Viendo archivo del sábado, 9 noviembre 2002
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 2002 Nov 09 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 313 Publicado el 2200Z a las 09 Nov 2002 ::::::::CORRECTED COPY::::::::IA. Análisis de regiones solares activas y de actividad desde 08-2100Z hasta 09-2100Z Solar activity was moderate. Region 180 (S10W41)
produced an M4/2B flare at 09/1323 UTC. The flare was accompanied by
type II/IV radio sweeps, a 760 sfu burst at 2695 MHz, and an
apparent earth-directed CME. Otherwise only C-class flares occurred,
mostly in Region 180 but also from Region 191 (S17E63).
IB. Pronóstico de la actividad solar
Solar activity is expected to be low
to moderate. Region 180 is the most likely source of energetic
flares with a slight chance of M-level activity in 191.
IIA. Resumen de la actividad geofísica 08-2100Z a 09-2100Z
The geomagnetic field was quiet to unsettled. The field became
somewhat disturbed after 09/1800 UTC in response to a shock observed
in the solar wind at about 09/1755 UTC. Further analysis of the
solar wind data since 09/2100 UTC suggests that this structure is
CME material rather than related to a high-speed stream as suggested
in the original filing of this report. A greater than 10 MeV proton
event began at 09/1920 UTC, following the M4 flare mentioned in Part
IA, and remains in progress. The current greater than 10 MeV proton
flux is about 30 pfu. The greater than 2 MeV electron flux at
geosynchronous orbit was moderate to high.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be mostly unsettled for the next 24-36 hours. Active
conditions are expected late on 11 November in response to the
M4/CME which occurred today. The greater than 10 MeV proton event is
expected to continue.
III. Probabilidades del evento 10 Nov a 12 Nov
| Clase M | 50% | 50% | 50% |
| Clase X | 10% | 10% | 10% |
| Protón | 90% | 10% | 05% |
| PCAF | yellow | ||
IV. Penticton 10.7cm flujo
Observado 09 Nov 191 Previsto 10 Nov-12 Nov 185/180/180 Media de 90 Días 09 Nov 178
V. Índices Geomagnéticos A
Observado Afr/Ap 08 Nov 003/008 Estimado Afr/Ap 09 Nov 008/012 Previsto Afr/Ap 10 Nov-12 Nov 010/012-015/015-020/020
VI. Probabilidades de Actividad Geomagnética 10 Nov a 12 Nov
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 20% | 30% |
| Tormenta Menor | 05% | 10% | 20% |
| Tormenta Mayor-Severa | 01% | 05% | 10% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 15% | 25% | 35% |
| Tormenta Menor | 10% | 15% | 25% |
| Tormenta Mayor-Severa | 01% | 05% | 10% |
< < Ir a la visión general diaria
Últimas noticias
lunes, 22 abril 2024
Lot's of sunspots! Big chance for major flare activity?
sábado, 23 marzo 2024
X1.1 solar flare with earth-directed CME
miércoles, 20 marzo 2024
Sunspot region 3615, G1 watch
Últimos mensajes del foro
Unproven theories 336Space Weather Memes 336Growth of Cycle 25 433Filaments and prominences 54Sporadic E and Flare activity 17
Más temasApoye a SpaceWeatherLive.com!
Mucha gente viene a SpaceWeatherLive para seguir la actividad del Sol o previsión de aurora, pero con esta cantidad de tráfico se incrementan los costos del servidor. ¡Considere hacer una donación si disfruta de SpaceWeatherLive para que podamos mantener el sitio web en línea!
Hechos clima espacial
| Último evento clase X | 2024/03/28 | X1.1 |
| Último evento clase M | 2024/04/23 | M3.0 |
| Últimas tormentas geomagnéticas | 2024/04/19 | Kp7 (G3) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| marzo 2024 | 104.9 -19.8 |
| Last 30 days | 125.4 +21.1 |