Viendo archivo del viernes, 14 abril 2000
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 2000 Apr 14 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 105 Publicado el 2200Z a las 14 APR 2000IA. Análisis de regiones solares activas y de actividad desde 13-2100Z hasta 14-2100Z SOLAR ACTIVITY REMAINED AT LOW LEVELS. REGION 8948
(S15W63) PRODUCED A LONG-DURATION C1 PARALLEL-RIBBON FLARE AT
13/2130Z ASSOCIATED WITH A SMALL FILAMENT DISAPPEARANCE AND A
PARTIAL-HALO CME. THIS REGION, WHICH REMAINED IN A STATE OF GRADUAL
DECAY, ALSO PRODUCED A C7/1F FLARE AT 14/0816Z. REGIONS 8955
(S22E33) AND 8960 (N19W31) SHOWED MINOR GROWTH DURING THE PERIOD.
THE REMAINING REGIONS WERE STABLE. NO NEW REGIONS WERE ASSIGNED.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE LOW.
THERE IS A FAIR BUT DIMINISHING CHANCE FOR AN ISOLATED LOW-LEVEL
M-CLASS FLARE FROM REGION 8948.
IIA. Resumen de la actividad geofísica 13-2100Z a 14-2100Z
GEOMAGNETIC FIELD ACTIVITY WAS AT MOSTLY QUIET LEVELS. THE GREATER
THAN 2 MEV ELECTRON FLUX AT GEOSYNCHRONOUS ORBIT WAS AT MODERATE TO
HIGH LEVELS.
IIB. Pronóstico de la actividad geofísica
GEOMAGNETIC FIELD ACTIVITY IS
EXPECTED TO INCREASE TO MOSTLY ACTIVE LEVELS ON 16 APRIL IN RESPONSE
TO THE PARTIAL-HALO CME MENTIONED ABOVE. UNSETTLED CONDITIONS ARE
EXPECTED FOR THE REMAINDER OF THE PERIOD. THE GREATER THAN 2 MEV
ELECTRON FLUX IS EXPECTED TO DECREASE TO NORMAL TO MODERATE LEVELS
SOMETIME DURING THE PERIOD.
III. Probabilidades del evento 15 APR a 17 APR
| Clase M | 30% | 30% | 25% |
| Clase X | 05% | 05% | 01% |
| Protón | 05% | 05% | 01% |
| PCAF | GREEN | ||
IV. Penticton 10.7cm flujo
Observado 14 APR 165 Previsto 15 APR-17 APR 165/160/160 Media de 90 Días 14 APR 184
V. Índices Geomagnéticos A
OBSERVED AFR/AP 13 APR 003/008 ESTIMATED AFR/AP 14 APR 003/004 PREDICTED AFR/AP 15 APR-17 APR 012/012-018/020-010/012
VI. Probabilidades de Actividad Geomagnética 15 APR a 17 APR
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 30% | 40% | 30% |
| Tormenta Menor | 10% | 20% | 10% |
| Tormenta Mayor-Severa | 01% | 05% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 35% | 45% | 35% |
| Tormenta Menor | 20% | 25% | 20% |
| Tormenta Mayor-Severa | 05% | 10% | 05% |
< < Ir a la visión general diaria
Últimas noticias
sábado, 23 marzo 2024
X1.1 solar flare with earth-directed CME
miércoles, 20 marzo 2024
Sunspot region 3615, G1 watch
jueves, 22 febrero 2024
X6.3 solar flare
Últimos mensajes del foro
C5.6 12/04/2024 CME 35AR3639 13AR 3637, 3638, 3643 29Space Weather Memes 333Where to find data for current polarity on the northern hemisphere of the sun? 27
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 | 2024/04/16 | M1.1 |
| Últimas tormentas geomagnéticas | 2024/03/25 | Kp5 (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| marzo 2024 | 104.9 -19.8 |