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Anisotropic Atomic Hydrogen Distribution in Interplanetary Space
Blum and Farr 1 have suggested modifications of current theories 2,3 concerning the interaction of the solar wind with interstellar hydrogen. One feature of their model involves the motion of the solar system. This motion, coupled with the velocity of the interstellar hydrogen, results in a velocity...
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| Published in: | Nature (London) 1970-02, Vol.225 (5234), p.713-714 |
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| Main Authors: | , , , |
| Format: | Article |
| Language: | English |
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| cites | cdi_FETCH-LOGICAL-c363t-1ffb09dc2aa22d59e2ad87132df40df552d712e1ff64ca710dff5aed339a3e943 |
| container_end_page | 714 |
| container_issue | 5234 |
| container_start_page | 713 |
| container_title | Nature (London) |
| container_volume | 225 |
| creator | CHAMBERS, W. H FEHLAU, P. E FULLER, J. C KUNZ, W. E |
| description | Blum and Farr
1
have suggested modifications of current theories
2,3
concerning the interaction of the solar wind with interstellar hydrogen. One feature of their model involves the motion of the solar system. This motion, coupled with the velocity of the interstellar hydrogen, results in a velocity of 10 to 40 km s
−1
for interstellar hydrogen relative to the solar system. According to Blum and Fahr the relative velocity gives rise to an anisotropic distribution of neutral hydrogen atoms in interplanetary space. The neutral hydrogen density is enhanced in the direction of approach of the interstellar hydrogen and diminished in the opposite hemisphere. The motion of the interstellar hydrogen is assumed to cause a highly aspherical transition region between the hydrogen and the solar wind. |
| doi_str_mv | 10.1038/225713a0 |
| format | article |
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1
have suggested modifications of current theories
2,3
concerning the interaction of the solar wind with interstellar hydrogen. One feature of their model involves the motion of the solar system. This motion, coupled with the velocity of the interstellar hydrogen, results in a velocity of 10 to 40 km s
−1
for interstellar hydrogen relative to the solar system. According to Blum and Fahr the relative velocity gives rise to an anisotropic distribution of neutral hydrogen atoms in interplanetary space. The neutral hydrogen density is enhanced in the direction of approach of the interstellar hydrogen and diminished in the opposite hemisphere. The motion of the interstellar hydrogen is assumed to cause a highly aspherical transition region between the hydrogen and the solar wind.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/225713a0</identifier><identifier>PMID: 16056709</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>Humanities and Social Sciences ; letter ; multidisciplinary ; Science ; Science (multidisciplinary)</subject><ispartof>Nature (London), 1970-02, Vol.225 (5234), p.713-714</ispartof><rights>Springer Nature Limited 1970</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c363t-1ffb09dc2aa22d59e2ad87132df40df552d712e1ff64ca710dff5aed339a3e943</citedby><cites>FETCH-LOGICAL-c363t-1ffb09dc2aa22d59e2ad87132df40df552d712e1ff64ca710dff5aed339a3e943</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,2727,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/16056709$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>CHAMBERS, W. H</creatorcontrib><creatorcontrib>FEHLAU, P. E</creatorcontrib><creatorcontrib>FULLER, J. C</creatorcontrib><creatorcontrib>KUNZ, W. E</creatorcontrib><title>Anisotropic Atomic Hydrogen Distribution in Interplanetary Space</title><title>Nature (London)</title><addtitle>Nature</addtitle><addtitle>Nature</addtitle><description>Blum and Farr
1
have suggested modifications of current theories
2,3
concerning the interaction of the solar wind with interstellar hydrogen. One feature of their model involves the motion of the solar system. This motion, coupled with the velocity of the interstellar hydrogen, results in a velocity of 10 to 40 km s
