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Related Experiment Video

Updated: Jun 17, 2026

Scattering And Absorption of Light in Planetary Regoliths

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Ultraviolet measurements in planetary atmospheres.

¹The Johns Hopkins University, Baltimore,Maryland 21218, USA.

|January 9, 2010

Summary

Advancements in optical and electronic components enhance far ultraviolet rocket spectrophotometry, enabling the measurement of weaker spectral features in the 1100-3000 Angstrom range.

Area of Science:

Aerospace Engineering
Spectroscopy
Atmospheric Physics

Background:

Far ultraviolet (FUV) spectrophotometry is crucial for studying atmospheric phenomena.
Previous limitations in optical and electronic components hindered detailed FUV spectral analysis.

Purpose of the Study:

To discuss the impact of new optical and electronic components on FUV rocket spectrophotometry.
To review recent experimental results from Earth's airglow and aurorae studies.

Main Methods:

Review of recent experimental data from FUV spectrophotometry.
Analysis of the performance of advanced optical and electronic components in FUV spectroscopy.

Main Results:

New components significantly improve FUV rocket spectrophotometry capabilities.

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Scattering And Absorption of Light in Planetary Regoliths

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Published on: July 1, 2019

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Weaker spectral features in the 1100-3000 Angstrom range are measurable with greater sensitivity.

Conclusions:

Latest component developments offer unprecedented opportunities for FUV atmospheric research.
Enhanced FUV spectrophotometry will lead to a deeper understanding of Earth's airglow and aurorae.