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D. Rowland<br />
How bright<br />
Brightness<br />
are<br />
distribution cuts<br />
they?<br />
off sharply around RHESSI's<br />
Fs observed during a single pass over a single storm:<br />
Wednesday, April 22, 2009<br />
For dessert:<br />
RHESSI cannot discriminate background<br />
fluctuations from TGFs at low fluxes<br />
(from Smith et al., SCIPP seminar, 2005)<br />
RHESSI Instrument saturates at high count rates.<br />
Possibly underestimating TGF fluxes by 2-5.<br />
sensitivity limit for our triggering algorithm; is this the<br />
tip of the iceberg?<br />
?<br />
10 6<br />
10 5<br />
10 4<br />
10 3<br />
10 2<br />
10 3<br />
RHESSI<br />
1 µs deadtime<br />
no deadtime<br />
0.1 µs deadtime<br />
<strong>CubeSat</strong> Developers’ Workshop April 22, 2009<br />
10 4<br />
10 5<br />
10 6<br />
8
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