Viendo archivo del viernes, 16 mayo 2003

Informe geofísico

Resumen conjunto USAF/NOAA actividad Solar y Geofísica

A. Eventos Energéticos

Inicio  Max  Fin  Rgn   Loc   Xray  Op 245MHz 10cm   Barrido
Ninguno

B. Eventos de Protones

C. Resumen de Actividad Geomagnética

D. Estratosfera caliente

E. Indices Diarios: (preliminares en tiempo real/valores estimados)

10 cm 099  SSN 097  Afr/Ap 015/023   X-ray Background B1.3
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV 1.2e+06   GT 10 MeV 1.1e+04 p/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-12 , W75 grados)
Fluidez diaria de electrones
GT 2 MeV 3.60e+08 e/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-8 , W92 grados)
3 Horas K-índices
Boulder 4 3 4 3 5 4 2 3 Planetary 4 4 4 4 4 4 3 3

F. Comentarios

  The GOES 10 energetic proton detectors are showing
intermittent, high noise levels in the higher energy proton channels
(greater than about 80 MeV). This problem was first noticed in data
taken April 26, 2003. 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. As of 1500 UT on May 15, GOES-8 became the
primary satellite for protons. GOES 12 will be the primary satellite
for magnetometer, X-ray, and electron measurements. GOES 10 will be
the secondary satellite for all SEM sensors - magnetometer, X-ray
sensor, and energetic particle sensor. This short-term solution
(approximately 2 - 3 months) will be in place until we define and
implement a permanent fix. A more detailed explanation can be found
at: http://www.sec.noaa.gov/GOES.html.

All times in UTC

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