Viewing archive of wtorek, 4 listopada 1997

Raport aktywności słonecznej

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.
Raport aktywności słoneczno- geomagnetycznej 1997 Nov 04 2200 UTC
Przygotowane przez NOAA © SWPC i przetworzone przez SpaceWeatherLive.com

Połączenie raportów USAF/NOAA o słonecznej i geofizycznej aktywności

Numer SDF 308 wydany w 2200Z na 04 NOV 1997

IA. Analiza aktywności regionów słonecznych i aktywność od 03-2100Z do 04-2100Z

SOLAR ACTIVITY BECAME HIGH. REGION 8100 (S21W38) PRODUCED AN X2/2B AT 04/0558Z. THIS EVENT HAD A 690 F.U. BURST AT 10 CM AND TYPE II/IV BURSTS. A HALO CORONAL MASS EJECTION WAS OBSERVED FOLLOWING THIS EVENT. THIS FLARE WAS PRECEDED BY AN M1 (NO OPTICAL) AT 04/0135Z AND AN M4/1F FROM REGION 8100 AT 04/0242Z. REGION 8100 ALSO PRODUCED MANY C-CLASS EVENTS. REGION 8100 CONTINUED TO GROW DURING THE PERIOD BUT AT A REDUCED RATE FROM THAT EXHIBITED ON 03 NOV. AREAL COVERAGE BECAME APPROXIMATELY 1000 MILLIONTHS DURING THE PERIOD. HOWEVER, SEVERAL AREAS THAT WERE EXHIBITING MIXED POLARITIES YESTERDAY ARE NOW FADING RESULTING IN A MORE BIPOLAR CONFIGURATION OF THE REGION. THE DELTA CONFIGURATION REMAINED BUT APPARENTLY IS WEAKENING. A NEW REGION EMERGED AT A RAPID PACE NEAR N24E10, WAS NUMBERED AS NEW REGION 8103, AND PRODUCED SEVERAL SUBFLARES.
IB. Prognoza aktywności słonecznej
SOLAR ACTIVITY SHOULD BE PREDOMINANTLY MODERATE. REGION 8100 REMAINS POTENT BUT THE DECREASE IN MAGNETIC COMPLEXITY ARGUES STRONGLY THAT FLARE FREQUENCY AND PEAK FLARE FLUX SHOULD ABATE SLIGHTLY. LARGE M-CLASS OR SMALL X-CLASS FLARES COULD OCCUR BUT ONLY INFREQUENTLY.
IIA. Podsumowanie aktywności geofizycznej 03-2100Z do 04-2100Z
THE GEOMAGNETIC FIELD WAS PREDOMINANTLY QUIET TO UNSETTLED. BRIEF ACTIVE CONDITIONS WERE OBSERVED IN THE 04/1500-1800Z PERIOD. A GREATER THAN 10 MEV PROTON EVENT BEGAN AT 04/0640Z, PASSED THE 10 PFU THRESHOLD AT 04/0830Z, AND REACHED A MAXIMUM OF 72 PFU AT 04/1120Z. THEREAFTER, GREATER THAN 10 MEV PROTON FLUXES SLOWLY DECLINED AND AT THE END OF THE PERIOD WERE AT 16 PFU. THE GREATER THAN 100 MEV PROTON FLUX REACHED A MAXIMUM OF 2.6 PFU AT 04/0930Z. POLAR CAP ABSORPTION DURING THIS EVENT WAS ESTIMATED TO HAVE BEEN 2.6 DB WITH A MAXIMUM AT APPROXIMATELY 04/1300Z.
IIB. Prognoza aktywności geofizycznej
THE GEOMAGNETIC FIELD SHOULD BE UNSETTLED TO SLIGHTLY ACTIVE ON 05 NOV. ACTIVE TO MINOR STORM CONDITIONS SHOULD BEGIN ON 06 NOV AS A RESULT OF A HALO CME OBSERVED ON 03 NOV. MAJOR STORM CONDITIONS ARE FORECAST FOR 07 NOV FROM THE X2 EVENT AND HALO CME OBSERVED ON 04 NOV. ISOLATED SEVERE STORMING IS POSSIBLE ON 07 NOV. ANOTHER PROTON EVENT IS POSSIBLE SHOULD REGION 8100 PRODUCE AN ADDITIONAL MAJOR FLARE. HOWEVER, AS MENTIONED ABOVE, ONLY ISOLATED MAJOR FLARES ARE EXPECTED IN THE NEAR FUTURE.
III. Prawdopodobieństwa zdarzenia 05 NOV do 07 NOV
Klasa M70%70%70%
Klasa X25%25%25%
Proton25%25%25%
PCAFIN PROGRESS
IV. Przepływ 10,7 cm z Penticton
  Zaobserwowano       04 NOV 118
  Przewidywane   05 NOV-07 NOV  121/122/120
  Średnia z 90 dni        04 NOV 089
V. Indeks geomagnetyczny A
OBSERVED AFR/AP 03 NOV  003/003
ESTIMATED AFR/AP 04 NOV  008/010
PREDICTED AFR/AP 05 NOV-07 NOV  015/020-025/035-050/060
VI. Prawdopodobieństwa aktywności geomagnetycznej 05 NOV do 07 NOV
A. Średnie szerokości geograficzne
Aktywne20%25%25%
Słaba burza10%30%25%
Bardzo znacząca burza05%15%30%
B. Wysokie szerokości geograficzne
Aktywne20%25%20%
Słaba burza20%35%30%
Bardzo znacząca burza05%20%35%

<< Idź do codziennego przeglądu

Najnowsze wiadomości

Wesprzyj SpaceWeatherLive.com!

Wielu ludzi odwiedza SpaceWeatherLive aby śledzić aktywność słoneczną lub sprawdzić czy jest szansa na zaobserwowanie zorzy polarnej. Niestety, większy ruch na stronie oznacza większe koszty utrzymania serwera. Dlatego, jeśli jesteś zadowolony ze strony SpaceWeatherLive, zachęcamy do wspierania nas finansowo. Dzięki temu będziemy mogli utrzymać naszą stronę.

54%
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Fakty na temat pogody kosmicznej

Ostatnie rozbłyski klasy X2024/03/28X1.1
Ostatnie rozbłyski klasy M2024/04/27M2.1
Ostatnia burza geomagnetyczna2024/04/26Kp5+ (G1)
Spotless days
Ostatni dzień bez skazy2022/06/08
Monthly mean Sunspot Number
marca 2024104.9 -19.8
Last 30 days136.8 +28.6

Ten dzień w przeszłości*

Rozbłyski słoneczne
11998X1.54
22006X1.13
32003M2.46
42024M2.1
52001M1.81
ApG
11956172G4
2195554G4
3193761G3
4196031G3
5199530G2
*od 1994

Sieci społeczne