Imagers for the magnetosphere, aurora, and plasmasphere
Creators
- Frank, L.A.1
- Sigwarth, J.B.1
- Williams, D.J.2
- Roelof, E.C.2
- Mitchell, D.G.2
- Gold, R.E.2
- Keath, E.P.2
- Mauk, B.H.2
- Meng, C.I.2
- Carpenter, D.L.3
- Hultqvist, B.K.4
- Lundin, R.N.4
- Siscoe, G.L.5
- Wolf, R.A.6
- Gorney, D.J.7
- Schulz, M.7
- McComas, D.J.8
- Funsten, H.O.8
- Moore, K.R.8
- Smith, B.W.8
- Craven, J.D.9
- Chiu, Y.T.10
- Meier, R.R.11
- Seely, J.F.11
- 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