Viendo archivo del domingo, 2 marzo 1997
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 1997 Mar 02 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 061 Publicado el 2200Z a las 02 MAR 1997IA. Análisis de regiones solares activas y de actividad desde 01-2100Z hasta 02-2100Z THE VISIBLE DISK REMAINED SPOTLESS AND SOLAR ACTIVITY
REMAINED VERY LOW.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY SHOULD CONTINUE AT VERY
LOW LEVELS FOR THE NEXT THREE DAYS.
IIA. Resumen de la actividad geofísica 01-2100Z a 02-2100Z
THE GEOMAGNETIC FIELD BEGAN THE PERIOD WITH QUIET CONDITIONS.
GENERALLY ACTIVE LEVELS WERE OBSERVED FROM 02/0300-1200Z. SOME HIGH
LATITUDE SITES EXPERIENCED STORM CONDITIONS DURING THAT INTERVAL.
THE FIELD RETURNED TO QUIET CONDITIONS FOR THE REMAINDER OF THE
PERIOD. WHEN COMPARED TO 01 MAR, SOLAR WIND VELOCITY DECREASED BY
ABOUT 100 KM/S DURING THE PERIOD. ENERGETIC ELECTRON FLUXES AT
GEOSYNCHRONOUS ORBIT WERE HIGH.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS
FORECAST TO BE QUIET TO UNSETTLED FOR THE NEXT THREE DAYS. ISOLATED
ACTIVE CONDITIONS ARE POSSIBLE DURING THAT TIME.
III. Probabilidades del evento 03 MAR a 05 MAR
| Clase M | 01% | 01% | 01% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 02 MAR 072 Previsto 03 MAR-05 MAR 072/072/072 Media de 90 Días 02 MAR 075
V. Índices Geomagnéticos A
OBSERVED AFR/AP 01 MAR 011/010 ESTIMATED AFR/AP 02 MAR 011/012 PREDICTED AFR/AP 03 MAR-05 MAR 010/010-010/010-010/010
VI. Probabilidades de Actividad Geomagnética 03 MAR a 05 MAR
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 10% | 10% |
| Tormenta Menor | 10% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 15% | 10% | 10% |
| Tormenta Menor | 10% | 05% | 05% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
All times in UTC
< < Ir a la visión general diaria
Últimas noticias
domingo, 1 febrero 2026
Complex sunspot region 4366
lunes, 19 enero 2026
CME impact! S4 solar radiation storm
domingo, 18 enero 2026
X1.9 solar flare with earth-directed CME
Últimos mensajes del foro
AR 4373 13Do the high-resolution sunspot counts point to more complex sunspots? 68Feb 8-9 CMEs 31Richard Carrington 1Yes, we really went to the moon before. 7
Más temasApoye a SpaceWeatherLive.com!
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
Hechos clima espacial
| Último evento clase X | 04/02/2026 | X4.3 |
| Último evento clase M | 13/02/2026 | M1.0 |
| Últimas tormentas geomagnéticas | 05/02/2026 | Kp5+ (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| enero 2026 | 112.6 -11.4 |
| febrero 2026 | 121.7 +9.1 |
| Last 30 days | 131.5 +34.7 |