Thermal Tides in the Dusty Martian Atmosphere: A Verification of Theory
Major features of the daily surface pressure oscillations observed by the Viking landers during the two great dust storms on Mars in 1977 can be explained in terms of the classical atmospheric tidal theory developed for the earth's atmosphere. The most dramatic exception is the virtual disappea...
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| Veröffentlicht in: | Science (American Association for the Advancement of Science) 1981-07, Vol.213 (4506), p.437-439 |
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| creator | Zurek, R. W. Leovy, C. B. |
| description | Major features of the daily surface pressure oscillations observed by the Viking landers during the two great dust storms on Mars in 1977 can be explained in terms of the classical atmospheric tidal theory developed for the earth's atmosphere. The most dramatic exception is the virtual disappearance of only the diurnal tide at Viking Lander 1 just before the second storm. This disappearance is attributed to destructive interference between the usually westward-traveling tide and an eastward-traveling diurnal Kelvin mode generated by orographically induced differential heating. The continuing Viking Lander 1 pressure measurements can be used with the model to monitor future great dust storms. |
| doi_str_mv | 10.1126/science.213.4506.437 |
| format | Article |
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W. ; Leovy, C. B.</creator><creatorcontrib>Zurek, R. W. ; Leovy, C. B.</creatorcontrib><description>Major features of the daily surface pressure oscillations observed by the Viking landers during the two great dust storms on Mars in 1977 can be explained in terms of the classical atmospheric tidal theory developed for the earth's atmosphere. The most dramatic exception is the virtual disappearance of only the diurnal tide at Viking Lander 1 just before the second storm. This disappearance is attributed to destructive interference between the usually westward-traveling tide and an eastward-traveling diurnal Kelvin mode generated by orographically induced differential heating. The continuing Viking Lander 1 pressure measurements can be used with the model to monitor future great dust storms.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.213.4506.437</identifier><identifier>PMID: 17760188</identifier><language>eng</language><publisher>United States: The American Association for the Advancement Science</publisher><subject>Atmosphere ; Atmospheric models ; Atmospheric tides ; Dust storms ; Impact craters ; Mars ; Mars (Planet) ; Ocean currents ; Opacity ; Planetary atmospheres ; Planetary meteorology ; Planets ; Pressure ; Tidal waves ; Trajectories</subject><ispartof>Science (American Association for the Advancement of Science), 1981-07, Vol.213 (4506), p.437-439</ispartof><rights>Copyright 1981 The American Association for the Advancement of Science</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c354t-7f9470e0a7d4185793f087f3c7e2aa24e7ce7c977ed97239b3393cef625bb9da3</citedby><cites>FETCH-LOGICAL-c354t-7f9470e0a7d4185793f087f3c7e2aa24e7ce7c977ed97239b3393cef625bb9da3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/1686518$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/1686518$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,777,781,800,2871,2872,27905,27906,57998,58231</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/17760188$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Zurek, R. 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The continuing Viking Lander 1 pressure measurements can be used with the model to monitor future great dust storms.</description><subject>Atmosphere</subject><subject>Atmospheric models</subject><subject>Atmospheric tides</subject><subject>Dust storms</subject><subject>Impact craters</subject><subject>Mars</subject><subject>Mars (Planet)</subject><subject>Ocean currents</subject><subject>Opacity</subject><subject>Planetary atmospheres</subject><subject>Planetary meteorology</subject><subject>Planets</subject><subject>Pressure</subject><subject>Tidal waves</subject><subject>Trajectories</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1981</creationdate><recordtype>article</recordtype><recordid>eNp9kcFqGzEQhkVIaRy3bxCCTsmhrCtpdldSb8Zp0kJKLk6uQtbOJgq7K1eSIX77KtiQW2FgDvPN8A8fIRecLTgX7ffkPE4OF4LDom5Yu6hBnpAZZ7qptGBwSmaMQVspJpszcp7SK2NlpuEzOeNStowrNSN36xeMox3o2neYqJ9ofkF6s0t5T__YmL2d6DKPIW0Lhz_okj5h9L13Nvsw0dDTciDE_RfyqbdDwq_HPiePtz_Xq1_V_cPd79XyvnLQ1LmSva4lQ2ZlV3PVSA09U7IHJ1FYK2qUrpSWEjstBegNgAaHfSuazUZ3Fubk-nB3G8PfHaZsRp8cDoOdMOySkQDlLybaQl79lxQglOS1KuC3A_hsBzR-cmHK-JZdGAZ8RlPirx7MkmvNeMk7J_WBdjGkFLE32-hHG_eGM_MuxhzFmCLGvIsxRUxZuzym2W1G7D6WjiYKcHEAXlMO8WPeqrbhCv4BSX2Szg</recordid><startdate>19810724</startdate><enddate>19810724</enddate><creator>Zurek, R. 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This disappearance is attributed to destructive interference between the usually westward-traveling tide and an eastward-traveling diurnal Kelvin mode generated by orographically induced differential heating. The continuing Viking Lander 1 pressure measurements can be used with the model to monitor future great dust storms.</abstract><cop>United States</cop><pub>The American Association for the Advancement Science</pub><pmid>17760188</pmid><doi>10.1126/science.213.4506.437</doi><tpages>3</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0036-8075 |
| ispartof | Science (American Association for the Advancement of Science), 1981-07, Vol.213 (4506), p.437-439 |
| issn | 0036-8075 1095-9203 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_733188026 |
| source | American Association for the Advancement of Science; Jstor Complete Legacy |
| subjects | Atmosphere Atmospheric models Atmospheric tides Dust storms Impact craters Mars Mars (Planet) Ocean currents Opacity Planetary atmospheres Planetary meteorology Planets Pressure Tidal waves Trajectories |
| title | Thermal Tides in the Dusty Martian Atmosphere: A Verification of Theory |
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