Viendo archivo del martes, 18 enero 2005
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: 20050118SGAS.txt
:Issued: 2005 Jan 18 0250 UT
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Resumen conjunto USAF/NOAA actividad Solar y Geofísica
SGAS Número 018 publicado el 0245Z a las 18 Jan 2005
Este infórmese ha elaborado a partir de los datos recibidos en SWO el 17 Jan
A. Eventos Energéticos
Inicio Max Fin Rgn Loc Xray Op 245MHz 10cm Barrido
0310 0321 0332 0720 M2.6
0659 0952 1007 0720 X3.8 2f 39000 12000 II/IV
B. Eventos de Protones
The proton event at greater than 10 MeV that
began on 16/0210 UTC remains in progress. The X3 flare which
occurred at 17/0952 UTC has increased the current peak flux to 5040
pfu observed at 17/1750 UTC. A proton event at greater than 100 MeV
also resulted from the X3 flare, beginning at 17/1215 UTC and with a
current peak flux of 28 pfu observed at 17/1700 UTC.
C. Resumen de Actividad Geomagnética
The geomagnetic field ranged from
unsettled to severe storm levels. Solar wind conditions observed by
the NASA ACE spacecraft show a fairly complex onset of activity
which may suggest the arrival of a solar wind structure from
combined CMEs expected from previous major flares on 15 January.
D. Estratosfera caliente
Ninguno
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 138 SSN 107 Afr/Ap 046/063 X-ray Background C1.5
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV 6.2e+08 GT 10 MeV 1.1e+08 p/(cm2-ster-day)
(Satélite órbita sincronizada GOES-11 , W107 grados)
Fluidez diaria de electrones
GT 2 MeV 1.40e+07 e/(cm2-ster-day)
(Satélite órbita sincronizada GOES-12 , W75 grados)
3 Horas K-índices
Roca 4 4 3 6 6 6 5 3 Planetario 5 4 3 7 7 7 5 3
F. Comentarios
The Afr index reported in Part E is estimated from
Boulder observations.
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