We describe chamber tests of simulated electrodynamic tethers (EDTs) of different geometries operating in a dense, high-speed plasma. The geometries tested were cylindrical, flat-ribbon, and sparse-ribbon or mesh. Several important conclusions that can be drawn from the tests are as follows: the currents collected by cylinder are close to what would be predicted via orbital-motion-limited (OML) current collection theory. The tape tether had comparable current levels to a theoretical equal area OML cylinder collector. However, I-V behavior clearly is different at nearest distances (similar to 15 lambda (D) tape width) as compared to furthest test distances (similar to 6 lambda (D) tape width). The tape tether did better than a theoretical equal mass solid cylinder. A "knee" in the I-V curves can be seen in the tape/mesh data at a potential that is just above the estimated energy of the incoming beam of ions, at least for the closest distances where Debye length is smallest. Below this knee the current increases rapidly as voltage is increased. Above the knee the current increases at a rate one might expect from OML. current-collection models depending on the relative width. This likely is an example of high-speed plasma flow effect. Perpendicular tape orientation performed slightly better than parallel.
机构:
Univ Michigan, Dept Elect Engn & Comp Sci, Radiat Lab, Ann Arbor, MI 48109 USAUniv Michigan, Dept Elect Engn & Comp Sci, Radiat Lab, Ann Arbor, MI 48109 USA
Bell, Iverson C., III
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Leon, Omar
Miars, Grant C.
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Univ Michigan, Dept Elect Engn & Comp Sci, Radiat Lab, Ann Arbor, MI 48109 USAUniv Michigan, Dept Elect Engn & Comp Sci, Radiat Lab, Ann Arbor, MI 48109 USA
Miars, Grant C.
Gilchrist, Brian E.
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Univ Michigan, Dept Elect Engn & Comp Sci, Radiat Lab, Ann Arbor, MI 48109 USA
Univ Michigan, Climate & Space Sci Engn Dept, Ann Arbor, MI 48109 USAUniv Michigan, Dept Elect Engn & Comp Sci, Radiat Lab, Ann Arbor, MI 48109 USA
机构:
Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Chinese Acad Sci, State Key Lab Space Weather, Beijing 100190, Peoples R ChinaPeking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Fu SuiYan
Shi QuanQi
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Shandong Univ, Sch Space Sci & Phys, Weihai 264209, Peoples R ChinaPeking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Shi QuanQi
Wang Chi
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Shandong Univ, Sch Space Sci & Phys, Weihai 264209, Peoples R ChinaPeking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Wang Chi
Parks, George
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Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USAPeking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Parks, George
Zheng Ling
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Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R ChinaPeking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Zheng Ling
Zheng Hao
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Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R ChinaPeking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Zheng Hao
Sun WeiJie
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Shandong Univ, Sch Space Sci & Phys, Weihai 264209, Peoples R ChinaPeking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
Sun WeiJie
CHINESE SCIENCE BULLETIN,
2011,
56
(12):
: 1182
-
1187
机构:
Emperor Alexander I St. Petersburg State Transport University, St. PetersburgEmperor Alexander I St. Petersburg State Transport University, St. Petersburg
Kim K.K.
Panychev A.Y.
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Emperor Alexander I St. Petersburg State Transport University, St. PetersburgEmperor Alexander I St. Petersburg State Transport University, St. Petersburg
Panychev A.Y.
Blazhko L.S.
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Emperor Alexander I St. Petersburg State Transport University, St. PetersburgEmperor Alexander I St. Petersburg State Transport University, St. Petersburg
Blazhko L.S.
Kolesova A.V.
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Emperor Alexander I St. Petersburg State Transport University, St. PetersburgEmperor Alexander I St. Petersburg State Transport University, St. Petersburg