Viendo archivo de miércoles, 18 junio 2003

Informe Geofísico

Resumen de Actividad Solar y Geofísica 2003 Jun 18 0245 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Resumen conjunto USAF/NOAA actividad Solar y Geofísica

SGAS Número 169 publicado el 0245Z a las 18 Jun 2003 Este infórmese ha elaborado a partir de los datos recibidos en SWO el 17 Jun
A. Eventos Energéticos
Inicio  Max  Fin  Rgn   Loc   Xray  Op 245MHz 10cm   Barrido
2144 2153 2158  0386 S07E55 C5.2  1f        140
2227 2255 2312  0386        M6.8     1200   2100   II/IV
B. Eventos de Protones
Ninguno
C. Resumen de Actividad Geomagnética
The geomagnetic field was at active to major storm levels. A six-hour period of southward Bz, from 06 - 09 UTC combined with elevated solar wind speed near 510 km/s produced minor and major storm levels. Greater than 2 MeV fluence levels were at background levels today.
D. Estratosfera caliente
Ninguno
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 122  SSN 080  Afr/Ap 040/050   X-ray Background B2.8
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV 7.9e+05   GT 10 MeV 1.8e+04 p/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-8 , W127 grados)
Fluidez diaria de electrones
GT 2 MeV 8.00e+06 e/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-12 , W76 grados)
3 Horas K-índices
Boulder 5 5 6 5 4 4 3 4 Planetary 5 6 6 6 4 4 4 4
F. Comentarios
  K-Indices:
On 16 June, it was determined that a scaling problem exists with the
H-trace on the Boulder magnetometer instrument.  While this problem,
and its fix are being investigated the primary instrument for
Boulder K-indices has been switched to the Boulder USGS (via Domsat)
magnetometer, effective 1500 UTC on 16 June.

GOES Protons:
To ensure continued operational monitoring of important energetic
particle data, it is necessary to reassign primary/secondary
designations for the GOES Space Environment Monitor (SEM) detectors.
Beginning 1700 UTC on June 18, GOES 11 (105W) will become the
primary satellite for protons. GOES 12 will continue as the primary
satellite for magnetometer, X-ray, and electron measurements. GOES
10 (135W) will be the secondary satellite for all SEM sensors -
magnetometer, X-ray, and energetic particles.  Because of the
degraded state of the proton data on GOES-10, its designation as the
secondary source for proton data is a short-term solution.  More
permanent solutions have been identified and are being evaluated.
Users will be notified when we define and schedule a permanent fix.
Further details can be found at http://www.sec.noaa.gov/GOES.html.

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