Scanning drift tube measurements and kinetic computations of electron swarm parameters in CO
POSTER
Abstract
We present scanning drift tube measurements and modelling results of electron swarm transport coefficients in CO as a function of the reduced electric field E/N at room temperature. The measurements are performed under time-of-flight (TOF) conditions: a cloud of electrons is initiated by short UV laser pulses and its evolution is traced by detecting the electrons beyond a drift region whose length is varied. This way, so-called swarm maps are recorded, which are used to extract the transport coefficients of the electrons by fitting the current signals. Using the most recent set of cross-sections for electron scattering in CO from Magboltz (v11.11), modelling results are obtained by Monte Carlo (MC) simulations and by solving the Boltzmann equation using a multi-term approach and the density gradient expansion procedure. The measured and computed values of electron swarm transport coefficients agree very well, except for E/N<5 Td. For such low values of E/N the more advanced model for the strongly forward-peaked nature of rotational excitation is required. Measurements and calculations under TOF conditions are augmented by MC simulations of electron transport for idealized steady-state Townsend (SST) conditions. We found a ‘window’ of E/N where the SST transport properties of the electrons exhibit oscillatory behaviour as they relax towards the equilibrium state far downstream from the electron emitting boundary.
*This work was partially supported by the Portuguese FCT-Fundacao para a Ciencia e Tecnologia, under projects UIDB/50010/2020 and UIDP/50010/2020, by the Hungarian Office for Research, Development and Innovation (NKFIH) grants K134462, and funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) {project number 327886311 and via SFB 1316, project A4. SD and DB are supported by the Ministry of Education, Science and Technological Development of the Republic of Serbia and Institute of Physics Belgrade, and the Science Fund of the Republic of Serbia [Grant No. 7749560, EGWIn].
Presenters
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Sasa Dujko
- Institute of Physics Belgrade, University of Belgrade