Viendo archivo del domingo, 9 enero 2011
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 2011 Jan 09 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 009 Publicado el 2200Z a las 09 Jan 2011IA. Análisis de regiones solares activas y de actividad desde 08-2100Z hasta 09-2100Z Solar activity remained at very low levels. Region 1140
(N32W49) produced a B1 flare at 09/1351Z. Region 1140 showed signs
of decay with the loss of spots in the positive-polarity field just
north of the main spot and was classified as an Hsx group. The
remaining spot groups were A- and B-types with simple magnetic
configurations, including newly numbered Regions 1144 (S16W36) and
1145 (N15E35).
IB. Pronóstico de la actividad solar
Solar activity is expected to be at
very low levels through the period (10 - 12 January).
IIA. Resumen de la actividad geofísica 08-2100Z a 09-2100Z
Geomagnetic field activity remained at quiet to unsettled levels. ACE
solar wind measurements indicated Earth remained within a recurrent
coronal hole high-speed stream. Solar wind velocities were variable
in the 554 to 648 km/s range. IMF Bt showed a gradual increase with
a peak value of 6 nT observed late in the period. IMF Bz was
variable and ranged from +5 to -4 nT during the period. The greater
than 2 MeV electron flux at geosynchronous orbit reached high levels
during the period.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is
expected to be at quiet to unsettled levels during day 1 (10
January) as the coronal hole high-speed stream persists. Field
activity is expected to decrease to quiet levels during days 2 - 3
(11 - 12 January) as the high-speed stream subsides.
III. Probabilidades del evento 10 Jan a 12 Jan
| Clase M | 01% | 01% | 01% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Penticton 10.7cm flujo
Observado 09 Jan 083 Previsto 10 Jan-12 Jan 082/082/080 Media de 90 Días 09 Jan 084
V. Índices Geomagnéticos A
Observado Afr/Ap 08 Jan 006/007 Estimado Afr/Ap 09 Jan 004/005 Previsto Afr/Ap 10 Jan-12 Jan 007/008-005/005-005/005
VI. Probabilidades de Actividad Geomagnética 10 Jan a 12 Jan
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 10% | 05% |
| Tormenta Menor | 05% | 01% | 01% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 25% | 15% | 10% |
| Tormenta Menor | 10% | 05% | 01% |
| 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
AR3654 24Unspecified geomagnetic activity 954Unproven theories 342Changelog/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 |