Difference between revisions of "November 15th, 2022"
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* On October 17th, we had a ''Hovanes'' CPS meeting for a development of the conseptual design of the Tiger hall with CPS [https://wiki.jlab.org/klproject/index.php/CPS_meeting_-_October_17,_2022]. Temperature map calculations (''Tim''). Updates on the conceptual design (''Vitaly''). | * On October 17th, we had a ''Hovanes'' CPS meeting for a development of the conseptual design of the Tiger hall with CPS [https://wiki.jlab.org/klproject/index.php/CPS_meeting_-_October_17,_2022]. Temperature map calculations (''Tim''). Updates on the conceptual design (''Vitaly''). | ||
| + | Adding raster to FLUKA simulations(''Hovanes''). | ||
| + | -Convolution of two distributions : Gaussian ⨁ Rastering | ||
| + | -Gaussian with 2.5mm in FWHM (which is the same as 1.1 mm in RMS) | ||
| + | -Uniform rastering of the center of the Gaussian within D = 2 mm | ||
| + | -Raster only the beam position but not the angle (parallel shift) | ||
| + | -Wider channel may be needed | ||
| + | -Evaluate the impact of FWHM dropping to 1mm instead of 2.5 mm but keeping the raster on | ||
* Thursday, November 10th, we had the 6th KLF Collaboration meeting. The agenda is at [https://wiki.jlab.org/klproject/index.php/November,_10th_2022]. | * Thursday, November 10th, we had the 6th KLF Collaboration meeting. The agenda is at [https://wiki.jlab.org/klproject/index.php/November,_10th_2022]. | ||
Revision as of 01:07, 18 October 2022
Attended: ..., and Igor.
- On October 3rd, we had a Hovanes CPS meeting for a development of the conseptual design of the Tiger hall with CPS [1]. Temperature map calculations (Tim). Updates on the conceptual design (Vitaly).
- On October 17th, we had a Hovanes CPS meeting for a development of the conseptual design of the Tiger hall with CPS [2]. Temperature map calculations (Tim). Updates on the conceptual design (Vitaly).
Adding raster to FLUKA simulations(Hovanes). -Convolution of two distributions : Gaussian ⨁ Rastering -Gaussian with 2.5mm in FWHM (which is the same as 1.1 mm in RMS) -Uniform rastering of the center of the Gaussian within D = 2 mm -Raster only the beam position but not the angle (parallel shift) -Wider channel may be needed -Evaluate the impact of FWHM dropping to 1mm instead of 2.5 mm but keeping the raster on
- Thursday, November 10th, we had the 6th KLF Collaboration meeting. The agenda is at [3].