Archiv von Mittwoch, 4 November 1998 anzeigen

Sonnenaktivitätsbericht

Für jede Sonneneruption in diesem Bericht wird ein Skalierungsfaktor vom Space Weather Prediction Center (SWPC) angewendet. Aufgrund dieses SWPC-Skalierungsfaktors werden Sonneneruptionen um 42 % kleiner gemeldet als die Daten für wissenschaftliche Zwecke. Der Skalierungsfaktor wurde aus unseren archivierten Sonneneruptionsdaten entfernt, um die tatsächlichen physikalischen Einheiten widerzuspiegeln.
Bericht der solaren und geophysikalischen Aktivität 1998 Nov 04 2200 UTC
Erstellt von NOAA © SWPC und verarbeitet von SpaceWeatherLive.com

Gemeinsamer Bericht der USAF und NOAA zur solaren und geophysikalischen Aktivität

SDF Nummer 308 ausgestellt am 04 NOV 1998 um 2200 Uhr UTC

IA. Analyse der aktiven Sonnenflecken-Gruppen und der Aktivität vom 03-2100Z Uhr bis 04-2100Z Uhr

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. Sonnenaktivitäts-Prognose
SOLAR ACTIVITY IS EXPECTED TO REMAIN LOW WITH POSSIBLE ISOLATED M-CLASS FLARING FROM REGION 8375.
IIA. Geophysikalische Aktivität vom 03-2100Z Uhr bis 04-2100Z Uhr
THE GEOMAGNETIC FIELD HAS BEEN QUIET.
IIB. Geophysikalische Aktivitätsprognose
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. Ereignis-Wahrscheinlichkeiten 05 NOV bis 07 NOV
Klasse M30%30%30%
Klasse X10%10%10%
Protonensturm01%01%01%
PCAFGREEN
IV. Penticton 10.7 cm Flux
  Beobachtet       04 NOV 141
  Vorhergesagt   05 NOV-07 NOV  145/150/150
  90 Tage Mittel        04 NOV 132
V. Geomagnetischer Ap Index
OBSERVED AFR/AP 03 NOV  005/005
ESTIMATED AFR/AP 04 NOV  ???/???
PREDICTED AFR/AP 05 NOV-07 NOV  020/???-020/???-010/???
VI. Geomagnetische Aktivität - Wahrscheinlichkeiten 05 NOV bis 07 NOV
A. Mittlere Breiten
Aktiv35%35%15%
Geringer Sturm15%15%05%
Schwerwiegender Sturm01%01%01%
B. Hohe Breiten
Aktiv50%50%20%
Geringer Sturm25%25%15%
Schwerwiegender Sturm01%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 : : : : : : : : : : : : : : SDF Nummer 308 ausgestellt am 04 NOV 1998 um 2200 Uhr UTC

IA. Analyse der aktiven Sonnenflecken-Gruppen und der Aktivität vom 03-2100Z Uhr bis 04-2100Z Uhr

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. Sonnenaktivitäts-Prognose
SOLAR ACTIVITY IS EXPECTED TO REMAIN LOW WITH POSSIBLE ISOLATED M-CLASS FLARING FROM REGION 8375.
IIA. Geophysikalische Aktivität vom 03-2100Z Uhr bis 04-2100Z Uhr
THE GEOMAGNETIC FIELD HAS BEEN QUIET.
IIB. Geophysikalische Aktivitätsprognose
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. Ereignis-Wahrscheinlichkeiten 05 NOV bis 07 NOV
Klasse M30%30%30%
Klasse X10%10%10%
Protonensturm01%01%01%
PCAFGREEN
IV. Penticton 10.7 cm Flux
  Beobachtet       04 NOV 141
  Vorhergesagt   05 NOV-07 NOV  145/150/150
  90 Tage Mittel        04 NOV 132
V. Geomagnetischer Ap Index
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. Geomagnetische Aktivität - Wahrscheinlichkeiten 05 NOV bis 07 NOV
A. Mittlere Breiten
Aktiv35%35%15%
Geringer Sturm15%15%05%
Schwerwiegender Sturm01%01%01%
B. Hohe Breiten
Aktiv50%50%20%
Geringer Sturm25%25%15%
Schwerwiegender Sturm01%01%01%

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