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Solar physics in the VUV: the importance of high resolution observations.
Applied optics·2010
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White Light Coronagraph in OSO-7.
Applied Optics
|February 6, 2010
Summary
The Orbiting Solar Observatory 7 (OSO-7) coronagraph captured daily images of the white light corona, revealing transient events and constant solar changes over 2.75 years.
Area of Science:
- Solar physics
- Coronagraphy
- Space-based solar observation
Background:
- The study details a coronagraph designed for the Orbiting Solar Observatory 7 (OSO-7).
- Previous solar observations lacked continuous, high-resolution data of the white light corona.
Purpose of the Study:
- To describe the design and operation of the OSO-7 coronagraph.
- To present findings on the dynamic nature of the solar corona.
Main Methods:
- Utilized a small, externally occulted Lyot-type coronagraph on OSO-7.
- Employed an SEC vidicon detector and a dedicated data system.
- Integrated the instrument into the spacecraft for orbital operation.
Main Results:
- Acquired daily images of the white light corona from 2.8 to 10 solar radii for 2.75 years.
- Recorded the first observations of white light coronal transient events.
- Demonstrated the continuously evolving nature of the solar corona.
Conclusions:
- The OSO-7 coronagraph provided unprecedented long-term data on coronal dynamics.
- Coronal transient events are a significant feature of solar activity.
- The solar corona is a highly dynamic and variable environment.

