Literature DB >> 20168602

Extreme uv spectroheliometer on the Apollo Telescope Mount.

E M Reeves, M C Huber, J G Timothy.   

Abstract

The Harvard College Observatory instrument on the Skylab was a seven-channel spectrometer-spectroheliometer operating in the 280-1340-A wavelength range and capable of a variety of observing modes encompassing both spatial and spectral scans of a wide range of solar features. The instrument design and operational performance are described in detail.

Year:  1977        PMID: 20168602     DOI: 10.1364/AO.16.000837

Source DB:  PubMed          Journal:  Appl Opt        ISSN: 1559-128X            Impact factor:   1.980


  2 in total

Review 1.  Coronal Loops: Observations and Modeling of Confined Plasma.

Authors:  Fabio Reale
Journal:  Living Rev Sol Phys       Date:  2014-07-29       Impact factor: 17.417

2.  Solar UV and X-ray spectral diagnostics.

Authors:  Giulio Del Zanna; Helen E Mason
Journal:  Living Rev Sol Phys       Date:  2018-08-31       Impact factor: 17.417

  2 in total

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