−1
for interstellar hydrogen relative to the solar system. According to Blum and Fahr the relative velocity gives rise to an anisotropic distribution of neutral hydrogen atoms in interplanetary space. The neutral hydrogen density is enhanced in the direction of approach of the interstellar hydrogen and diminished in the opposite hemisphere. The motion of the interstellar hydrogen is assumed to cause a highly aspherical transition region between the hydrogen and the solar wind.</description><subject>Humanities and Social Sciences</subject><subject>letter</subject><subject>multidisciplinary</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1970</creationdate><recordtype>article</recordtype><recordid>eNp9kD1PwzAQhi0EoqUg8QtQJgRD4GwncbJRlY9WqsQAzJEbXypXrR1sZ-i_x1VL2ZhOunv06L2XkGsKDxR4-chYLiiXcEKGNBNFmhWlOCVDAFamUPJiQC68XwFATkV2Tga0gLwQUA3J09hob4OznW6ScbCbOKZb5ewSTfKsfXB60QdtTaJNMjMBXbeWBoN02-Sjkw1ekrNWrj1eHeaIfL2-fE6m6fz9bTYZz9OGFzyktG0XUKmGScmYyitkUpUxM1NtBqrNc6YEZRixImukoHHX5hIV55XkWGV8RG733s7Z7x59qDfaN7jepbG9r0uoqKAZi-DdHmyc9d5hW3dOb2LemkK9a6v-bSuiNwdnv9ig-gMP9UTgfg_4eDJLdPXK9s7EP_-RGRl6h0fZEfgBLnl8LA</recordid><startdate>19700221</startdate><enddate>19700221</enddate><creator>CHAMBERS, W. H</creator><creator>FEHLAU, P. E</creator><creator>FULLER, J. C</creator><creator>KUNZ, W. E</creator><general>Nature Publishing Group UK</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope></search><sort><creationdate>19700221</creationdate><title>Anisotropic Atomic Hydrogen Distribution in Interplanetary Space</title><author>CHAMBERS, W. H ; FEHLAU, P. E ; FULLER, J. C ; KUNZ, W. E</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c363t-1ffb09dc2aa22d59e2ad87132df40df552d712e1ff64ca710dff5aed339a3e943</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1970</creationdate><topic>Humanities and Social Sciences</topic><topic>letter</topic><topic>multidisciplinary</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>CHAMBERS, W. H</creatorcontrib><creatorcontrib>FEHLAU, P. E</creatorcontrib><creatorcontrib>FULLER, J. C</creatorcontrib><creatorcontrib>KUNZ, W. E</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Nature (London)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>CHAMBERS, W. H</au><au>FEHLAU, P. E</au><au>FULLER, J. C</au><au>KUNZ, W. E</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Anisotropic Atomic Hydrogen Distribution in Interplanetary Space</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><addtitle>Nature</addtitle><date>1970-02-21</date><risdate>1970</risdate><volume>225</volume><issue>5234</issue><spage>713</spage><epage>714</epage><pages>713-714</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><abstract>Blum and Farr
1
have suggested modifications of current theories
2,3
concerning the interaction of the solar wind with interstellar hydrogen. One feature of their model involves the motion of the solar system. This motion, coupled with the velocity of the interstellar hydrogen, results in a velocity of 10 to 40 km s
−1
for interstellar hydrogen relative to the solar system. According to Blum and Fahr the relative velocity gives rise to an anisotropic distribution of neutral hydrogen atoms in interplanetary space. The neutral hydrogen density is enhanced in the direction of approach of the interstellar hydrogen and diminished in the opposite hemisphere. The motion of the interstellar hydrogen is assumed to cause a highly aspherical transition region between the hydrogen and the solar wind.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><pmid>16056709</pmid><doi>10.1038/225713a0</doi><tpages>2</tpages></addata></record> |
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| ispartof | Nature (London), 1970-02, Vol.225 (5234), p.713-714 |
| issn | 0028-0836 1476-4687 |
| language | eng |
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| source | Nature |
| subjects | Humanities and Social Sciences letter multidisciplinary Science Science (multidisciplinary) |
| title | Anisotropic Atomic Hydrogen Distribution in Interplanetary Space |
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