Viendo archivo del domingo, 29 agosto 2004
Informe geofísico
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.
:Product: 20040829SGAS.txt
:Issued: 2004 Aug 29 0250 UT
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.comResumen conjunto USAF/NOAA actividad Solar y Geofísica
SGAS Número 242 publicado el 0245Z a las 29 Aug 2004 Este infórmese ha elaborado a partir de los datos recibidos en SWO el 28 AugA. Eventos Energéticos
Inicio Max Fin Rgn Loc Xray Op 245MHz 10cm Barrido 1734 1734 1734 120
B. Eventos de Protones
Ninguno
C. Resumen de Actividad Geomagnética
The geomagnetic field was at
predominantly quiet to unsettled levels. There was an isolated
active period that occurred between 28/0600 and 0900Z in response to
southward Bz oscillations in the interplanetary magnetic field.
D. Estratosfera caliente
Ninguno
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 087 SSN 028 Afr/Ap 012/012 X-ray Background A7.1 Flujo Diario de Protones (flujo acumulado en 24 hr) GT 1 MeV 3.8e+05 GT 10 MeV 1.5e+04 p/(cm2-ster-day) (Satélite órbita sincronizada GOES-11 , W98 grados) Fluidez diaria de electrones GT 2 MeV 4.30e+07 e/(cm2-ster-day) (Satélite órbita sincronizada GOES-12 , W75 grados) 3 Horas K-índices Roca 2 3 4 3 2 3 2 2 Planetario 2 3 4 3 3 3 3 2
F. Comentarios
The ACE spacecraft orbit will bring ACE to its closest approach with the Sun on August 30, 2004. During that time possible solar radio noise may interfere with spacecraft telemetry resulting in the loss of real time solar wind plasma, magnetic field, and particle data.
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