This page (revision-14) was last changed on 27-Nov-2017 16:38 by Peter Young

This page was created on 08-Oct-2013 20:24 by Peter Young

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At line 13 changed one line
!!H. Warren method
!!Warren, Ugarte-Urra, and Landi method
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I have attempted to extend Giulio's method of using the atomic data to infer the shape of the effective areas by including information from the SDO/EVE instrument. EIS routinely makes full-disk mosaics (HOP130), which can be used to compute irradiances that be compared with those from EVE.
We have attempted to extend Giulio's method of using the atomic data to infer the shape of the effective areas by including information from the SDO/EVE instrument. EIS routinely makes full-disk mosaics (HOP130), which can be used to compute irradiances that be compared with those from EVE. Below is a comparison of the EIS and EVE irradiances for 195.
At line 19 added 4 lines
We then use very deep observations taken above the limb to fit a mode that includes both an emission measure distribution and potential modifications to the effective areas. The effective area near 195 is fixed to lie on the EIS-EVE curve shown above. Here is an example of this analysis.