Viewing archive of tisdag, 20 januari 2004

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 2004 Jan 20 2200 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com

USAF/NOAA rapport för sol- och geofysisk aktivitet

SDF Nummer 020 publicerat klockan 2200Z på 20 Jan 2004

IA. Analys av solfläcksgrupper och solaktivitet från 19-2100Z till 20-2100Z

Solar activity was high. Region 540 (S14W22) produced an M6/2n flare at 20/0743Z. Radio bursts associated with this flare included a 4500 sfu burst on 245 MHz and Type II sweep with a shock speed of 950 km/s. A CME was visible on LASCO imagery. Region 540 also produced an impressive long duration C5 flare that occurred between 19/2202Z through 20/0229Z, peaking at 20/0045Z. A full halo CME was observed with this event. Soon after the eruption in Region 540, segments of the large circular filament in the northwest quadrant also erupted. Region 540 maintains a weak delta configuration in its trailing spots, but further decay in total area was also noted. The trailing spots in Region 542 (N10W03) have been identified as a separate region and were numbered as Region 544.
IB. Prognos för solaktivitet
Solar activity is expected to be low to moderate. Though in decay, Region 540 still maintains potential for isolated M-class flares. The remaining three spot groups on the visible disk have potential for C-class activity.
IIA. Sammanfattning av geofysisk aktivitet 19-2100Z till 20-2100Z
The geomagnetic field was quiet to active. Solar wind speed is in gradual decline as a large transequatorial coronal hole rotates out of a geoeffective position. Solar wind speed decreased to near 500 km/s, but periods of southward Bz generated occasional active periods. 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 range from quiet to major storming over the next three days. Quiet to active periods are expected on 21 January. The full halo CME observed on LASCO imagery at 20/0006Z will likely impact the geomagnetic field early on 22 January. Active to major storm periods are possible. Unsettled to active conditions are expected on January 23 as the storm subsides.
III. Chans för solutbrott från 21 Jan till 23 Jan
M-klass30%30%30%
X-klass05%05%05%
Proton05%05%05%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observerad       20 Jan 129
  Prognoserat   21 Jan-23 Jan  130/130/130
  90 Day Mean        20 Jan 138
V. Geomagnetiskt A-index
  Observerad Afr/Ap 19 Jan  010/017
  Förväntat     Afr/Ap 20 Jan  018/022
  Prognoserat    Afr/Ap 21 Jan-23 Jan  012/015-035/045-015/025
VI. Chanser för geomagnetisk aktivitet från 21 Jan till 23 Jan
A. Medelhöga breddgrader
Aktivt25%45%35%
Små stormförhållanden10%25%15%
Svåra stormförhållanden05%15%05%
B. Höga breddgrader
Aktivt30%45%40%
Små stormförhållanden15%35%20%
Svåra stormförhållanden05%20%10%

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