Published February 1994 | Version v1
Journal article

Imagers for the magnetosphere, aurora, and plasmasphere

  • 1. Univ. of Iowa, Iowa City, IA (United States). Dept. of Physics and Astronomy
  • 2. Johns Hopkins Univ., Laurel, MD (United States). Applied Physics Lab.
  • 3. Stanford Univ., CA (United States). Starlab/Electrical Engineering Dept.
  • 4. Swedish Inst. of Space Physics, Kiruna (Sweden)
  • 5. Boston Univ., MA (United States). Center for Space Physics
  • 6. Rice Univ., Houston, TX (United States). Space Physics and Astronomy Dept.
  • 7. Aerospace Corp., Los Angeles, CA (United States). Space and Environmental Technology Center
  • 8. Los Alamos National Lab., NM (United States)
  • 9. Univ. of Alaska, Fairbanks, AK (United States). Geophysical Inst.
  • 10. Lockheed Palo Alto Research Lab., CA (United States)
  • 11. Naval Research Lab., Washington, DC (United States)

Description

The authors present a small Explorer mission, Imagers for the Magnetosphere, Aurora, and Plasmasphere (IMAP), to provide the first global magnetospheric images that will allow a systematic study of major regions of the magnetosphere, their dynamics, and their interactions. The mission objective is to obtain simultaneous images of the inner magnetosphere (ring current and trapped particles), the plasma-sphere, the aurora, and auroral upflowing ions. The instruments are (1) a Low Energy Neutral Particle Imagers for imaging H and O atoms, separately, in the energy range of ∼1 to 30 keV, in several energy passbands; (2) an Energetic Neutral Particle Imager for imaging H atoms in the energy range ∼15 to 200 keV and, separately, O atoms in the energy range ∼60 to 200 keV, each in several energy pass-bands; (3) an Extreme-Ultraviolet imager to obtain images of the plasmasphere the distribution of cold He+ by means of He+ (30.4 nm) emissions; and (4) a Far-Ultraviolet Imaging Monochromator to provide images of the aurora and the geocorona. All images will be obtained with time and spatial resolutions appropriate to the global and macroscale structures to be observed. IMAP promises new quantitative analyses that will provide great advances in insight and knowledge of global and macroscale magnetospheric parameters

Additional details

Publishing Information

Journal Title
Optical Engineering
Journal Volume
33
Journal Issue
2
Journal Page Range
p. 391-408.
ISSN
0091-3286
CODEN
OPEGAR

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
25051853
Subject category
S58: GEOSCIENCES;
Descriptors DEI
AURORAE; DYNAMICS; EARTH MAGNETOSPHERE; EXPLORER SATELLITES; HYDROGEN; ION DRIFT; MEASURING INSTRUMENTS; OXYGEN; REMOTE SENSING
Descriptors DEC
EARTH ATMOSPHERE; ELEMENTS; MECHANICS; NONMETALS; SATELLITES