Geosynchronous Environment for Identification of Satellite Hit Anomalies
(GEISHA)
Doses and solar array degradation



This service allows to retrieve solar proton fluence at GEO altitude according to a user defined longitude and time period (a cumulative fluence will be provided - one fluence value every 5 minutes - integrated in time from start time). In this case, Solar proton environment is deduced fom GOES measurements. Five channels are available: 4.-9. MeV, 9.-15. MeV, 15.-40. MeV, 40.-80. MeV, 80.-165. MeV and 165.-500. MeV. More info ...

1. Select start and stop dates :

Start Date :  00:00:00 UT      End Date :  24:00:00 UT

* note : yyyy/mm/dd
* Important notice: A maximum of 15 days is allowed.

2. East longitude of geostationnary spacecraft (Degres)

3. Options to retrieve corresponding space environment
Retrieve solar proton fluence with a confidence level of


4. Date and time of anomaly (optional)
Highlight anomaly occurence with a vertical bar on the plot on: (yyyy/mm/dd hh:mm:ss)




For any comment or question please send Email to Bourdarie Sebastien.

Last update : March 20 2020 15:38:35.