Viendo archivo del sábado, 8 marzo 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 Mar 08 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 067 Publicado el 2200Z a las 08 Mar 2003IA. Análisis de regiones solares activas y de actividad desde 07-2100Z hasta 08-2100Z Solar activity increased to low levels today. The
largest flare during the period was a C2.6/Sf event that occurred in
Region 206 (N05E63) at 08/0957Z. White light currently shows this
group to consist of a single large penumbral spot which may share
both polarities. Will be able to better analyze once region rotates
further onto disk. A C1.0 flare was observed from Region 301
(N22W18) at 08/0116Z. There was little in the way of magnetic
structure changes seen in this region during the period. Region 297
(S14W25) produced a couple low level B-class flares today. Regions
307 (S26W02) and 308 (n08E75) were newly assigned today.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at
low levels. There is a small chance for an isolated M-class flare
from Region 296 (N13W31).
IIA. Resumen de la actividad geofísica 07-2100Z a 08-2100Z
The geomagnetic field has been at quiet to unsettled levels. There
was an isolated active period at mid latitudes in response to a
southward oscillation in the Bz component of the interplanetary
magnetic field between 08/1500 and 1800Z. The coronal hole high
speed stream that has been geoeffective for the past several days
appears to have rotated out of its favorable position early in the
period. The greater than 2 MeV electron fluxes at geosynchronous
orbit reached high levels again today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to continue at quiet to unsettled levels throughout the
period.
III. Probabilidades del evento 09 Mar a 11 Mar
| Clase M | 20% | 20% | 20% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 08 Mar 148 Previsto 09 Mar-11 Mar 150/150/145 Media de 90 Días 08 Mar 142
V. Índices Geomagnéticos A
Observado Afr/Ap 07 Mar 013/014 Estimado Afr/Ap 08 Mar 008/009 Previsto Afr/Ap 09 Mar-11 Mar 008/010-007/010-007/008
VI. Probabilidades de Actividad Geomagnética 09 Mar a 11 Mar
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 20% | 15% | 15% |
| Tormenta Menor | 01% | 01% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 25% | 25% | 20% |
| Tormenta Menor | 10% | 10% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
< < 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
Unspecified geomagnetic activity 949AR3654 9Changelog/Featurelog 154What are these long and thin eruptions? 9IMF - BT strength 8
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 | 2024/04/27 | M2.1 |
| Últimas tormentas geomagnéticas | 2024/04/26 | Kp5+ (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| marzo 2024 | 104.9 -19.8 |
| Last 30 days | 136.8 +28.6 |