Changeset 813
- Timestamp:
- 05/29/01 17:14:26 (23 years ago)
- File:
-
- 1 edited
Legend:
- Unmodified
- Added
- Removed
-
trunk/ICRC_01/mccontrib.tex
r811 r813 330 330 photons in the camera plane are needed to trigger the Telescope. 331 331 And it helps the low energy showers to fulfil the required trigger 332 conditions. In figure 3 one can see that the threshold energy decreases333 while lowering the discriminator. It is 25 GeV for 3 mV and 105 GeV334 for 7 mV. Since one of the aims of the Telescope is lowering as much335 as possible the energy threshold, a low discriminator value is332 conditions. In figure \ref{fig_enerthres} one can see that the threshold 333 energy decreases while lowering the discriminator. It is 25 GeV for 3 mV 334 and 105 GeV for 7 mV. Since one of the aims of the Telescope is lowering as 335 much as possible the energy threshold, a low discriminator value is 336 336 preferred. But for 3 mV the expected rate due to protons increases a 337 337 lot (see section 3.1.3), while it keeps under control at 4 mV.
Note:
See TracChangeset
for help on using the changeset viewer.