Artificial auroras in the upper atmosphere: 2. Imaging results
On the ATLAS 1 mission (STS‐45, launched March 24, 1992) two experiments, AEPI (Atmospheric Emissions Photometric Imaging) and SEPAC (Space Experiments with Particle Accelerators) performed the first experiment in a series of active experiments intended to probe the atmosphere, ionosphere and magnet...
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| Veröffentlicht in: | Geophysical research letters 1993-03, Vol.20 (6), p.495-498 |
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| container_end_page | 498 |
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| container_title | Geophysical research letters |
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| creator | Mende, S. B. Burch, J. L. Swenson, G. R. Aamodt, E. K. Geller, S. P. Rairden, R. L. Hassler, P. L. |
| description | On the ATLAS 1 mission (STS‐45, launched March 24, 1992) two experiments, AEPI (Atmospheric Emissions Photometric Imaging) and SEPAC (Space Experiments with Particle Accelerators) performed the first experiment in a series of active experiments intended to probe the atmosphere, ionosphere and magnetosphere with electron beams. The luminous artificial aurora generated by the electron beam interaction was detected and measured by AEPI both in white light and in a narrow wavelength band at 427.8 nm (peak intensity 5 kR). Modelling calculation showed that there was a significant contribution from emissions originating near the spacecraft. The spatial intensity distribution of the observed auroral patch is consistent with emission contribution from both high and low altitude regions. An extended tail in the direction of the shuttle wake was observed in the 427.8 nm channel, consistent with a decay time associated with the dissipation of the hot electron plasma. |
| doi_str_mv | 10.1029/93GL00594 |
| format | Article |
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Imaging results</title><source>Wiley Online Library Journals Frontfile Complete</source><creator>Mende, S. B. ; Burch, J. L. ; Swenson, G. R. ; Aamodt, E. K. ; Geller, S. P. ; Rairden, R. L. ; Hassler, P. L.</creator><creatorcontrib>Mende, S. B. ; Burch, J. L. ; Swenson, G. R. ; Aamodt, E. K. ; Geller, S. P. ; Rairden, R. L. ; Hassler, P. L.</creatorcontrib><description>On the ATLAS 1 mission (STS‐45, launched March 24, 1992) two experiments, AEPI (Atmospheric Emissions Photometric Imaging) and SEPAC (Space Experiments with Particle Accelerators) performed the first experiment in a series of active experiments intended to probe the atmosphere, ionosphere and magnetosphere with electron beams. The luminous artificial aurora generated by the electron beam interaction was detected and measured by AEPI both in white light and in a narrow wavelength band at 427.8 nm (peak intensity 5 kR). Modelling calculation showed that there was a significant contribution from emissions originating near the spacecraft. The spatial intensity distribution of the observed auroral patch is consistent with emission contribution from both high and low altitude regions. An extended tail in the direction of the shuttle wake was observed in the 427.8 nm channel, consistent with a decay time associated with the dissipation of the hot electron plasma.</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/93GL00594</identifier><language>eng</language><publisher>United States: Blackwell Publishing Ltd</publisher><subject>Atmospherics ; AURORAE ; Auroras ; BEAM INJECTION ; BEAMS ; Channels ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; EARTH ATMOSPHERE ; EARTH MAGNETOSPHERE ; ELECTRON BEAMS ; EMISSION ; Imaging ; IONOSPHERE ; LEPTON BEAMS ; PARTICLE BEAMS ; Photometry ; PLANETARY IONOSPHERES 661320 -- Auroral, Ionospheric, & Magnetospheric Phenomena-- (1992-) ; PLASMA ; PULSES ; SIMULATION ; Space shuttles ; SYNTHESIS ; White light</subject><ispartof>Geophysical research letters, 1993-03, Vol.20 (6), p.495-498</ispartof><rights>Copyright 1993 by the American Geophysical Union.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3998-ce96feebffc0405c9a0f9705b699db8a4282868fdd0ad5d6b5c8e66609b068b3</citedby><cites>FETCH-LOGICAL-c3998-ce96feebffc0405c9a0f9705b699db8a4282868fdd0ad5d6b5c8e66609b068b3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F93GL00594$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F93GL00594$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>230,314,777,781,882,1412,27905,27906,45555,45556</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/6771949$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Mende, S. B.</creatorcontrib><creatorcontrib>Burch, J. L.</creatorcontrib><creatorcontrib>Swenson, G. R.</creatorcontrib><creatorcontrib>Aamodt, E. K.</creatorcontrib><creatorcontrib>Geller, S. P.</creatorcontrib><creatorcontrib>Rairden, R. L.</creatorcontrib><creatorcontrib>Hassler, P. L.