145/150/150
  среднее значение за последние 3 месяца        04 NOV 132
V. Геомагнитные индексы
OBSERVED AFR/AP 03 NOV  005/005
ESTIMATED AFR/AP 04 NOV  7/7
PREDICTED AFR/AP 05 NOV-07 NOV  20/12-20/15-15/10
VI. Вероятность геомагнитной активности с 05 - NOV до 07 - NOV
A. Средние широты
Активно35%35%15%
Слабый шторм15%15%05%
Большой шторм01%01%01%
B. Высокие широты
Активно50%50%20%
Слабый шторм25%25%15%
Большой шторм01%01%01%

<< Перейти на сегодняшнюю страницу обзора

Последние новости

Поддержка SpaceWeatherLive.com!

Большое количество посетителей приходят на сайт SpaceWeatherLive, чтобы получить информацию о состоянии Солнца, его активности или возможном появлении полярного сияния. Однако с увеличением трафика растет и стоимость хостинга. Если вы находите наш сайт SpaceWeatherLive.com полезным, пожалуйста, подумайте о пожертвовании на его содержание и поддержку!

54%
Поддержите SpaceWeatherLive с помощью наших товаров
Ознакомьтесь с нашими товарами

Сообщения и прогнозы

Получить текущие сообщения!

Факты о космической погоде

Последняя X-вспышка08/05/2024X1.0
Последняя M-вспышка08/05/2024M7.8
Последняя геомагнитная буря06/05/2024Kp5 (G1)
Безупречные дни
Последний безупречный день08/06/2022
Среднемесячное количество солнечных пятен
апреля 2024136.5 +31.6
Last 30 days161.2 +69.2

Этот день в истории (TOP5 рейтинг самых активных дней)*

Солнечные вспышки
12024X1.0
22024X1.0
32024M8.5
42024M7.8
52014M7.6
Ар-индексG
11960128G4
2200591G4
3201670G2
4194634G2
5199340G2
*с 1994 года

Социальные сети