Viendo archivo del jueves, 19 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 19 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 201 Publicado el 2200Z a las 19 Jul 2012

IA. Análisis de regiones solares activas y de actividad desde 18-2100Z hasta 19-2100Z

Solar activity was high. Shortly after rotating off the west limb, Region 1520 (S17W90) produced a long duration M7 event with max at 19/0558Z. The event was associated with a Type II sweep (1110 km/s), a Tenflare (1000 sfu), and a Type IV sweep. A partial-halo CME was subsequently observed in SOHO/LASCO C3 coronagraph imagery beginning at 19/0606Z with an estimated plane-of-sky speed of about 1500 km/s. This CME is not expected to be geoeffective. Region 1523 (S28W64) and Region 1524 (S16W24) showed slight decay. Region 1525 (S22W23) increased over the course of the period and produced a C-flare.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low throughout the period.
IIA. Resumen de la actividad geofísica 18-2100Z a 19-2100Z
Geomagnetic field activity was generally quiet. The greater than 10 MeV proton event that began at 17/1715Z continued with an enhancement from the 19/0513 M7 event, reaching a max value of 79 PFU at 19/1425Z during the analysis interval. The greater than 2 MeV electron flux at geosynchronous orbit was at high levels throughout the period.
IIB. Pronóstico de la actividad geofísica
Geomagnetic activity is expected to be at quiet levels for the first and second days (20-21 July). An increase to unsettled levels with a chance for active periods is expected on the third day (22 July) due to a favorably positioned coronal hole. The greater than 10 MeV proton event that began 17/1715 is expected to end on 20 July.
III. Probabilidades del evento 20 Jul a 22 Jul
Clase M10%01%01%
Clase X01%01%01%
Protón90%20%01%
PCAFred
IV. Penticton 10.7cm flujo
  Observado       19 Jul 100
  Previsto   20 Jul-22 Jul  095/095/100
  Media de 90 Días        19 Jul 128
V. Índices Geomagnéticos A
  Observado Afr/Ap 18 Jul  005/004
  Estimado     Afr/Ap 19 Jul  005/006
  Previsto    Afr/Ap 20 Jul-22 Jul  006/005-006/005-011/012
VI. Probabilidades de Actividad Geomagnética 20 Jul a 22 Jul
A. Latitudes Medias
Activo05%05%30%
Tormenta Menor01%01%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%15%15%
Tormenta Menor10%10%30%
Tormenta Mayor-Severa05%05%35%

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