Viendo archivo del sábado, 9 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 09 2245 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 161 Publicado el 2200Z a las 09 Jun 2012 :::::::::Corrected Copy:::::::::::

IA. Análisis de regiones solares activas y de actividad desde 08-2100Z hasta 09-2100Z

Solar activity was moderate. Region 1499 (N16W31) was the most active region producing two M-class x-ray events. The first event was an impulsive M1 flare at 09/1132Z and the second was also an impulsive M1/Sf event which occurred at 09/1645Z. Region 1499 also produced several C1 events at 09/0308Z, 1032Z, and 1527Z. Region 1499 was classified as a Cao type group with beta-gamma magnetic characteristics. New Region 1504 (S18E67) was numbered today and classified as a Cao type group with beta magnetic characteristics. New Region 1505(S09E63) was also numbered today and classified as a Axx type group with alpha magnetic characteristics. There were no earth-directed CMEs observed during the period.
IB. Pronóstico de la actividad solar
Solar activity is expected to remain low with an increasing chance for occasional M-class activity for the next three days (10-12 June).
IIA. Resumen de la actividad geofísica 08-2100Z a 09-2100Z
The geomagnetic field activity was mostly quiet. A weak disturbance was observed on both ground and GOES magnetometers at 09/1841Z leading to the single unsettled period of the day. Solar wind speed at the ACE spacecraft continued to decline and ended the period near 440 km/s. The Bz component of the interplanetary magentic field remained mostly neutral or positive. The greater than 2 MeV electron flux at geosynchronous orbit reached high levels during the period.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be quiet to unsettled for the next three days (10-12 June) with the anticiapted glancing blows from CMEs on 06 June and 08 June and the arrival on 11 June of a coronal hole high speed stream.
III. Probabilidades del evento 10 Jun a 12 Jun
Clase M45%50%55%
Clase X01%01%01%
Protón01%01%01%
PCAFGreen
IV. Penticton 10.7cm flujo
  Observado       09 Jun 128
  Previsto   10 Jun-12 Jun  130/130/130
  Media de 90 Días        09 Jun 117
V. Índices Geomagnéticos A
  Observado Afr/Ap 08 Jun  009/009
  Estimado     Afr/Ap 09 Jun  006/007
  Previsto    Afr/Ap 10 Jun-12 Jun  007/010-007/010-007/010
VI. Probabilidades de Actividad Geomagnética 10 Jun a 12 Jun
A. Latitudes Medias
Activo20%20%20%
Tormenta Menor10%10%10%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%15%15%
Tormenta Menor25%25%25%
Tormenta Mayor-Severa30%30%30%

< < Ir a la visión general diaria

Últimas noticias

Apoye 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!

23%
Apoya a SpaceWeatherLive con nuestro merchandise
Échale un ojo a nuestro merchandise

Hechos clima espacial

Último evento clase X2024/03/28X1.1
Último evento clase M2024/03/29M3.2
Últimas tormentas geomagnéticas2024/03/25Kp5 (G1)
Días sin manchas
Último día sin manchas2022/06/08
Promedio de manchas solares mensuales
febrero 2024124.7 +1.7

Efemérides*

Llamarada solar
12001X2.45
22014X1.45
32023X1.2
42024M3.2
52001M3.13
ApG
1199928G2
2200337G1
3201328G1
4200122G1
5199820G1
*desde 1994

Redes sociales