Visualització de l'arxiu de divendres, 27 de gener 2012

Informe d'activitat solar

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.
Informe d'activitat Geofísica-Solar 2012 Jan 27 2200 UTC
Preparat pel SWPC NOAA © i processat per SpaceWeatherLive.com

Informe conjunt segons USAF / NOAA d’activitat Solar i Geofísica

SDF número 027 emès a 2200Z el Jan 27 2012

IA. Anàlisi de les regions actives solars i de l'activitat de 2100Z-26 a 2100Z-27

Solar activity was high. Region 1402 (N29W88) produced an X1/1f flare at 27/1837Z with associated Type II (est. speed 1523 km/s) and Type IV Radio Sweeps, along with an 810 pfu Tenflare. An associated CME was first visible in SOHO/LASCO C2 imagery at 27/1827Z. The majority of the ejecta is directed towards the STEREO A spacecraft, however, further analysis is necessary to determine potential geoeffectiveness.
IB. Previsió d'activitat solar
Solar activity is expected to be low on day one (28 January) with a chance for isolated M-class activity as Region 1402 rotates around the west limb. Activity is expected to be very low to low on days two and three (29-30 January).
IIA. Resum d'activitat geofísica del 2100Z-26 al 2100Z-27
The geomagnetic field was quiet to unsettled with isolated active periods observed at mid-latitudes and an isolated minor storm period observed at high latitudes. The increase in activity is due to the arrival of a recurrent coronal hole high speed stream (CH HSS). The greater than 10 MeV and greater than 100 MeV proton flux at geosynchronous orbit were above event threshold during the period due to the X1 flare mentioned above. The greater than 10 MeV proton event, which began at 27/1905Z and reached 96 pfu at the time of this writing, is still in progress. The greater than 100 MeV proton event, which began at 27/1900Z and reached 11 pfu at the time of this writing, is also still in progress. The Penticton 10.7 cm flux value was enhanced due to the X1 flare mentioned above. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Previsió d'activitat geofísica
The geomagnetic field is expected to be quiet to unsettled on day one (28 January) due to continued effects from the CH HSS. Mostly quiet conditions are expected for days two and three (29-30 January). The greater than 10 MeV and 100 MeV proton events are expected to continue on day one. A more reliable end time will be possible once the peak levels are observed.
III. Probabilitats d’esdeveniments de les Jan del 28 a les Jan del 30
Classe M25%01%01%
Classe X05%01%01%
Protó99%50%01%
PCAFRed
IV. Penticton Flux de 10,7 cm
  Observat       27 Jan 142
  Predit   28 Jan-30 Jan  120/120/120
  Mitjana de 90 dies        27 Jan 144
V. Índexs geomagnètics A
  Observat Afr/Ap 26 Jan  005/006
  Estimat     Afr/Ap 27 Jan  007/008
  Predit    Afr/Ap 28 Jan-30 Jan  007/008-005/005-005/005
VI. Probabilitats d’activitat geomagnètica del 28 Jan al 30 Jan
A. Latituds mitjanes
Actiu20%10%10%
Tempesta menor10%01%01%
Tempesta major-severa01%01%01%
B. Latituds altes
Actiu25%15%15%
Tempesta menor15%01%01%
Tempesta major-severa05%01%01%

All times in UTC

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