Viendo archivo del martes, 1 abril 2003
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 2003 Apr 01 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.comInforme conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 091 Publicado el 2200Z a las 01 Apr 2003
IA. Análisis de regiones solares activas y de actividad desde 31-2100Z hasta 01-2100Z
Solar activity was at low levels. There were only two
C-class flares from Regions 323 (S08W43) and 318 (S12W65).
IB. Pronóstico de la actividad solar
Solar activity is expected to be low.
There is a small chance for an isolated M-Class flare from either
Region 323 (S08W43), Region 325 (N12E14), or Region 324 (S11W08).
IIA. Resumen de la actividad geofísica 31-2100Z a 01-2100Z
The geomagnetic field was at quiet to minor storm levels, with
occasional major storming at high latitudes. The high speed stream
that began early on 30 March continued during the period. The
greater than 2 MeV electrons at geosynchronous orbit reached high
levels.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at quiet to unsettled levels. The high speed stream
which has impacted earth for the previous two days will pass by day
two.
III. Probabilidades del evento 02 Apr a 04 Apr
Clase M | 30% | 30% | 30% |
Clase X | 05% | 05% | 05% |
Protón | 01% | 01% | 01% |
PCAF | green
|
IV. Penticton 10.7cm flujo
Observado 01 Apr 153
Previsto 02 Apr-04 Apr 155/150/145
Media de 90 Días 01 Apr 134
V. Índices Geomagnéticos A
Observado Afr/Ap 31 Mar 015/031
Estimado Afr/Ap 01 Apr 017/015
Previsto Afr/Ap 02 Apr-04 Apr 010/012-010/010-008/010
VI. Probabilidades de Actividad Geomagnética 02 Apr a 04 Apr
A. Latitudes Medias |
Activo | 40% | 30% | 30% |
Tormenta Menor | 10% | 10% | 10% |
Tormenta Mayor-Severa | 05% | 05% | 05% |
B. Latitudes Altas |
Activo | 45% | 30% | 30% |
Tormenta Menor | 15% | 10% | 10% |
Tormenta Mayor-Severa | 10% | 05% | 05% |
VII. Comments: Beginning 1500 UTC April 8, SEC will begin using data from the GOES 12 satellite, and stop receiving GOES 8 data. GOES 12 has the new Solar X-Ray Imager (SXI), which will acquire real-time, operational images of the solar x-ray flux. With the switch from GOES 8 to GOES 12, the primary/secondary designations will change. GOES 12 will be the primary satellite for the SXI. All other data, including magnetometer, XRS x-ray measurements, and energetic particles, will have GOES 10 as their primary source, with GOES 12 as the secondary source where available. Please see http://www.sec.noaa.gov/GOES.html for important information on this changeover.
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