DIB table 2015 Aug 5
From RHESSI Wiki
(Difference between revisions)
(Created page with "Last updated 2013 Feb. 13 address DIB table: 1 2 3 4 5 6 7 8 9 0 General control 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 1 global enables 0x01 0x01 0x01 0x01...") |
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| - | Last updated 2013 Feb. | + | Last updated 2013 Feb. 14 |
address DIB table: 1 2 3 4 5 6 7 8 9 | address DIB table: 1 2 3 4 5 6 7 8 9 | ||
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10 rear fast threshold 0x45 0x45 0x60 0x55 0x45 0x45 0x45 0x45 0x60 | 10 rear fast threshold 0x45 0x45 0x60 0x55 0x45 0x45 0x45 0x45 0x60 | ||
11 12-bit pulser amplitude 0x00 0xFF 0x00 0x00 0x00 0x00 0x00 0x00 0x00 | 11 12-bit pulser amplitude 0x00 0xFF 0x00 0x00 0x00 0x00 0x00 0x00 0x00 | ||
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| + | A note on converting threshold values to keV: | ||
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| + | Very roughly, the standard threshold, 0x0C, represents a little under 3 keV. So 0x58 is roughly 88/12 * 3 = 22 keV. Probably a little lower. But in the end we want to calibrate this using flare data. | ||
Revision as of 23:09, 14 February 2013
Last updated 2013 Feb. 14
address DIB table: 1 2 3 4 5 6 7 8 9 0 General control 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 0x0A 1 global enables 0x01 0x01 0x01 0x01 0x01 0x01 0x01 0x01 0x01 2 front enables 0x29 0x29 0x29 0x29 0x29 0x29 0x29 0x29 0x29 3 front decimation 0x00 0x00 0x00 0x00 0x00 0x00 0x00 0x00 0x00 4 rear enables 0x2D 0x2D 0x2D 0x2D 0x2D 0x2D 0x2D 0x2D 0x2D 5 rear decimation 0x85 0x85 0x85 0x85 0x85 0x85 0x85 0x85 0x85 6 pulser frequency code 0x0B 0x0B 0x0B 0x0B 0x0B 0x0B 0x0B 0x0B 0x0B 7 front slow threshold 0x0C 0x58 0x0C 0x0C 0x0C 0x0C 0x0C 0x0C 0x0C 8 front fast threshold 0x22 0x80 0x22 0x50 0x22 0x22 0x22 0x22 0x22 9 rear slow threshold 0x30 0x30 0x30 0x30 0x30 0x30 0x30 0x30 0x30 10 rear fast threshold 0x45 0x45 0x60 0x55 0x45 0x45 0x45 0x45 0x60 11 12-bit pulser amplitude 0x00 0xFF 0x00 0x00 0x00 0x00 0x00 0x00 0x00
A note on converting threshold values to keV:
Very roughly, the standard threshold, 0x0C, represents a little under 3 keV. So 0x58 is roughly 88/12 * 3 = 22 keV. Probably a little lower. But in the end we want to calibrate this using flare data.
