Peržiūrimas ketvirtadienis, gegužės 15. 2003

Geofizinis pranešimas

Bendra USAF/NOAA Saulės ir geofizinio aktyvumo santrauka

A. Energijos įvykiai

Pradėti Max End Rgn Loc Xray Op 245MHz 10cm Sweep
Nė vieno

B. Protonų įvykiai

C. Geomagnetinio aktyvumo suvestinė

D. Stratwarm

E. Dienos indeksai: (realaus laiko preliminarios / įvertintos vertės)

10 cm 096  SSN 075  Afr/Ap 025/027   X-ray Background B1.0
Dienos protonų srautas (srautas sukauptas per 24 valandas)
GT 1 MeV 6.8e+06   GT 10 MeV 1.1e+04 p/(cm2-ster-day)
(GOES-10 palydovo sinchroninė orbita W135 laipsniai)
Kasdienis elektronų srautas
GT 2 MeV 7.80e+08 e/(cm2-ster-day)
(GOES-10 palydovo sinchroninė orbita W135 laipsniai)
3 valandų K indeksai
Boulder 5 5 5 4 3 3 4 3 Planetary 5 5 5 4 3 4 4 3

F. Komentarai

  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. Beginning 1500 UT on May 15, GOES-8 will
once again become 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.

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