Radiation Gas Dynamics:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Vienna
Springer Vienna
1966
|
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | When the temperature of a gas is not too high and the density of a gas is not too low, the transfer of heat by radiation is usually negligibly small in comparison with that by conduction and convection. However, in the hypersonic flow of space flight, particularly in the re-entry of a space vehicle, and in the flow problem involving nuclear reaction such as in the blast wave of nuclear bomb or in the peaceful use of the controlled fusion reaction, the temperature of the gas may be very high and the density of the gas may be very low. As a result, thermal radiation becomes a very important mode of heat transfer. A complete analysis of such high temperature flow fields should be based upon a study of the gasdynamic field and the radiation field simultaneously. Hence during the last few years, considerable efforts have been made to study such interaction problems between gasdynamic field and radiation field and a new title, Radiation Gasdynamics, has been suggested for this subject. Even though radiative transfer has been studied for a long time by astro physicists, the interaction between the radiation field and the gadsynamic field has been only extensively studied recently |
| Beschreibung: | 1 Online-Ressource (VIII, 230 p) |
| ISBN: | 9783709157305 9783709157336 |
| DOI: | 10.1007/978-3-7091-5730-5 |
Internformat
MARC
| LEADER | 00000nmm a2200000zc 4500 | ||
|---|---|---|---|
| 001 | BV042414774 | ||
| 003 | DE-604 | ||
| 005 | 00000000000000.0 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150316s1966 |||| o||u| ||||||eng d | ||
| 020 | |a 9783709157305 |c Online |9 978-3-7091-5730-5 | ||
| 020 | |a 9783709157336 |c Print |9 978-3-7091-5733-6 | ||
| 024 | 7 | |a 10.1007/978-3-7091-5730-5 |2 doi | |
| 035 | |a (OCoLC)863976959 | ||
| 035 | |a (DE-599)BVBBV042414774 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-91 |a DE-83 | ||
| 082 | 0 | |a 530 |2 23 | |
| 084 | |a PHY 000 |2 stub | ||
| 100 | 1 | |a Pai, Shih-I. |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Radiation Gas Dynamics |c by Shih-I Pai |
| 264 | 1 | |a Vienna |b Springer Vienna |c 1966 | |
| 300 | |a 1 Online-Ressource (VIII, 230 p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 500 | |a When the temperature of a gas is not too high and the density of a gas is not too low, the transfer of heat by radiation is usually negligibly small in comparison with that by conduction and convection. However, in the hypersonic flow of space flight, particularly in the re-entry of a space vehicle, and in the flow problem involving nuclear reaction such as in the blast wave of nuclear bomb or in the peaceful use of the controlled fusion reaction, the temperature of the gas may be very high and the density of the gas may be very low. As a result, thermal radiation becomes a very important mode of heat transfer. A complete analysis of such high temperature flow fields should be based upon a study of the gasdynamic field and the radiation field simultaneously. Hence during the last few years, considerable efforts have been made to study such interaction problems between gasdynamic field and radiation field and a new title, Radiation Gasdynamics, has been suggested for this subject. Even though radiative transfer has been studied for a long time by astro physicists, the interaction between the radiation field and the gadsynamic field has been only extensively studied recently | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Physics, general | |
| 650 | 0 | 7 | |a Strahlungsgasdynamik |0 (DE-588)4183534-7 |2 gnd |9 rswk-swf |
| 689 | 0 | 0 | |a Strahlungsgasdynamik |0 (DE-588)4183534-7 |D s |
| 689 | 0 | |8 1\p |5 DE-604 | |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-3-7091-5730-5 |x Verlag |3 Volltext |
| 912 | |a ZDB-2-PHA |a ZDB-2-BAE | ||
| 940 | 1 | |q ZDB-2-PHA_Archive | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-027850267 | ||
| 883 | 1 | |8 1\p |a cgwrk |d 20201028 |q DE-101 |u https://d-nb.info/provenance/plan#cgwrk | |
Datensatz im Suchindex
| _version_ | 1804153080968642560 |
|---|---|
| any_adam_object | |
| author | Pai, Shih-I |
| author_facet | Pai, Shih-I |
| author_role | aut |
| author_sort | Pai, Shih-I |
| author_variant | s i p sip |
| building | Verbundindex |
| bvnumber | BV042414774 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)863976959 (DE-599)BVBBV042414774 |
| dewey-full | 530 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 530 - Physics |
| dewey-raw | 530 |
| dewey-search | 530 |
| dewey-sort | 3530 |
| dewey-tens | 530 - Physics |
| discipline | Physik |
| doi_str_mv | 10.1007/978-3-7091-5730-5 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02543nmm a2200421zc 4500</leader><controlfield tag="001">BV042414774</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1966 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9783709157305</subfield><subfield code="c">Online</subfield><subfield code="9">978-3-7091-5730-5</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9783709157336</subfield><subfield code="c">Print</subfield><subfield code="9">978-3-7091-5733-6</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-3-7091-5730-5</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)863976959</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042414774</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-91</subfield><subfield code="a">DE-83</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">530</subfield><subfield code="2">23</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 000</subfield><subfield code="2">stub</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Pai, Shih-I.