Viewing archive of onsdag, 7 maj 2003

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 2003 May 07 2200 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com

USAF/NOAA rapport för sol- och geofysisk aktivitet

SDF Nummer 127 publicerat klockan 2200Z på 07 May 2003

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

Solar activity has been low. Today's flare activity consisted of occasional C-class flares, mostly from Region 348 (S34W80) and Region 349 (S14W86). The largest event of the day, however, was a C5 at 2049 UTC from a new region behind east limb at about N17. A 10 degree filament near S10W18 disappeared between 1342 UTC and 1403 UTC.
IB. Prognos för solaktivitet
Solar activity is expected to be predominantly low, but there is a fair chance for an isolated M-class event sometime during the next three days. An overall downward trend in activity levels and in the background levels is expected over the next three days with the departure of regions 348 and 349.
IIA. Sammanfattning av geofysisk aktivitet 06-2100Z till 07-2100Z
The geomagnetic field was at active to minor storm levels for most of the day. An interval of major storm levels was observed at mid and high latitudes from 0600-0900 UTC. Today's activity resulted from the persistence of a high speed solar wind stream (velocities ranging from 670 to 750 km/s) accompanied by weakly to moderately negative Bz (-5 to -10 nT). The greater than 2 MeV electron fluxes continue to be at high levels.
IIB. Prognos för geofysisk aktivitet
The geomagnetic field is expected to be mostly active for the next 24 hours, with a chance for some isolated storm intervals, as the current high speed solar wind stream is expected to continue. A slight decline in activity levels to unsettled to active is expected on the second and third days. Conditions should stay somewhat elevated relative to quiet, however, as a new coronal hole will be rotating into a geoeffective location.
III. Chans för solutbrott från 08 May till 10 May
M-klass40%30%25%
X-klass05%01%01%
Proton05%01%01%
PCAFgreen
IV. Penticton 10.7 cm Flux
  Observerad       07 May 110
  Prognoserat   08 May-10 May  105/100/095
  90 Day Mean        07 May 128
V. Geomagnetiskt A-index
  Observerad Afr/Ap 06 May  015/023
  Förväntat     Afr/Ap 07 May  032/037
  Prognoserat    Afr/Ap 08 May-10 May  015/020-012/015-012/015
VI. Chanser för geomagnetisk aktivitet från 08 May till 10 May
A. Medelhöga breddgrader
Aktivt35%30%30%
Små stormförhållanden20%15%15%
Svåra stormförhållanden05%05%05%
B. Höga breddgrader
Aktivt35%30%30%
Små stormförhållanden25%20%20%
Svåra stormförhållanden15%15%15%

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