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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 2012 May 10 2200 UTC
Skapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com

USAF/NOAA rapport för sol- och geofysisk aktivitet

SDF Nummer 131 publicerat klockan 2200Z på 10 May 2012

IA. Analys av solfläcksgrupper och solaktivitet från 09-2100Z till 10-2100Z

Solar activity has been at high levels for the past 24 hours with multiple M-class solar flares observed. Region 1476 (N12E08) was responsible for almost all of the activity with 3 M-class events observed, the largest being a M5/2b event at 10/0418Z. Associated with these events, were discrete frequency radio bursts, Tenflares, and even a Type IV radio sweep. Region 1476 has shown mixed growth and shear effects across the polarities as it continues to evolve. A weak Earth directed CME was observed in STEREO COR2 A and B imagery early in the period. Analysis and current models show this CME joining the current coronal hole high speed stream (CH HSS). Region 1477 (S22E47) was split into two regions today as SDO magnetogram data indicated the leader and follower sunspot groups were actually two magnetic bipoles. Leader group is Region 1477 and follower group is now Region 1478 (S24E55).
IB. Prognos för solaktivitet
Solar activity is expected to be at moderate levels with a slight chance for X-class events for the next three days (11 - 13 May) as Region 1476 continues to grow and evolve.
IIA. Sammanfattning av geofysisk aktivitet 09-2100Z till 10-2100Z
The geomagnetic field has been at quiet to active levels for the past 24 hours with an isolated minor storm period observed at high latitudes. Solar wind measurements, as observed by the ACE spacecraft, showed a continued increase in solar wind speeds to around 620 km/s, a drop off in solar wind density, and the total IMF began to stabilize around 5 nT. These characteristics are indicative of a CH HSS. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Prognos för geofysisk aktivitet
The geomagnetic field is expected to be at quiet to unsettled levels with a chance for active periods for the next three days (11 - 13 May). The increased activity is due to both the continued CH HSS effects and three weak, slow moving CMEs intertwined within.
III. Chans för solutbrott från 11 May till 13 May
M-klass75%75%75%
X-klass20%20%20%
Proton10%10%10%
PCAFGreen
IV. Penticton 10.7 cm Flux
  Observerad       10 May 131
  Prognoserat   11 May-13 May  130/130/130
  90 Day Mean        10 May 113
V. Geomagnetiskt A-index
  Observerad Afr/Ap 09 May  019/025
  Förväntat     Afr/Ap 10 May  010/010
  Prognoserat    Afr/Ap 11 May-13 May  012/012-010/012-006/010
VI. Chanser för geomagnetisk aktivitet från 11 May till 13 May
A. Medelhöga breddgrader
Aktivt20%20%15%
Små stormförhållanden05%05%01%
Svåra stormförhållanden01%01%01%
B. Höga breddgrader
Aktivt40%40%30%
Små stormförhållanden10%10%10%
Svåra stormförhållanden01%01%01%

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