Plasma density, temperature and turbulence in the wake of the shuttle orbiter
Plasma density, temperature, and turbulence in the near, mid, and far wake of the Shuttle orbiter are examined on the basis of in situ observations by The University of Iowa Plasma Diagnostics Package (PDP). These observations, the only such measurements in the mid and far wake of the orbiter, indic...
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| Veröffentlicht in: | Planetary and space science 1989-08, Vol.37 (8), p.1001-1010 |
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| container_title | Planetary and space science |
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| creator | Tribble, A.C. Pickett, J.S. D'Angelo, N. Murphy, G.B. |
| description | Plasma density, temperature, and turbulence in the near, mid, and far wake of the
Shuttle orbiter are examined on the basis of
in situ observations by The University of Iowa
Plasma Diagnostics Package (PDP). These observations, the only such measurements in the mid and far wake of the
orbiter, indicate that plasma disturbances produced by the passage of the
orbiter extend downstream for a distance of several hundred meters behind the
orbiter. The electron density profile is found to exhibit nonmonotonic behavior. Most of the 6–40 Hz turbulence in the wake is confined to a region ≈20 m downstream of the
orbiter.
ΔN
e
/
N
e
spectra show a rapid decline in the 10
4–10
5 Hz decade, both in the ambient ionosphere and in the wake. |
| doi_str_mv | 10.1016/0032-0633(89)90054-8 |
| format | Article |
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Shuttle orbiter are examined on the basis of
in situ observations by The University of Iowa
Plasma Diagnostics Package (PDP). These observations, the only such measurements in the mid and far wake of the
orbiter, indicate that plasma disturbances produced by the passage of the
orbiter extend downstream for a distance of several hundred meters behind the
orbiter. The electron density profile is found to exhibit nonmonotonic behavior. Most of the 6–40 Hz turbulence in the wake is confined to a region ≈20 m downstream of the
orbiter.
ΔN
e
/
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e
spectra show a rapid decline in the 10
4–10
5 Hz decade, both in the ambient ionosphere and in the wake.</description><identifier>ISSN: 0032-0633</identifier><identifier>EISSN: 1873-5088</identifier><identifier>DOI: 10.1016/0032-0633(89)90054-8</identifier><identifier>CODEN: PLSSAE</identifier><language>eng</language><publisher>Legacy CDMS: Elsevier Ltd</publisher><subject>Earth, ocean, space ; Exact sciences and technology ; External geophysics ; Physics of the ionosphere ; Plasma Physics ; Plasmasphere</subject><ispartof>Planetary and space science, 1989-08, Vol.37 (8), p.1001-1010</ispartof><rights>1989</rights><rights>1990 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c418t-969122855a04c1810dd45b83a449d98b8b2c49bd76762f1ddc2555046e32cf513</citedby><cites>FETCH-LOGICAL-c418t-969122855a04c1810dd45b83a449d98b8b2c49bd76762f1ddc2555046e32cf513</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/0032-0633(89)90054-8$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3550,27924,27925,45995</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=6653328$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Tribble, A.C.</creatorcontrib><creatorcontrib>Pickett, J.S.</creatorcontrib><creatorcontrib>D'Angelo, N.</creatorcontrib><creatorcontrib>Murphy, G.B.</creatorcontrib><title>Plasma density, temperature and turbulence in the wake of the shuttle orbiter</title><title>Planetary and space science</title><description>Plasma density, temperature, and turbulence in the near, mid, and far wake of the
Shuttle orbiter are examined on the basis of
in situ observations by The University of Iowa
Plasma Diagnostics Package (PDP). These observations, the only such measurements in the mid and far wake of the
orbiter, indicate that plasma disturbances produced by the passage of the
orbiter extend downstream for a distance of several hundred meters behind the
orbiter. The electron density profile is found to exhibit nonmonotonic behavior. Most of the 6–40 Hz turbulence in the wake is confined to a region ≈20 m downstream of the
orbiter.
