Viewing archive of wtorek, 6 listopada 2001

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 2001 Nov 06 2200 UTC
Przygotowane przez NOAA © SWPC i przetworzone przez SpaceWeatherLive.com

Połączenie raportów USAF/NOAA o słonecznej i geofizycznej aktywności

Numer SDF 310 wydany w 2200Z na 06 Nov 2001

IA. Analiza aktywności regionów słonecznych i aktywność od 05-2100Z do 06-2100Z

Solar activity was at moderate levels. Four M-class events were reported during the period. Region 9687 (S20E08) produced the largest event, an M2/1b flare at 06/0300 UTC. This event also had an accompanying Type II radio sweep (velocity estimated at 600 km/s). Region 9687 developed into a complex beta-gamma-delta magnetic classification during the period. Region 9690 was by far, the most active region on the disk today. It produced several C-class events and two minor M-class events. Region 9690 has fully rotated onto the disk and appears to be a moderately large region (750 millionths) with a beta-gamma magnetic classification. Region 9684 (N06W55), which produced the X1/3b proton flare on 04 November, retains a beta-gamma-delta magnetic classification, but did not produce any significant activity during the period.
IB. Prognoza aktywności słonecznej
Solar activity is expected to continue to be moderate to high. Regions 9684, 9687, and 9690 all possess major flare potential.
IIA. Podsumowanie aktywności geofizycznej 05-2100Z do 06-2100Z
The geomagnetic field was at unsettled to severe storm conditions. The full-halo coronal mass ejection (CME) from the 04 November event impacted the geomagnetic field at 06/0150 UTC. This was indicated by a 90 nT sudden impulse as measured by the USGS Boulder magnetometer. Severe geomagnetic storming occurred between 06/0000 and 06/0600 UTC and 15-1800 UTC. The greater than 10 MeV proton event peaked at 31,700 pfu at 06/0215 UTC. The greater than 100 MeV proton event peaked at 253 pfu at 06/0220 UTC. Both proton events levels declined sharply during the period but continued through the end of the day. A polar cap absorption event remained in effect.
IIB. Prognoza aktywności geofizycznej
The geomagnetic field is expected to be unsettled to minor storm conditions on the first day of the period and then declining to mostly quiet to unsettled, with isolated active conditions possible, on days two and three. However, there have been several long and near long duration flares in the last two days that could have produced earth-directed coronal mass ejections. Since the onset of the proton storm at approximately 1700 UTC on 04 November, the LASCO instrument has been saturated by the particles and it is nearly impossible to determine if any CME's have been produced or if they are earth-directed. Impacts from any earth-directed CME's would obviously cause an increase in geomagnetic activity. The greater than 100 MeV proton event is expected to continue until approximately 07/1200 UTC. The greater than 10 MeV proton event ended the day at 567 pfu and is expected to continue for at least another 24 hours. The Polar cap absorption event is expected to last until 09/0000 UTC.
III. Prawdopodobieństwa zdarzenia 07 Nov do 09 Nov
Klasa M80%80%80%
Klasa X25%25%25%
Proton99%99%80%
PCAFin progress
IV. Przepływ 10,7 cm z Penticton
  Zaobserwowano       06 Nov 237
  Przewidywane   07 Nov-09 Nov  235/235/230
  Średnia z 90 dni        06 Nov 208
V. Indeks geomagnetyczny A
  Zaobserwowano Afr/Ap 05 Nov  012/013
  Szacowane     Afr/Ap 06 Nov  075/100
  Przewidywane    Afr/Ap 07 Nov-09 Nov  030/030-012/015-010/012
VI. Prawdopodobieństwa aktywności geomagnetycznej 07 Nov do 09 Nov
A. Średnie szerokości geograficzne
Aktywne50%35%35%
Słaba burza25%15%15%
Bardzo znacząca burza04%04%04%
B. Wysokie szerokości geograficzne
Aktywne40%30%25%
Słaba burza35%15%15%
Bardzo znacząca burza20%10%05%

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