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The solar red-shift

Abstract:

Shortly after Rowland's fundamental study of the wavelengths of Fraunhofer lines, Jewell in 1896 observed that the solar wavelengths were shifted to the red side of the corresponding wavelengths observed in the laboratory. This shift became known as the red shift of solar lines, and at first led to various erroneous concepts of conditions in the solar atmosphere. Moreover, in 1907, Halm discovered that the solar wavelengths were not themselves constant, but depended upon the radial distanc...

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Peer review status:
Peer reviewed

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Department:
University of Oxford
Role:
Author
Type of award:
DPhil
Level of award:
Doctoral
Awarding institution:
University of Oxford
Source identifiers:
601870562
UUID:
uuid:ca4cb627-3d99-4105-a9aa-e3c976c52780
Local pid:
polonsky:9:46
Deposit date:
2017-10-05

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