This page (revision-7) was last changed on 07-Dec-2016 14:14 by PeterYoung

This page was created on 19-Mar-2010 16:02 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
7 07-Dec-2016 14:14 5 KB PeterYoung to previous
6 19-Mar-2010 17:38 5 KB PeterYoung to previous | to last
5 19-Mar-2010 17:25 5 KB PeterYoung to previous | to last
4 19-Mar-2010 17:11 4 KB PeterYoung to previous | to last
3 19-Mar-2010 16:18 3 KB PeterYoung to previous | to last
2 19-Mar-2010 16:07 3 KB PeterYoung to previous | to last
1 19-Mar-2010 16:02 2 KB PeterYoung to last

Page References

Incoming links Outgoing links

Version management

Difference between version and

At line 44 changed one line
The anomalously bright exposures 57 and 88 for the Mg VII 280.75 and Fe XV 284.16 windows are probably due to the fact that exposure times of 0 have been assigned to these exposures. When the intensity is computed, a division by the exposure time is performed. It seems likely that an arbitrarily small exposure time has been used giving a much higher intensity value than normal.
The anomalously bright exposures 57 and 88 for the Mg VII 280.75 and Fe XV 284.16 windows are probably due to the fact that exposure times of 0 have been assigned to these exposures. When the intensity is computed, a division by the exposure time is performed. It seems likely that an arbitrarily small exposure time has been used giving a much higher intensity value than normal. The image below shows an image from the Mg VII 280.75 window, with the two bright exposures clearly seen.
At line 46 added 5 lines
[{Image src = 'mg7_image.png' width='400'}]
Only two windows show 'weird' spectra. Examples from exposure 26 are shown below:
[{Image src = 'weird_exp26.png' width='400'}]