</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Radiation Gas Dynamics</subfield><subfield code="c">by Shih-I Pai</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Vienna</subfield><subfield code="b">Springer Vienna</subfield><subfield code="c">1966</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (VIII, 230 p)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">When the temperature of a gas is not too high and the density of a gas is not too low, the transfer of heat by radiation is usually negligibly small in comparison with that by conduction and convection. However, in the hypersonic flow of space flight, particularly in the re-entry of a space vehicle, and in the flow problem involving nuclear reaction such as in the blast wave of nuclear bomb or in the peaceful use of the controlled fusion reaction, the temperature of the gas may be very high and the density of the gas may be very low. As a result, thermal radiation becomes a very important mode of heat transfer. A complete analysis of such high temperature flow fields should be based upon a study of the gasdynamic field and the radiation field simultaneously. Hence during the last few years, considerable efforts have been made to study such interaction problems between gasdynamic field and radiation field and a new title, Radiation Gasdynamics, has been suggested for this subject. Even though radiative transfer has been studied for a long time by astro physicists, the interaction between the radiation field and the gadsynamic field has been only extensively studied recently</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics, general</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Strahlungsgasdynamik</subfield><subfield code="0">(DE-588)4183534-7</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Strahlungsgasdynamik</subfield><subfield code="0">(DE-588)4183534-7</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2=" "><subfield code="8">1\p</subfield><subfield code="5">DE-604</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-3-7091-5730-5</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-PHA</subfield><subfield code="a">ZDB-2-BAE</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-PHA_Archive</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-027850267</subfield></datafield><datafield tag="883" ind1="1" ind2=" "><subfield code="8">1\p</subfield><subfield code="a">cgwrk</subfield><subfield code="d">20201028</subfield><subfield code="q">DE-101</subfield><subfield code="u">https://d-nb.info/provenance/plan#cgwrk</subfield></datafield></record></collection> |
| id | DE-604.BV042414774 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:56Z |
| institution | BVB |
| isbn | 9783709157305 9783709157336 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850267 |
| oclc_num | 863976959 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (VIII, 230 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1966 |
| publishDateSearch | 1966 |
| publishDateSort | 1966 |
| publisher | Springer Vienna |
| record_format | marc |
| spelling | Pai, Shih-I. Verfasser aut Radiation Gas Dynamics by Shih-I Pai Vienna Springer Vienna 1966 1 Online-Ressource (VIII, 230 p) txt rdacontent c rdamedia cr rdacarrier When the temperature of a gas is not too high and the density of a gas is not too low, the transfer of heat by radiation is usually negligibly small in comparison with that by conduction and convection. However, in the hypersonic flow of space flight, particularly in the re-entry of a space vehicle, and in the flow problem involving nuclear reaction such as in the blast wave of nuclear bomb or in the peaceful use of the controlled fusion reaction, the temperature of the gas may be very high and the density of the gas may be very low. As a result, thermal radiation becomes a very important mode of heat transfer. A complete analysis of such high temperature flow fields should be based upon a study of the gasdynamic field and the radiation field simultaneously. Hence during the last few years, considerable efforts have been made to study such interaction problems between gasdynamic field and radiation field and a new title, Radiation Gasdynamics, has been suggested for this subject. Even though radiative transfer has been studied for a long time by astro physicists, the interaction between the radiation field and the gadsynamic field has been only extensively studied recently Physics Physics, general Strahlungsgasdynamik (DE-588)4183534-7 gnd rswk-swf Strahlungsgasdynamik (DE-588)4183534-7 s 1\p DE-604 https://doi.org/10.1007/978-3-7091-5730-5 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Pai, Shih-I Radiation Gas Dynamics Physics Physics, general Strahlungsgasdynamik (DE-588)4183534-7 gnd |
| subject_GND | (DE-588)4183534-7 |
| title | Radiation Gas Dynamics |
| title_auth | Radiation Gas Dynamics |
| title_exact_search | Radiation Gas Dynamics |
| title_full | Radiation Gas Dynamics by Shih-I Pai |
| title_fullStr | Radiation Gas Dynamics by Shih-I Pai |
| title_full_unstemmed | Radiation Gas Dynamics by Shih-I Pai |
| title_short | Radiation Gas Dynamics |
| title_sort | radiation gas dynamics |
| topic | Physics Physics, general Strahlungsgasdynamik (DE-588)4183534-7 gnd |
| topic_facet | Physics Physics, general Strahlungsgasdynamik |
| url | https://doi.org/10.1007/978-3-7091-5730-5 |
| work_keys_str_mv | AT paishihi radiationgasdynamics |