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High Temperature Material Processes: An International Quarterly of High-Technology Plasma Processes

Publicado 4 números por año

ISSN Imprimir: 1093-3611

ISSN En Línea: 1940-4360

The Impact Factor measures the average number of citations received in a particular year by papers published in the journal during the two preceding years. 2017 Journal Citation Reports (Clarivate Analytics, 2018) IF: 0.4 The Immediacy Index is the average number of times an article is cited in the year it is published. The journal Immediacy Index indicates how quickly articles in a journal are cited. Immediacy Index: 0.1 The Eigenfactor score, developed by Jevin West and Carl Bergstrom at the University of Washington, is a rating of the total importance of a scientific journal. Journals are rated according to the number of incoming citations, with citations from highly ranked journals weighted to make a larger contribution to the eigenfactor than those from poorly ranked journals. Eigenfactor: 0.00005 The Journal Citation Indicator (JCI) is a single measurement of the field-normalized citation impact of journals in the Web of Science Core Collection across disciplines. The key words here are that the metric is normalized and cross-disciplinary. JCI: 0.07 SJR: 0.198 SNIP: 0.48 CiteScore™:: 1.1 H-Index: 20

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MODELING OF THE RADIATIVE EMISSION OF A PLASMA SURROUNDING A SPACE PROBE ENTERING MARS ATMOSPHERE

Volumen 7, Edición 1, 2003, 11 pages
DOI: 10.1615/HighTempMatProc.v7.i1.160
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SINOPSIS

Spectral emission of the plasma formed in front of a space vehicle entering the upper layer of Mars atmosphere is analysed. The high temperatures behind a hypersonic shock wave leads to dissociation and ionisation of the molecules found in the Martian atmosphere. The chemical reactions responsible for the formation of a Martian plasma are presented. A simulation of the spectra of some of the most important emitting systems is performed (numerical code SESAM), and a comparison with experimental spectra obtained in a low pressure arc-jet wind tunnel is presented. The influence on the shape of the simulated CN violet spectra, of the apparatus function, vibration and rotation temperatures is studied.

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