Find out aluminium thickness from MSL RAD model, see paper J. Appel 2017 ==== Mars Paper 2 ==== ==== Simulation preparation ==== * Lennart has prepared a PSF file on 12th of October \\ * Sasha has confirmed that the PSF file is OK \\ * Sasha has converted the PSF file to GDML \\ * Sasha has checked that the GDML file is OK \\ * Sasha has prepared extended GCR phantoms for ICRU and msl/rad detector B \\ * Sasha has created a 2mars directory in his phd git repository \\ * Based on the discussion with Jingnan, we are going to use the following energy range: \\ * Sasha has prepared a simulation script which takes: Z, number_of_threads, portion_factor and performs the needed run. \\ * We need for a single run the binary output! Also we need to benchmark if this is quicker or not. \\ * Based on the previous paper, we are going to use INCLXX for our calculations. \\ * INCLXX seams to have a bug when dealing with highest Z ions. == Simulation status == ^ Z ^ element name ^ status ^ machine ^ ETA ^ | 1 ^ H ^ | malanosa | 14.12. | | 2 ^ He ^ | malanosa | 16.12. | | 3 ^ Li ^ | optimus | 16.12. | | 4 ^ Be ^ | tr1 | 17.12. | | 5 ^ B ^ | tr1 | 18.12. | | 6 ^ C ^ | tr1 | 18.12. | | 7 ^ N ^ | tr1 | 19.12. | | 8 ^ O ^ | optimus | 20.12. | | 9 ^ F ^ | malanosa | 20.12. | | 10 ^ Ne ^ | malanosa | 20.12. | | 11 ^ Natrium ^ | terminator | 21.12. | | 12 ^ Magnesium ^ | optimus | 23.12. | | 13 ^ Al ^ | tr1 | 24.12. | | 14 ^ Si ^ | tr1 | 25.12. | | 15 ^ P ^ | tr1 | 26.12. | | 16 ^ S ^ | tr1 | 26.12. | | 17 ^ Cl ^ | tr2 | 27.12. | | 18 ^ Ar ^ | tr2 | 31.12. | | 19 ^ K (potasium) ^ | tr2 | 30.12. | | 20 ^ calcium ^ | malanosa | 27.12. | | 21 ^ scandium ^ | malanosa | 29.12. | | 22 ^ titanium ^ | malanosa | 31.12. | | 23 ^ vanadium ^ | optimus | 4.1. | | 24 ^ chromium ^ | optimus | 4.1. | | 25 ^ manganese ^ | optimus | 5.1. | | 26 ^ Ferum (Iron) ^ | terminator | 1.1. | | 27 ^ cobalt ^ | terminator | 2.1. | | 28 ^ nickel ^ | terminator | 5.1. | ==== Mars SEP calculator paper ==== * 20 Mars atmospheres with approx 15Pa steps in pressure * Only primary protons * energy range between 0.1 MeV and 10 GeV, i.e. -1 to 4 decades * 20 bins per decade ( total 100 bins) * 5000 parts per decade (500.000 particles per run) * 5 runs per atmosphere * in total 100 runs * Calculate results for all the GLEs Goal: make a function that takes (pressure, diffspectrum) and calculates dose altitude profile for radb and for an icrusphere. In paper: Talk about the atmospheres, talk about the convolution method, talk about the outlook: determining SEP spectra around mars