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Updated: Jun 16, 2026
10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
Extreme uv spectroheliometer on the Apollo Telescope Mount.
Applied Optics
|February 20, 2010
Summary
The Skylab solar instrument, a seven-channel spectrometer-spectroheliometer, captured detailed spatial and spectral data across a wide wavelength range. Its design and performance for observing solar features are thoroughly documented.
Area of Science:
- Solar physics
- Astronomy
- Astrophysics
Background:
- The Skylab mission provided a unique platform for solar observation.
- Understanding solar features requires advanced spectroscopic instruments.
Purpose of the Study:
- To detail the design of the Harvard College Observatory's solar instrument.
- To describe the operational performance of the spectrometer-spectroheliometer.
Main Methods:
- Utilized a seven-channel spectrometer-spectroheliometer.
- Operated within the 280-1340 Angstrom wavelength range.
- Employed spatial and spectral scanning modes for solar feature analysis.
Main Results:
- The instrument successfully performed spatial and spectral scans.
- Data was collected across a broad spectrum of solar emissions.
- The instrument's capabilities for observing diverse solar features were demonstrated.
Conclusions:
- The Harvard College Observatory instrument was a versatile tool for solar research.
- Detailed documentation of the instrument's design and performance is now available.
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