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Space plasma physics: atmospheric emissions photometric imaging experiment
The Atmospheric Emissions Photometric Imaging Experiment detected magnesium ion emissions in the Earth's lower ionosphere. This study analyzed faint atmospheric phenomena using advanced imaging and spectral analysis from Spacelab 1.
Area of Science:
- Atmospheric science
- Space physics
- Optical physics
Background:
- Faint natural and artificial atmospheric emissions are crucial for understanding upper atmospheric processes.
- Previous studies lacked high-resolution imaging and spectral analysis capabilities for these phenomena.
Purpose of the Study:
- To investigate faint atmospheric emission phenomena using photometric imaging.
- To analyze the spectral characteristics of Earth's airglow and spacecraft glow.
Main Methods:
- Utilized the Atmospheric Emissions Photometric Imaging Experiment on Spacelab 1.
- Employed a television system with wide-angle and telephoto optical channels.
- Used a microchannel plate photomultiplier tube and a hand-held image intensifier camera with an objective grating for spectral analysis.
Main Results:
- Successfully imaged optical emissions between 2000 and 7500 angstroms.
- Detected magnesium ion emission features in the lower ionosphere.
- Obtained the spectrum of the spacecraft glow.
Conclusions:
- The experiment demonstrated the capability to study faint atmospheric emissions with high detail.
- Preliminary data confirm the presence of specific ion emissions and provide insights into atmospheric composition.
- Further analysis of the spectral data will enhance our understanding of ionospheric processes and spacecraft-induced atmospheric effects.
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