Viendo archivo del martes, 5 junio 2012
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 2012 Jun 05 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 157 Publicado el 2200Z a las 05 Jun 2012IA. Análisis de regiones solares activas y de actividad desde 04-2100Z hasta 05-2100Z Solar activity was low during the past 24 hours. Region
1499 (N15E17) produced the largest x-ray event of the period with a
C4/2f at 05/2059Z. New Region 1503 (N11W38) was numbered today and
is considered a Bxo-beta type spot group. No Earth-directed CMEs
were observed during the period.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low
with a slight chance for an isolated M-class event for the next
three days (06-08 June).
IIA. Resumen de la actividad geofísica 04-2100Z a 05-2100Z
The geomagnetic field has been unsettled to active during the past 24
hours due to continued effects from a favorably positioned coronal
hole high speed stream (CH HSS). Solar wind speeds increased from
approximately 650 km/s to 750 km/s and the interplanetary magnetic
field (IMF) Bt remained stable at about 8 nT. The Bz component of
the IMF varied between +6 and -7 nT but held steady at approximately
-5 nT for the last 2 hours of the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to be unsettled with active periods likely on day one (06
June) due to continued effects from the CH HSS. Quiet to unsettled
conditions, with a chance for isolated active periods, are expected
on days two and three (07-08 June) as the CH HSS effects subside.
III. Probabilidades del evento 06 Jun a 08 Jun
| Clase M | 15% | 15% | 15% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 05 Jun 139 Previsto 06 Jun-08 Jun 140/140/140 Media de 90 Días 05 Jun 117
V. Índices Geomagnéticos A
Observado Afr/Ap 04 Jun 014/018 Estimado Afr/Ap 05 Jun 014/018 Previsto Afr/Ap 06 Jun-08 Jun 014/018-011/015-007/008
VI. Probabilidades de Actividad Geomagnética 06 Jun a 08 Jun
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 40% | 30% | 20% |
| Tormenta Menor | 20% | 10% | 10% |
| Tormenta Mayor-Severa | 05% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 10% | 15% | 15% |
| Tormenta Menor | 30% | 25% | 25% |
| Tormenta Mayor-Severa | 55% | 40% | 30% |
< < 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
IMF - BT strength 5What are these long and thin eruptions? 6AR 3637, 3638, 3643 89Unproven theories 341Space Weather Memes 338
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 | 2024/04/25 | M1.3 |
| Últimas tormentas geomagnéticas | 2024/04/19 | Kp7 (G3) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| marzo 2024 | 104.9 -19.8 |
| Last 30 days | 135.5 +27.6 |