Guarda l'archivio di giovedì, 19 giugno 2003

Rapporto geofisico

Riassunto delle attività solari e geofisiche 2003 Jun 19 0245 UTC
Preparato dal NOAA © SWPC ed elaborato da SpaceWeatherLive.com

Sintesi delle attività solari e geofisiche congiunte USAF/NOAA

Numero SGAS 170 Rilascialo alle 0245Z il 19 Jun 2003 Questo rapporto è compilato dai dati ricevuti allo SWO il 18 Jun
A. Eventi Energetici
Inizio  Max  Fine  Rgn   Loc   Xray  Op 245MHz 10cm   Sweep
2227 2255 2312  0386        M6.8     1200   2100   II/IV
B. Eventi Protone
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. Sommario Attività Geomagnetica
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. Stratwarm
Nessuna
E. Indici Giornalieri: (valori preliminari/stimati in tempo reale)
10 cm 120  SSN 099  Afr/Ap 045/054   X-ray Background B3.2
Fluenza di Protoni Giornaliera (accumulo di flusso nelle 24 ore)
GT 1 MeV 2.5e+07   GT 10 MeV 1.4e+06 p/(cm2-ster-day)
(GOES-8 satellite ad orbita sincrona W128 gradi)
Flusso Giornaliero di Elettroni
GT 2 MeV 2.30e+06 e/(cm2-ster-day)
(GOES-12 satellite ad orbita sincrona W75 gradi)
Indice K a 3 ore
Boulder 5 5 6 6 3 5 4 3 Planetary 5 6 7 6 4 4 4 4
F. Commenti
  Nessuna
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.
99999

<< Vai alla pagina della panoramica giornaliera

Ultime notizie

Supporta SpaceWeatherLive.com!

Molte persone vengono su SpaceWeatherLive per seguire l'attività del Sole o se c'è un'aurora da vedere, ma con un maggior traffico arrivano maggiori costi del server. Considera una donazione se ti piace SpaceWeatherLive in modo da poter mantenere il sito online!

100%

Ultimi avvisi

Ricevi avvisi istantanei!

Notizie sul meteo spaziale

Ultimo X-flare:2017/09/10X8.2
Ultimo M-flare:2017/10/20M1.0
Ultima tempesta geomagnetica:2019/09/28Kp5 (G1)
Numero di giorni senza macchie nel 2019:218
Attuali giornate senza macchie:20

Questo giorno nella storia*

Flares solari
12014X1.6
22001X1.2
32003M9.9
42014M8.7
52001M6.7
ApG
1200196G3
2199991G4
3199638G3
4200334G1
5199425G2
*dal 1994

Social networks