This code does a power sweep to calculate at which point the multipactor starts to develop inside a single rectangular waveguide. EM fields can be resolved analytically for the TE10 mode of a rectangular waveguide, or through the FDTD method with a TE10 excited at one end of the guide, or other fields could be imported (e.g. from COMSOL).
The particle wall interaction is modeled using G. Chen, L. Liu (2011) ejection-collection algorithm but the actual method for deciding between absorption, elastic or inelastic collision or secondaries has been slightly modified to match FEST3D results. The option to use the Furman & Pivi model is also made available.
The Ecuyer Taus random number generator from Alan Miller's library is used. It has a period of 2^88 and the poisson deviates are generated using this generator and the waiting time method for means < 15.
Studies of how sensitive the threshold is to different parameters can be performed through the control of the variable atype. At the moment only 11 different studies can be performed but it is not hard to program more into MULH.
NOTE: There are some outstanding issues that ought to be resolved:
- MULH predicts a breakdown for wide waveguides (WR-229 and WR-284), while FEST3D doesn't. The breakdown calculated by both programs for other geometries seem to agree though. Perhaps the fields and particle steppers in these wide guides should be checked.
- MULH didn't see a resonance when applaying a DC toroidal B-field equal to the one predicted by a gyrofrequency of 3.7GHz (Tore-Supra), while Spark3D did.
- The trends in breakdown when DC B-fields are applied were never rigorously checked against FEST3D or Spark3D. (This work has been done by A. Placais)
The MULH parent directory contains five subfolders.
- sources: contains all the source files used in the code. subdirectory active contains the latest in-use source files.
- data: .txt files containing data used in some runs and the subdirectory results, where output data is stored. It also contains two m-files used for processing COMSOL fields from Melanie Preyna's PICCOLO and for processing MULH output data.
- execs: where the executables are placed during compilation
- test: for storing executables and other files used while testing pieces of or all of the code.
AP :
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MULHBatch: where MULH.py and MULH_parallel_batch.py are stored.
To run the code once run MULH.py with Python 3.6 or higher. To do a parameter sweep run MULH_parallel_batch.py with Python 3.6 or higher. These scripts execute the following command:
make export LD_LIBRARY_PATH="path to executable" ./MULH "path_to_config_file" "output_path"The config_file can be created using the create_config_file class in MULH.py.
The code was developed and worked well with the gfortran compiler. It hasn't been tried with other compilers.
For more details on the code see: Francisquez, M. 2012. Power limit modeling of lower hybrid antenna waveguides in tokamaks. BA Honors Thesis. Dartmouth College, November 2012.
Please feel free to contact me with questions and/or suggestions.
AUTHOR: Manaure Francisquez Department of Physics & Astronomy Dartmouth College Hanover, NH 03755 USA http://engineering.dartmouth.edu/~d24789f
Spring 2011 - Spring 2012
This code was later modified by: Adrien Placais GSCP IRFM, CEA Cadarache France adrien.placais@hotmail.fr
April - September 2017