Questions for the General meeting
Can Gigi or Giulio confirm these points?
- The run stopped at the end of 2022 due to network problems; no more data have been taken.
- Andrea recalls that the quality of BLU data was worse than that of ROSSO and NERO.
Minutes of the meeting
General matters
- Add Giulio to muraves-analysis mailing list.
Data
- No BLU data available on T2B.
Simulation
- Mulder uses by default an altitude of 598m
- Shadow around elevation angle 25
- Both free sky and vesuvio MULDER simulations have a different muon flux with respect to calculations.
Yanwen
Feedbacks:
- Add ratio of the calculations and simulation GUAN curve. This way it is easier to grasp the percentage difference.
- Use log scale on the flux.
Next steps:
- Debug the Free Sky MULDER simulation (central topic of upcoming meetings).
- Yanwen suspects that the way scattering is implemented in MULDER could be part of the problem.
- Gabor suggests experimenting and tweaking other simulation parameters as well.
- Collaboration with Gabor:
Yanwen will provide the elevation and rock-thickness maps, and Gabor will run the prediction calculations. He will provide results using two or three average rock densities. The objective is to integrate this information into TURTLE.
Alice
Next step:
- Compare outputs with existing files
- Got full analysis folder from Muripper -> Run main reconstruction script
Gábor
- Moving data from Muripper to T2B:
/pnfs/iihe/muraves/muraves_DATA/RAW_GZ/<BLU/NERO/ROSSO>
