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The Radiative Gas Dynamics of Spacecraft in the Martian Atmosphere
The problems of the radiative gas dynamics of the Martian space vehicles MSRO , Pathfinder , and Exomars-2016 are solved using the author’s custom NERAT-2D radiative-gasdynamic code. The cause of considerable heating of the rear surface of the spacecraft by heat radiation in the Martian atmosphere i...
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Published in: | Fluid dynamics 2022-12, Vol.57 (Suppl 2), p.S572-S593 |
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container_end_page | S593 |
container_issue | Suppl 2 |
container_start_page | S572 |
container_title | Fluid dynamics |
container_volume | 57 |
creator | Surzhikov, S. T. |
description | The problems of the radiative gas dynamics of the Martian space vehicles
MSRO
,
Pathfinder
, and
Exomars-2016
are solved using the author’s custom NERAT-2D radiative-gasdynamic code. The cause of considerable heating of the rear surface of the spacecraft by heat radiation in the Martian atmosphere is studied. Calculation studies of the spectral composition of heat radiation heating the front and rear surfaces of the SC were carried out, and the effect of catalytic properties of the surface on the results of aerothermodynamic modeling is explained. |
doi_str_mv | 10.1134/S0015462822100731 |
format | article |
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MSRO
,
Pathfinder
, and
Exomars-2016
are solved using the author’s custom NERAT-2D radiative-gasdynamic code. The cause of considerable heating of the rear surface of the spacecraft by heat radiation in the Martian atmosphere is studied. Calculation studies of the spectral composition of heat radiation heating the front and rear surfaces of the SC were carried out, and the effect of catalytic properties of the surface on the results of aerothermodynamic modeling is explained.</description><identifier>ISSN: 0015-4628</identifier><identifier>EISSN: 1573-8507</identifier><identifier>DOI: 10.1134/S0015462822100731</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Analysis ; Classical and Continuum Physics ; Classical Mechanics ; Engineering Fluid Dynamics ; Fluid- and Aerodynamics ; Gas dynamics ; Mars (Planet) ; Mars atmosphere ; Physics ; Physics and Astronomy ; Radiant heating ; Space ships ; Space vehicles ; Spacecraft ; Thermal radiation ; Thermodynamic models</subject><ispartof>Fluid dynamics, 2022-12, Vol.57 (Suppl 2), p.S572-S593</ispartof><rights>Pleiades Publishing, Ltd. 2022. ISSN 0015-4628, Fluid Dynamics, 2022, Vol. 57, Suppl. 2, pp. S572–S593. © Pleiades Publishing, Ltd., 2022.</rights><rights>COPYRIGHT 2022 Springer</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c285t-2c291b8052368a945021d49bac8bb62112ec4f048324d5b1ce590d8aa28b92633</citedby><cites>FETCH-LOGICAL-c285t-2c291b8052368a945021d49bac8bb62112ec4f048324d5b1ce590d8aa28b92633</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Surzhikov, S. T.</creatorcontrib><title>The Radiative Gas Dynamics of Spacecraft in the Martian Atmosphere</title><title>Fluid dynamics</title><addtitle>Fluid Dyn</addtitle><description>The problems of the radiative gas dynamics of the Martian space vehicles
MSRO
,
Pathfinder
, and
Exomars-2016
are solved using the author’s custom NERAT-2D radiative-gasdynamic code. The cause of considerable heating of the rear surface of the spacecraft by heat radiation in the Martian atmosphere is studied. Calculation studies of the spectral composition of heat radiation heating the front and rear surfaces of the SC were carried out, and the effect of catalytic properties of the surface on the results of aerothermodynamic modeling is explained.</description><subject>Analysis</subject><subject>Classical and Continuum Physics</subject><subject>Classical Mechanics</subject><subject>Engineering Fluid Dynamics</subject><subject>Fluid- and Aerodynamics</subject><subject>Gas dynamics</subject><subject>Mars (Planet)</subject><subject>Mars atmosphere</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Radiant heating</subject><subject>Space ships</subject><subject>Space vehicles</subject><subject>Spacecraft</subject><subject>Thermal radiation</subject><subject>Thermodynamic models</subject><issn>0015-4628</issn><issn>1573-8507</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp1kE1LAzEQhoMoWKs_wFvA89bJ1yZ7rFWroAi2npdsNtumtLs1SYX-e7Os4EFkDgPzvs98IXRNYEII47cLACJ4ThWlBEAycoJGREiWKQHyFI16Oev1c3QRwgYACpnTEbpbri1-17XT0X1ZPNcB3x9bvXMm4K7Bi7021njdROxaHJP3VfvodIuncdeF_dp6e4nOGr0N9uonj9HH48Ny9pS9vM2fZ9OXzFAlYkYNLUilQFCWK11wAZTUvKi0UVWVU0KoNbwBrhjltaiIsaKAWmlNVVXQnLExuhn67n33ebAhlpvu4Ns0sqRSAigmk22MJoNrpbe2dG3TRa9Nitqmo7rWNi7Vp5JxJQoieoAMgPFdCN425d67nfbHkkDZ_7b889vE0IEJyduurP9d5X_oGxtrd9s</recordid><startdate>20221201</startdate><enddate>20221201</enddate><creator>Surzhikov, S. T.</creator><general>Pleiades Publishing</general><general>Springer</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20221201</creationdate><title>The Radiative Gas Dynamics of Spacecraft in the Martian Atmosphere</title><author>Surzhikov, S. T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c285t-2c291b8052368a945021d49bac8bb62112ec4f048324d5b1ce590d8aa28b92633</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Analysis</topic><topic>Classical and Continuum Physics</topic><topic>Classical Mechanics</topic><topic>Engineering Fluid Dynamics</topic><topic>Fluid- and Aerodynamics</topic><topic>Gas dynamics</topic><topic>Mars (Planet)</topic><topic>Mars atmosphere</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Radiant heating</topic><topic>Space ships</topic><topic>Space vehicles</topic><topic>Spacecraft</topic><topic>Thermal radiation</topic><topic>Thermodynamic models</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Surzhikov, S. T.</creatorcontrib><collection>CrossRef</collection><jtitle>Fluid dynamics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Surzhikov, S. T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Radiative Gas Dynamics of Spacecraft in the Martian Atmosphere</atitle><jtitle>Fluid dynamics</jtitle><stitle>Fluid Dyn</stitle><date>2022-12-01</date><risdate>2022</risdate><volume>57</volume><issue>Suppl 2</issue><spage>S572</spage><epage>S593</epage><pages>S572-S593</pages><issn>0015-4628</issn><eissn>1573-8507</eissn><abstract>The problems of the radiative gas dynamics of the Martian space vehicles
MSRO
,
Pathfinder
, and
Exomars-2016
are solved using the author’s custom NERAT-2D radiative-gasdynamic code. The cause of considerable heating of the rear surface of the spacecraft by heat radiation in the Martian atmosphere is studied. Calculation studies of the spectral composition of heat radiation heating the front and rear surfaces of the SC were carried out, and the effect of catalytic properties of the surface on the results of aerothermodynamic modeling is explained.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0015462822100731</doi></addata></record> |
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language | eng |
recordid | cdi_proquest_journals_2770083726 |
source | Springer Nature |
subjects | Analysis Classical and Continuum Physics Classical Mechanics Engineering Fluid Dynamics Fluid- and Aerodynamics Gas dynamics Mars (Planet) Mars atmosphere Physics Physics and Astronomy Radiant heating Space ships Space vehicles Spacecraft Thermal radiation Thermodynamic models |
title | The Radiative Gas Dynamics of Spacecraft in the Martian Atmosphere |
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