A Composite, High-Resolution Solar Spectrum From 2080 to 3600 A

To satisfy a need for digitized information on the solar spectrum between 2000 and 3600 A, an attempt was made to combine the available measurements into a composite, high-resolution solar spectrum in absolute units. The final values, though not absolutely accurate, should be adequate for many geophysical studies involving the near and middle ultraviolet portion of the solar spectrum.

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Copyright Author(s). This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.
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Resource Support Email opensky@ucar.edu
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Author Furukawa, Paul
Haagenson, Philip
Scharberg, Mary Jo
Publisher UCAR/NCAR - Library
Publication Date 1967-01-01T00:00:00
Digital Object Identifier (DOI) Not Assigned
Alternate Identifier N/A
Resource Version N/A
Topic Category geoscientificInformation
Progress N/A
Metadata Date 2023-08-18T18:04:05.567744
Metadata Record Identifier edu.ucar.opensky::technotes:18
Metadata Language eng; USA
Suggested Citation Furukawa, Paul, Haagenson, Philip, Scharberg, Mary Jo. (1967). A Composite, High-Resolution Solar Spectrum From 2080 to 3600 A. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d71v5dcv. Accessed 18 April 2024.

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