Viendo archivo del domingo, 17 octubre 2010

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 2010 Oct 17 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 290 Publicado el 2200Z a las 17 Oct 2010

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

Solar activity was at low levels due to a few C-class events from Region 1112 (S20W44), the largest a C1.7 x-ray event observed at 17/0859Z. The region continued to evolve over the past 24 hours, increasing in both area and extent, while maintaining Beta-Gamma magnetic characteristics. New Region 1116 (N22W14) was numbered as a simple bi-polar spot group.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at very low to low levels all three days of the forecast period (18 - 20 October), with a chance for M-class events from evolving Region 1112.
IIA. Resumen de la actividad geofísica 16-2100Z a 17-2100Z
The geomagnetic field ranged from quiet to minor storm levels during the period. Activity was at quiet to unsettled levels until about 17/0700Z when the field became disturbed. Geomagnetic activity increased to active to minor storm levels through 17/0900Z, returning to mostly quiet levels through the remainder of the period. At about 17/0400Z, signatures at the ACE satellite indicated gradual increases in temperature, density and wind velocity. The Bz component of the interplanetary magnetic field (IMF) turned southward, and remained south for about 7 hours, reaching a maximum deflection of -7nT at 17/0737Z. The Bt component of the IMF reached a maximum of 10nT at 17/0520Z. This short-lived disturbance is thought to have been a result of a glancing blow from the slow-moving CME observed on 10 October.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at quiet to active levels all three days of the forecast period (18 - 20 October). Isolated minor storm periods are possible on 19 October. A coronal hole high speed stream (CH HSS) is expected to rotate into a geoeffective position late on 18 October, followed by a second geoeffective CH HSS likely to arrive early on 20 October. These features, coupled with possible effects from the CME observed on 14 October, expected to arrive on 19 October, are the reasons for the forecasted increase in geomagnetic activity.
III. Probabilidades del evento 18 Oct a 20 Oct
Clase M25%25%25%
Clase X01%01%01%
Protón01%01%01%
PCAFGreen
IV. Penticton 10.7cm flujo
  Observado       17 Oct 084
  Previsto   18 Oct-20 Oct  086/086/086
  Media de 90 Días        17 Oct 081
V. Índices Geomagnéticos A
  Observado Afr/Ap 16 Oct  003/006
  Estimado     Afr/Ap 17 Oct  009/013
  Previsto    Afr/Ap 18 Oct-20 Oct  008/010-012/012-008/010
VI. Probabilidades de Actividad Geomagnética 18 Oct a 20 Oct
A. Latitudes Medias
Activo20%30%20%
Tormenta Menor05%15%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo25%35%25%
Tormenta Menor15%20%15%
Tormenta Mayor-Severa01%01%01%

All times in UTC

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