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Informe actividad solar

Informe de actividad Solar-Geofísica 2026 May 26 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 146 Publicado el 2200Z a las 26 May 2026

IA. Análisis de regiones solares activas y de actividad desde 25-2100Z hasta 26-2100Z

Solar activity has been at low levels for the past 24 hours. There are currently 9 numbered sunspot regions on the disk.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low with a chance for M-class flares on days one, two, and three (27 May, 28 May, 29 May).
IIA. Resumen de la actividad geofísica 25-2100Z a 26-2100Z
The geomagnetic field has been at quiet to unsettled levels for the past 24 hours. Solar wind speed reached a peak of 459 km/s at 26/1918Z. Total IMF reached 9 nT at 26/1838Z. The maximum southward component of Bz reached -7 nT at 26/2021Z. Protons greater than 10 MeV at geosynchronous orbit reached a peak level of 23 pfu at 26/0110Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 455 pfu.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at quiet to active levels on days one and two (27 May, 28 May) and quiet levels on day three (29 May). Protons greater than 10 Mev have a slight chance of crossing threshold on day one (27 May).
III. Probabilidades del evento 27 May a 29 May
Clase M40%40%40%
Clase X05%05%05%
Protón10%01%01%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       26 May 141
  Previsto   27 May-29 May 145/150/145
  Media de 90 Días        26 May 125

V. Índices Geomagnéticos A
  Observado Afr/Ap 25 May  008/008
  Estimado     Afr/Ap 26 May  006/006
  Previsto    Afr/Ap 27 May-29 May  009/012-010/012-006/008

VI. Probabilidades de Actividad Geomagnética 27 May a 29 May
A. Latitudes Medias
Activo25%25%20%
Tormenta Menor10%10%05%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo20%20%20%
Tormenta Menor35%35%25%
Tormenta Mayor-Severa30%30%25%

All times in UTC

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