ΔN
e
/
N
e
spectra show a rapid decline in the 10
4–10
5 Hz decade, both in the ambient ionosphere and in the wake.</description><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Physics of the ionosphere</subject><subject>Plasma Physics</subject><subject>Plasmasphere</subject><issn>0032-0633</issn><issn>1873-5088</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1989</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNqFkE1LJDEQhoMoOI7-gzn0YRGFbc13JxdhGdxdQdGDnkM6qca4Pd1jknbx39tti0c9VRX11JvwILQi-IxgIs8xZrTEkrETpU81xoKXagctiKpYKbBSu2jxieyjg5SeMMZS0mqBbu5amza28NClkF9_Fhk2W4g2DxEK2_libOqhhc5BEboiP0Lx3_6Dom_e-_Q45NyOY6xDhniI9hrbJjj6qEv08Pvyfv23vL79c7X-dV06TlQutdSEUiWExdwRRbD3XNSKWc6116pWNXVc176SlaQN8d5RIQTmEhh1jSBsiY7n3G3snwdI2WxCctC2toN-SIYKVknCvweJohWbQT6DLvYpRWjMNoaNja-GYDNJNpNBMxk0Spt3yUaNZz8-8m1ytm2i7VxIn7dSCsbohK1mrLPJmi7H8WWtxhApFJvWF_MaRmcvAaJJLkzKfYjgsvF9-Pobb1j5lwQ</recordid><startdate>19890801</startdate><enddate>19890801</enddate><creator>Tribble, A.C.</creator><creator>Pickett, J.S.</creator><creator>D'Angelo, N.</creator><creator>Murphy, G.B.</creator><general>Elsevier Ltd</general><general>Pergamon Press</general><scope>CYE</scope><scope>CYI</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19890801</creationdate><title>Plasma density, temperature and turbulence in the wake of the shuttle orbiter</title><author>Tribble, A.C. ; Pickett, J.S. ; D'Angelo, N. ; Murphy, G.B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c418t-969122855a04c1810dd45b83a449d98b8b2c49bd76762f1ddc2555046e32cf513</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1989</creationdate><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>External geophysics</topic><topic>Physics of the ionosphere</topic><topic>Plasma Physics</topic><topic>Plasmasphere</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Tribble, A.C.</creatorcontrib><creatorcontrib>Pickett, J.S.</creatorcontrib><creatorcontrib>D'Angelo, N.</creatorcontrib><creatorcontrib>Murphy, G.B.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Planetary and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Tribble, A.C.</au><au>Pickett, J.S.</au><au>D'Angelo, N.</au><au>Murphy, G.B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Plasma density, temperature and turbulence in the wake of the shuttle orbiter</atitle><jtitle>Planetary and space science</jtitle><date>1989-08-01</date><risdate>1989</risdate><volume>37</volume><issue>8</issue><spage>1001</spage><epage>1010</epage><pages>1001-1010</pages><issn>0032-0633</issn><eissn>1873-5088</eissn><coden>PLSSAE</coden><abstract>Plasma density, temperature, and turbulence in the near, mid, and far wake of the
Shuttle orbiter are examined on the basis of
in situ observations by The University of Iowa
Plasma Diagnostics Package (PDP). These observations, the only such measurements in the mid and far wake of the
orbiter, indicate that plasma disturbances produced by the passage of the
orbiter extend downstream for a distance of several hundred meters behind the
orbiter. The electron density profile is found to exhibit nonmonotonic behavior. Most of the 6–40 Hz turbulence in the wake is confined to a region ≈20 m downstream of the
orbiter.
ΔN
e
/
N
e
spectra show a rapid decline in the 10
4–10
5 Hz decade, both in the ambient ionosphere and in the wake.</abstract><cop>Legacy CDMS</cop><pub>Elsevier Ltd</pub><doi>10.1016/0032-0633(89)90054-8</doi><tpages>10</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0032-0633 |
| ispartof | Planetary and space science, 1989-08, Vol.37 (8), p.1001-1010 |
| issn | 0032-0633 1873-5088 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_25376141 |
| source | Access via ScienceDirect (Elsevier); NASA Technical Reports Server |
| subjects | Earth, ocean, space Exact sciences and technology External geophysics Physics of the ionosphere Plasma Physics Plasmasphere |
| title | Plasma density, temperature and turbulence in the wake of the shuttle orbiter |
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