Viewing archive of onsdag, 7 september 2005

Solaktivitetsrapport

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.
Rapport för sol- och geofysisk aktivitet 2005 Sep 07 2204 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com

USAF/NOAA rapport för sol- och geofysisk aktivitet

SDF Nummer 250 publicerat klockan 2200Z på 07 Sep 2005

IA. Analys av solfläcksgrupper och solaktivitet från 06-2100Z till 07-2100Z

Solar activity increased to high levels this period as newly numbered Region 808 (S12E83) produced one of the largest solar flares of Cycle 23. An X17/3b white light flare erupted in this region at 07/1740Z. A large and fast CME was visible on the MK4 coronagraph at Mauna Loa. Intense centimetric radio bursts accompanied this flare, including a 27,000 sfu Tenflare. Type II (1860 km/s) and Type IV radio sweeps were also observed. This region also produced a very long duration M1 flare, which peaked at 06/2202Z. A fast and bright CME (1400 km/s) on LASCO imagery was observed with this event. The sunspot cluster associated with Region 808 is just now rotating into view, so an accurate assessment of its true size and complexity will have to wait. Region 808 is the return of old Region 798, which produced significant solar and geophysical activity during its last passage on the visible disk.
IB. Prognos för solaktivitet
Solar activity is expected to be moderate to high. Region 808 is obviously a complex and moderate-large size sunspot group with great flare potential. Expect further major flares.
IIA. Sammanfattning av geofysisk aktivitet 06-2100Z till 07-2100Z
The geomagnetic field was quiet to active. Today's powerful X17 flare produced a sudden disturbance in the geomagnetic field at 07/1725Z. This 82 nT magnetic crochet was one of the largest observed this Solar Cycle. A slow rise in the greater than 10 MeV protons at geosynchronous orbit began near issue time. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels again today.
IIB. Prognos för geofysisk aktivitet
The geomagnetic field is expected to continue at quiet to unsettled levels with isolated active periods. The CME activity associated with yesterday's long-duration M1 and today's X17 flares were not Earth directed. The greater than 10 MeV protons at geosynchronous orbit are slowly rising now and are expected to continue to do so. These protons will likely cross the 10 pfu threshold on 08 Sep.
III. Chans för solutbrott från 08 Sep till 10 Sep
M-klass70%75%75%
X-klass30%30%30%
Proton60%50%40%
PCAFyellow
IV. Penticton 10.7 cm Flux
  Observerad       07 Sep 100
  Prognoserat   08 Sep-10 Sep  110/120/120
  90 Day Mean        07 Sep 091
V. Geomagnetiskt A-index
  Observerad Afr/Ap 06 Sep  006/009
  Förväntat     Afr/Ap 07 Sep  010/010
  Prognoserat    Afr/Ap 08 Sep-10 Sep  008/012-010/015-005/010
VI. Chanser för geomagnetisk aktivitet från 08 Sep till 10 Sep
A. Medelhöga breddgrader
Aktivt20%20%15%
Små stormförhållanden05%05%05%
Svåra stormförhållanden01%01%01%
B. Höga breddgrader
Aktivt25%25%20%
Små stormförhållanden10%10%05%
Svåra stormförhållanden01%01%01%

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