Viendo archivo del jueves, 10 enero 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 Jan 10 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 010 Publicado el 2200Z a las 10 Jan 2002IA. Análisis de regiones solares activas y de actividad desde 09-2100Z hasta 10-2100Z Solar activity was low. Region 9773 (N14W17) belied its
ominous appearance in white light and h-alpha by producing just
C-class events in the past 24 hours. A C7/Sf at 1018 UTC was the
largest event, although the x-ray background from GOES was enhanced
throughout the day. The region measures more than 500 millionths in
white light, and retains a significant degree of magnetic
complexity. Elsewhere, Region 9778 (S17E45) grew in most parameters
and produced occasional subflares.
IB. Pronóstico de la actividad solar
Solar activity is expected to be
moderate. Region 9773 is capable of M class activity.
IIA. Resumen de la actividad geofísica 09-2100Z a 10-2100Z
The geomagnetic field varied from quiet to minor storm levels. A high
speed solar wind stream began to impact the magnetosphere early in
the period, with solar wind speeds increasing from 350 km/s to more
than 600 km/s. In addition, there have been intervals where the
interplanetary magnetic field has been near 20 nT southward, further
fueling the disturbance. An enhancement in the greater than 10 MeV
protons at GOES began around 0700 UTC. The flux attained event level
(10 pfu at greater than 10 MeV) at 2045 UTC. This increase may be
associated with east limb activity that occurred late on January 8.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be at active to minor storm levels. The current
disturbance should persist for the next 24-48 hours. The greater
than 10 MeV proton event is likely to slowly decay.
III. Probabilidades del evento 11 Jan a 13 Jan
| Clase M | 75% | 75% | 75% |
| Clase X | 25% | 25% | 25% |
| Protón | 75% | 50% | 25% |
| PCAF | yellow | ||
IV. Penticton 10.7cm flujo
Observado 10 Jan 225 Previsto 11 Jan-13 Jan 230/235/240 Media de 90 Días 10 Jan 223
V. Índices Geomagnéticos A
Observado Afr/Ap 09 Jan 002/003 Estimado Afr/Ap 10 Jan 015/023 Previsto Afr/Ap 11 Jan-13 Jan 020/030-015/020-015/015
VI. Probabilidades de Actividad Geomagnética 11 Jan a 13 Jan
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 50% | 50% | 50% |
| Tormenta Menor | 30% | 30% | 30% |
| Tormenta Mayor-Severa | 10% | 10% | 10% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 30% | 40% | 40% |
| Tormenta Menor | 50% | 40% | 40% |
| Tormenta Mayor-Severa | 10% | 10% | 05% |
< < 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 344AR3654 25Unspecified geomagnetic activity 954Changelog/Featurelog 154What are these long and thin eruptions? 9
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 | M3.0 |
| 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 | 137.7 +30.3 |