This page (revision-3) was last changed on 07-Dec-2016 14:14 by PeterYoung

This page was created on 14-Jun-2007 11:50 by PeterYoung

Only authorized users are allowed to rename pages.

Only authorized users are allowed to delete pages.

Page revision history

Version Date Modified Size Author Changes ... Change note
3 07-Dec-2016 14:14 1 KB PeterYoung to previous
2 14-Jun-2007 11:55 1 KB PeterYoung to previous | to last
1 14-Jun-2007 11:50 986 bytes PeterYoung to last

Page References

Incoming links Outgoing links
CosmicRays
CosmicRays

Version management

Difference between version and

At line 1 removed 3 lines
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
There are two IDL routines that were used for de-spiking SOHO/CDS data, and they are found to give good results for EIS data. The routines are:
At line 2 added 2 lines
There are two IDL routines that were used for cleaning SOHO/CDS data from cosmic rays, and they are found to give good results for EIS data. The routines are:
At line 17 changed 9 lines
If you eis_prep on your data, then it automatically removes CRs with eis_despike unless the /nocr keyword is given.
If you are worried about whether real data are being flagged as CRs, then use the routine [eis_spike_viewer|EISSpikeViewer].
If you find an example where real data has been removed then please contact Peter Young.
! SAA periods
There are usually too many cosmic rays during SAA periods for the de-spiking routines to work effectively and so you should generally ignore SAA periods in your data. A possible exception is if you use very short exposure times, but this has not been checked.
If you worried about whether real data are being flagged as CRs, then use the routine [eis_spike_viewer|EISSpikeViewer].
This page (revision-3) was last changed on 07-Dec-2016 14:14 by PeterYoungTop