Viendo archivo del martes, 4 septiembre 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 Sep 04 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 248 Publicado el 2200Z a las 04 Sep 2012

IA. Análisis de regiones solares activas y de actividad desde 03-2100Z hasta 04-2100Z

Solar activity was low. Region 1564 (S14E14 - Esi/beta-gamma) was the most active region, producing occasional low-level C-class flares. It increased in spot count and area during the first half of the period, but showed gradual spot and penumbral decay during the latter half of the period. Region 1560 (N04W47 - Eai/beta-gamma-delta) showed a slight decrease in spots and area, but maintained a delta in its interior spots. No significant changes were observed in the remaining spotted regions and no new regions were numbered. No Earth-directed CME activity was observed during the period.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low through the period (05 - 07 September) with a chance for an isolated M-class flare.
IIA. Resumen de la actividad geofísica 03-2100Z a 04-2100Z
Geomagnetic field activity ranged from quiet to minor storm levels with major storm periods detected at high latitudes, all due to residual CME effects. The greater than 10 MeV proton event at geosynchronous orbit that began at 01/1335Z, reached a maximum of 59 pfu at 02/0850Z, and ended at 04/0625Z.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is expected to be at quiet to unsettled levels during days 1 - 2 (05 - 06 September) with a chance for active levels. This is due to the arrival of CMEs observed on 02 September along with a co-rotating interaction region in advance of a coronal hole high-speed stream (CH HSS). The CMEs are expected to arrive around midday on day 1. The CH HSS is expected to commence on day 2. Field activity is expected to be at quiet to unsettled levels on day 3 (07 September) as CH HSS effects subside.
III. Probabilidades del evento 05 Sep a 07 Sep
Clase M25%25%25%
Clase X01%01%01%
Protón01%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       04 Sep 138
  Previsto   05 Sep-07 Sep  135/135/130
  Media de 90 Días        04 Sep 124
V. Índices Geomagnéticos A
  Observado Afr/Ap 03 Sep  023/040
  Estimado     Afr/Ap 04 Sep  012/014
  Previsto    Afr/Ap 05 Sep-07 Sep  010/012-010/010-007/008
VI. Probabilidades de Actividad Geomagnética 05 Sep a 07 Sep
A. Latitudes Medias
Activo20%15%15%
Tormenta Menor05%05%01%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%15%15%
Tormenta Menor30%20%25%
Tormenta Mayor-Severa30%25%20%

All times in UTC

< < Ir a la visión general diaria

Últimas noticias

Apoye a SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Suscripciones
Donations
Apoye a SpaceWeatherLive.com! Donar
Apoya a SpaceWeatherLive con nuestro merchandise
Échale un ojo a nuestro merchandise

Hechos clima espacial

Último evento clase X18/01/2026X1.9
Último evento clase M21/01/2026M3.4
Últimas tormentas geomagnéticas22/01/2026Kp5+ (G1)
Días sin manchas
Último día sin manchas08/06/2022
Promedio de manchas solares mensuales
diciembre 2025124 +32.2
enero 2026118.7 -5.3
Last 30 days120.4 +5.6

Efemérides*

Llamarada solar
12014M7.04
22014M5.27
32014M5.01
42014M3.79
52001M2.27
DstG
11985-125G2
21971-97G2
31972-56G1
41980-55G1
51982-47
*desde 1994

Redes sociales