Viendo archivo del sábado, 22 enero 2005

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 2005 Jan 22 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 022 Publicado el 2200Z a las 22 Jan 2005

IA. Análisis de regiones solares activas y de actividad desde 21-2100Z hasta 22-2100Z

Solar activity was low during the past 24 hours. There were three C-class flares: a C3 at 0432 UTC from the west limb at S07, a C1 at 1245 UTC from the west limb at N14, and a C1 at 2053 UTC from the west limb at N15. The first flare was probably from old Region 719 which recently rotated around west limb, and the other two were probably from Region 720 which rotated off the disk today. With the departure of Region 720, Region 725 (S04W49) is now the largest group on the disk with an area of about 190 millionths. Region 725 has been growing steadily but so far has produced only minor flare activity.
IB. Pronóstico de la actividad solar
Solar activity is expected to be mostly low. There is a chance for an M-class event, and a slight chance for a major flare event, from Region 720 during the next 24 hours (23 January). However, the likelihood for M-class or higher level events is expected to decline strongly for the 2nd and 3rd days (24-25 January) as the region gets further beyond the west limb.
IIA. Resumen de la actividad geofísica 21-2100Z a 22-2100Z
The geomagnetic field was at active to major storm levels from the beginning of the period (21/2100 UTC) through 22/0600 UTC. Since 0600 UTC conditions have been mostly unsettled. Solar wind signatures show a steady decline in velocity from around 950 km/s at the beginning of the interval down to about 650 km/s by 22/2100 UTC. Bz has been weak and density has been low since 22/0200 UTC up to the current time. The greater than 10 MeV proton fluxes continued to decline today and appear to have dropped below threshold of 10 PFU after 22/1755 UTC.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be mostly active tomorrow (23 January) in response to a favorably positioned coronal hole. Mostly unsettled levels with some active periods are expected for 24-25 January.
III. Probabilidades del evento 23 Jan a 25 Jan
Clase M40%25%10%
Clase X20%10%01%
Protón20%10%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       22 Jan 102
  Previsto   23 Jan-25 Jan  095/090/090
  Media de 90 Días        22 Jan 108
V. Índices Geomagnéticos A
  Observado Afr/Ap 21 Jan  030/061
  Estimado     Afr/Ap 22 Jan  020/030
  Previsto    Afr/Ap 23 Jan-25 Jan  016/020-015/015-015/015
VI. Probabilidades de Actividad Geomagnética 23 Jan a 25 Jan
A. Latitudes Medias
Activo30%25%25%
Tormenta Menor20%15%15%
Tormenta Mayor-Severa10%05%05%
B. Latitudes Altas
Activo35%35%30%
Tormenta Menor30%30%25%
Tormenta Mayor-Severa10%05%05%

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