Viendo archivo del martes, 17 julio 2012

Informe actividad 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 de actividad Solar-Geofísica 2012 Jul 17 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 199 Publicado el 2200Z a las 17 Jul 2012

IA. Análisis de regiones solares activas y de actividad desde 16-2100Z hasta 17-2100Z

Solar activity was moderate. Todays activity was dominated by a very long-duration M1 flare that occurred between 1203-1904Z with maximum at 1715Z. The source region appeared to primarily be Region 1520 (S17W75), although it appears that Region 1521 (S19W85) was involved in the early phase and may have been the initial trigger for the overall event. An associated, bright CME was observed off the southwest limb beginning at 1400Z; the leading edge plane-of-sky speed was estimated to be about 960 km/s in the LASCO C3 field of view. The proximity of Regions 1519 (S17 just past west limb), 1520, and 1521 to the west limb hindered analysis of the spot groups. New Region 1524 (S18E52) was assigned and is a simple C-type sunspot group. An additional new spot group appeared to be emerging just south of Region 1524.
IB. Pronóstico de la actividad solar
Solar activity is expected to be moderate for the next 24 hours with 1520 and 1521 as the most likely source regions. Activity and background levels are expected to decrease significantly by the second and third days as these regions rotate beyond west limb.
IIA. Resumen de la actividad geofísica 16-2100Z a 17-2100Z
The geomagnetic field ranged from active to quiet levels with some isolated minor and major storm intervals at high latitudes. Unsettled to active levels prevailed duing the earlier part of the period and quiet to unsettled levels dominated from 17/0900Z through the end of the day. Solar wind observations from the ACE spacecraft showed continued influence of the 12 July CME from the beginning of the period through about 17/0600Z. The z-component of the interplanetary magnetic field was initially negative and reached a peak negative value of about -9 nT during this latter phase of the CME passage. Nominal solar wind conditions prevailed from 17/0600Z through the end of the day. A greater than 10 MeV proton event began at 17/1715Z in response to todays long-duration M1 and associated CME event. The peak value observed so far was 87 PFU at 17/2030Z. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be quiet for the next three days. Model results for todays CME from the west limb indicate an interplanetary disturbance that is too far west to produce geomagnetic activity. The greater than 10 MeV proton event is expected to continue through part of the first day (18 July).
III. Probabilidades del evento 18 Jul a 20 Jul
Clase M55%40%25%
Clase X10%10%05%
Protón95%20%05%
PCAFyellow
IV. Penticton 10.7cm flujo
  Observado       17 Jul 128
  Previsto   18 Jul-20 Jul  115/105/095
  Media de 90 Días        17 Jul 129
V. Índices Geomagnéticos A
  Observado Afr/Ap 16 Jul  027/040
  Estimado     Afr/Ap 17 Jul  015/020
  Previsto    Afr/Ap 18 Jul-20 Jul  006/005-007/005-006/005
VI. Probabilidades de Actividad Geomagnética 18 Jul a 20 Jul
A. Latitudes Medias
Activo05%05%05%
Tormenta Menor01%01%01%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%15%15%
Tormenta Menor10%10%10%
Tormenta Mayor-Severa05%05%05%

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