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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 Nov 25 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 330 Publicado el 2200Z a las 25 Nov 2012

IA. Análisis de regiones solares activas y de actividad desde 24-2100Z hasta 25-2100Z

Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C1 event observed at 25/2014Z from the west limb. Region 1618 (N08W55) was responsible for a B9 flare at 24/0617Z. Region 1618 was classified as an Ekc type group covering 270 millions of the visible solar disk. Further magnetic simplification was observed in Region 1618s leader spot, however it contained a delta in its larger trailing spot earlier in the period. Region 1620 (S13W14) appeared to develop gamma characteristics over the past 24 hours. New flux emergence was noted in the southeast quadrant near S17E38 and S24E30. These regions were small, simple beta type groups and will be monitored for continued development before being numbered.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at low levels on days one, two, and three (26 Nov, 27 Nov, 28 Nov) with a chance for an M-class event.
IIA. Resumen de la actividad geofísica 24-2100Z a 25-2100Z
The geomagnetic field has been at quiet levels for the past 24 hours. There were no obvious signs the 21 November CME passage in the time series data from the ACE spacecraft in the past 24 hours. Solar wind speed began rising slowly from 350 km/s around 25/0400 UTC and peaked at 487 km/s 11 hours later. The Phi angle was near 225 degrees until 25/1000 UTC when it became variable. It came to rest at 315 degrees (negative sector) about 90 minutes later. Coincident with the variable period, Bz became negative. In the hours prior, it had been between 0 and +10nT. The temperature also began rising about the same time as the wind speed, but peaked around 25/1100 UTC. The EPAM instrument reported low energy particle flux rose from around 25/0600 to 0900 UTC, but abruptly leveled off afterwards and only minor fluctuations have followed. Total IMF reached 12.3 nT at 25/0303Z. The maximum southward component of Bz reached -8.1 nT at 25/1259Z.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field should begin at mostly quiet levels with some isolated unsettled periods. WSA-ENLIL model runs place the 23 Nov CME at earth at the earliest by 15 UTC on the 26th and at the latest by about 00 UTC on the 27th. With the CME arrival, conditions are expected to be unsettled to active with a slight chance for isolated minor storm levels, particularly at high latitudes.
III. Probabilidades del evento 26 Nov a 28 Nov
Clase M30%30%30%
Clase X05%05%05%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       25 Nov 121
  Previsto   26 Nov-28 Nov 120/115/110
  Media de 90 Días        25 Nov 123

V. Índices Geomagnéticos A
  Observado Afr/Ap 24 Nov  011/015
  Estimado     Afr/Ap 25 Nov  005/006
  Previsto    Afr/Ap 26 Nov-28 Nov  009/010-013/015-008/008

VI. Probabilidades de Actividad Geomagnética 26 Nov a 28 Nov
A. Latitudes Medias
Activo20%25%10%
Tormenta Menor10%10%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%15%15%
Tormenta Menor25%25%15%
Tormenta Mayor-Severa30%35%15%

All times in UTC

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