The low-energy neutral atom imager for IMAGE

被引:114
|
作者
Moore, TE [1 ]
Chornay, DJ
Collier, MR
Herrero, FA
Johnson, J
Johnson, MA
Keller, JW
Laudadio, JF
Lobell, JF
Ogilvie, KW
Rozmarynowski, P
Fuselier, SA
Ghielmetti, AG
Hertzberg, E
Hamilton, DC
Lundgren, R
Wilson, P
Walpole, P
Stephen, TM
Peko, BL
Van Zyl, B
Wurz, P
Quinn, JM
Wilson, GR
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Lockheed Martin Adv Technol Ctr, Palo Alto, CA 94304 USA
[3] Univ Maryland, College Pk, MD 20742 USA
[4] Univ Denver, Denver, CO 80208 USA
[5] Univ Bern, CH-301 Bern, Switzerland
[6] Univ New Hampshire, Durham, NH 03824 USA
[7] Mission Res Corp, Nashua, NH 03062 USA
关键词
D O I
10.1023/A:1005211509003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The 'Imager for Magnetosphere-to-Aurora Global Exploration' (IMAGE) will be launched early in the year 2000. It will be the first mission dedicated to imaging, with the capability to determine how the magnetosphere changes globally in response to solar storm effects in the solar wind, on time scales as short as a few minutes. The low energy neutral atom (LENA) imager uses a new atom-to-negative ion surface conversion technology to image the neutral atom flux and measure its composition (H and O) and energy distribution (10 to 750 eV). LENA uses electrostatic optics techniques for energy (per charge) discrimination and carbon foil time-of-flight techniques for mass discrimination. It has a 90 degrees x8 degrees field-of-view in 12 pixels, each nominally 8 degrees x8 degrees. Spacecraft spin provides a total field-of-view of 90 degrees x360 degrees, comprised of 12x45 pixels. LENA is designed to image fast neutral atom fluxes in its energy range, emitted by auroral ionospheres or the sun, or penetrating from the interstellar medium. It will thereby determine how superthermal plasma heating is distributed in space, how and why it varies on short time scales, and how this heating is driven by solar activity as reflected in solar wind conditions.
引用
收藏
页码:155 / 195
页数:41
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