Source:http://linkedlifedata.com/resource/pubmed/id/17734747
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| Predicate | Object |
|---|---|
| rdf:type | |
| lifeskim:mentions | |
| pubmed:issue |
4277
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| pubmed:dateCreated |
2010-6-7
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| pubmed:abstractText |
Temperature profiles of the martian atmosphere have been derived from airborne observations of the 8 April 1976 occultation of epsilon Geminorum. Within the altitude range from 50 to 90 kilometers, these profiles show peak-to-peak variations of 35 degrees K with a vertical scale of 20 kilometers and represent evidence for strong tides in the martian atmosphere. However, more information is necessary to conclusively rule out a radiative explanation for the temperature variations.
|
| pubmed:language |
eng
|
| pubmed:journal | |
| pubmed:status |
PubMed-not-MEDLINE
|
| pubmed:month |
Feb
|
| pubmed:issn |
0036-8075
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| pubmed:author | |
| pubmed:issnType |
Print
|
| pubmed:day |
4
|
| pubmed:volume |
195
|
| pubmed:owner |
NLM
|
| pubmed:authorsComplete |
Y
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| pubmed:pagination |
485-6
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| pubmed:year |
1977
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| pubmed:articleTitle |
Occultation of egr Geminorum by Mars: Evidence for Atmospheric Tides?
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| pubmed:publicationType |
Journal Article
|