Viendo archivo del sábado, 29 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 29 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 088 Publicado el 2200Z a las 29 MAR 1997IA. Análisis de regiones solares activas y de actividad desde 28-2100Z hasta 29-2100Z SOLAR ACTIVITY WAS VERY LOW. OCCASIONAL LOW-LEVEL
B-CLASS FLARES WERE OBSERVED. REGION 8026 (S23E46) CONTINUED TO GROW
SLOWLY DURING THE PERIOD AND HAS DEVELOPED PENUMBRA ON LEADER AND
TRAILER SPOTS. THE ACTIVITY IN THE REGION HAS SUBSIDED SOMEWHAT.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE VERY
LOW TO LOW. THERE CONTINUES TO BE A FAIR CHANCE FOR AN OCCASIONAL
C-CLASS EVENT OUT OF REGION 8026. THE CHANCES FOR M-CLASS LEVEL
ACTIVITY FROM THIS GROUP ARE SLIGHT, BUT ARE NOW CONSIDERED TO BE
NON-NEGLIGIBLE, GIVEN THE CONTINUED INCREASE OF PHOTOSPHERIC
MAGNETIC FIELD INTENSITY AND THE CONTINUED TREND OF FLUX EMERGENCE
FROM THE REGION.
IIA. Resumen de la actividad geofísica 28-2100Z a 29-2100Z
THE GEOMAGNETIC FIELD WAS MOSTLY QUIET TO UNSETTLED WITH SOME
INTERVALS OF ACTIVE CONDITIONS AT HIGH LATITUDES. THE GREATER THAN 2
MEV ELECTRON FLUXES WERE AT MODERATE TO HIGH LEVELS DURING THE
PERIOD.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE PREDOMINANTLY UNSETTLED FOR THE NEXT THREE DAYS.
THERE MAY BE OCCASIONAL ACTIVE PERIODS AT HIGH LATITUDE SITES.
III. Probabilidades del evento 30 MAR a 01 APR
| Clase M | 05% | 05% | 05% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 29 MAR 075 Previsto 30 MAR-01 APR 076/077/078 Media de 90 Días 29 MAR 074
V. Índices Geomagnéticos A
OBSERVED AFR/AP 28 MAR 012/013 ESTIMATED AFR/AP 29 MAR 010/015 PREDICTED AFR/AP 30 MAR-01 APR 010/015-010/012-012/010
VI. Probabilidades de Actividad Geomagnética 30 MAR a 01 APR
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 15% | 25% |
| Tormenta Menor | 05% | 05% | 15% |
| Tormenta Mayor-Severa | 01% | 01% | 05% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 20% | 20% | 25% |
| Tormenta Menor | 10% | 10% | 15% |
| Tormenta Mayor-Severa | 05% | 05% | 05% |
All times in UTC
< < Ir a la visión general diaria
Últimas noticias
viernes, 17 mayo 2024
Let's compare! Halloween 2003 VS May 2024 Solar Storms!
viernes, 17 mayo 2024
Coronal mass ejection impact, New website feature!
miércoles, 15 mayo 2024
More X-flares!
Últimos mensajes del foro
Unproven theories 481May 2024 Geomagnetic Storms from AR 13664 (2) 316"It Was Fake, It Was HAARP" - What? 7Don't we need better high geomagnetic parameters? 7What makes AR3684 magnetically distinct from AR3685? 2
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 | 2024/05/15 | X2.9 |
| Último evento clase M | 2024/05/17 | M7.1 |
| Últimas tormentas geomagnéticas | 2024/05/17 | Kp6 (G2) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| abril 2024 | 136.5 +31.6 |
| mayo 2024 | 157.2 +20.7 |
| Last 30 days | 174.3 +64.2 |