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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14 27-Nov-2017 16:38 4 KB Peter Young to previous
13 07-Dec-2016 14:14 3 KB ogenopanurequ to previous | to last
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11 03-Nov-2016 18:26 4 KB ajeekinok to previous | to last
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9 29-Oct-2013 21:52 3 KB Peter Young to previous | to last
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6 21-Oct-2013 12:50 2 KB Harry Warren to previous | to last
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2 09-Oct-2013 14:47 1 KB Peter Young to previous | to last
1 08-Oct-2013 20:24 1 KB Peter Young to last

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At line 15 added 2 lines
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.