Viendo archivo de jueves, 19 junio 2003

Informe Geofísico

Resumen de Actividad Solar y Geofísica 2003 Jun 19 0245 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Resumen conjunto USAF/NOAA actividad Solar y Geofísica

SGAS Número 170 publicado el 0245Z a las 19 Jun 2003 Este infórmese ha elaborado a partir de los datos recibidos en SWO el 18 Jun
A. Eventos Energéticos
Inicio  Max  Fin  Rgn   Loc   Xray  Op 245MHz 10cm   Barrido
2227 2255 2312  0386        M6.8     1200   2100   II/IV
B. Eventos de Protones
The greater than 10 Mev proton fluxes at geosynchronous orbit reached event threshold at 18/2050Z and due to the recent activity the exact source for this particle event is not certain at this time but is most likely from the M6.8 x-ray flare from 17 June..
C. Resumen de Actividad Geomagnética
The geomagnetic field was at predominantly minor to major storm levels with an isolated period of severe storm conditions seen at high latitudes between 18/0600 and 0900Z. A co-rotating integrated region preceding a recurrent high speed coronal hole stream and is believed to responsible for the storm conditions.
D. Estratosfera caliente
Ninguno
E. Indices Diarios: (preliminares en tiempo real/valores estimados)
10 cm 120  SSN 099  Afr/Ap 045/054   X-ray Background B3.2
Flujo Diario de Protones (flujo acumulado en 24 hr)
GT 1 MeV 2.5e+07   GT 10 MeV 1.4e+06 p/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-8 , W128 grados)
Fluidez diaria de electrones
GT 2 MeV 2.30e+06 e/(cm2-ster-day)
(Satélite órbita sincronizada  GOES-12 , W75 grados)
3 Horas K-índices
Boulder 5 5 6 6 3 5 4 3 Planetary 5 6 7 6 4 4 4 4
F. Comentarios
  Ninguno
PLAIN
K-Indices:
On 16 June, it was determined that a scaling problem exists with 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. GOES 11 (113W) will become the primary satellite for protons. The transition from GOES 8 to GOES 11 was scheduled for 18 June, but has been delayed until 19 June. 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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