</creatorcontrib><title>Artificial auroras in the upper atmosphere: 2. Imaging results</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>On the ATLAS 1 mission (STS‐45, launched March 24, 1992) two experiments, AEPI (Atmospheric Emissions Photometric Imaging) and SEPAC (Space Experiments with Particle Accelerators) performed the first experiment in a series of active experiments intended to probe the atmosphere, ionosphere and magnetosphere with electron beams. The luminous artificial aurora generated by the electron beam interaction was detected and measured by AEPI both in white light and in a narrow wavelength band at 427.8 nm (peak intensity 5 kR). Modelling calculation showed that there was a significant contribution from emissions originating near the spacecraft. The spatial intensity distribution of the observed auroral patch is consistent with emission contribution from both high and low altitude regions. An extended tail in the direction of the shuttle wake was observed in the 427.8 nm channel, consistent with a decay time associated with the dissipation of the hot electron plasma.</description><subject>Atmospherics</subject><subject>AURORAE</subject><subject>Auroras</subject><subject>BEAM INJECTION</subject><subject>BEAMS</subject><subject>Channels</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>EARTH ATMOSPHERE</subject><subject>EARTH MAGNETOSPHERE</subject><subject>ELECTRON BEAMS</subject><subject>EMISSION</subject><subject>Imaging</subject><subject>IONOSPHERE</subject><subject>LEPTON BEAMS</subject><subject>PARTICLE BEAMS</subject><subject>Photometry</subject><subject>PLANETARY IONOSPHERES 661320 -- Auroral, Ionospheric, & Magnetospheric Phenomena-- (1992-)</subject><subject>PLASMA</subject><subject>PULSES</subject><subject>SIMULATION</subject><subject>Space shuttles</subject><subject>SYNTHESIS</subject><subject>White light</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1993</creationdate><recordtype>article</recordtype><recordid>eNqN0MFK5EAQBuBmUXDUPfgGYU96yFjpJJ0uD4KKjrqDu8iAx6bTqTitmSR2d1Df3kgWbwueqg7fX1A_YwcJzBPgeIzpYgmQY_aDzRLMslgCFFtsBoDjzguxw3a9fwKAFNJkxk7PXLC1NVY3kR5c57SPbBuFNUVD35OLdNh0vl-To5OIz6ObjX607WPkyA9N8Ptsu9aNp5__5h5bXV2uLq7j5Z_FzcXZMjYpoowNoaiJyro2kEFuUEONBeSlQKxKqTMuuRSyrirQVV6JMjeShBCAJQhZpnvs13S288Eqb2wgszZd25IJShTF-CmO6HBCveteBvJBbaw31DS6pW7wKikAC8wF_wbNOSJPMhQjPZqocZ33jmrVO7vR7l0loD4rV1-Vj3Y-2Vfb0Pv_oVrcL4XI5BiIp4D1gd6-Ato9j1-lRa4e7hbq_Jb_FXe_H9Qq_QBHho6e</recordid><startdate>19930319</startdate><enddate>19930319</enddate><creator>Mende, S. B.</creator><creator>Burch, J. L.</creator><creator>Swenson, G. R.</creator><creator>Aamodt, E. K.</creator><creator>Geller, S. P.</creator><creator>Rairden, R. L.</creator><creator>Hassler, P. L.</creator><general>Blackwell Publishing Ltd</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TV</scope><scope>7UA</scope><scope>C1K</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>KR7</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>19930319</creationdate><title>Artificial auroras in the upper atmosphere: 2. Imaging results</title><author>Mende, S. B. ; Burch, J. L. ; Swenson, G. R. ; Aamodt, E. K. ; Geller, S. P. ; Rairden, R. L. ; Hassler, P. 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B.</au><au>Burch, J. L.</au><au>Swenson, G. R.</au><au>Aamodt, E. K.</au><au>Geller, S. P.</au><au>Rairden, R. L.</au><au>Hassler, P. L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Artificial auroras in the upper atmosphere: 2. Imaging results</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>1993-03-19</date><risdate>1993</risdate><volume>20</volume><issue>6</issue><spage>495</spage><epage>498</epage><pages>495-498</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>On the ATLAS 1 mission (STS‐45, launched March 24, 1992) two experiments, AEPI (Atmospheric Emissions Photometric Imaging) and SEPAC (Space Experiments with Particle Accelerators) performed the first experiment in a series of active experiments intended to probe the atmosphere, ionosphere and magnetosphere with electron beams. The luminous artificial aurora generated by the electron beam interaction was detected and measured by AEPI both in white light and in a narrow wavelength band at 427.8 nm (peak intensity 5 kR). Modelling calculation showed that there was a significant contribution from emissions originating near the spacecraft. The spatial intensity distribution of the observed auroral patch is consistent with emission contribution from both high and low altitude regions. An extended tail in the direction of the shuttle wake was observed in the 427.8 nm channel, consistent with a decay time associated with the dissipation of the hot electron plasma.</abstract><cop>United States</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/93GL00594</doi><tpages>4</tpages></addata></record> |
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| ispartof | Geophysical research letters, 1993-03, Vol.20 (6), p.495-498 |
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| language | eng |
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| source | Wiley Online Library Journals Frontfile Complete |
| subjects | Atmospherics AURORAE Auroras BEAM INJECTION BEAMS Channels CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS EARTH ATMOSPHERE EARTH MAGNETOSPHERE ELECTRON BEAMS EMISSION Imaging IONOSPHERE LEPTON BEAMS PARTICLE BEAMS Photometry PLANETARY IONOSPHERES 661320 -- Auroral, Ionospheric, & Magnetospheric Phenomena-- (1992-) PLASMA PULSES SIMULATION Space shuttles SYNTHESIS White light |
| title | Artificial auroras in the upper atmosphere: 2. Imaging results |
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