Abstract
A new high-speed digital solar radio spectrograph has been designed and is being operated at the Clark Lake Radio Observatory in California. The spectrograph design attempts to optimize sensitivity, dynamic range, and frequency-time resolution while utilizing modern high-speed computer data-handling techniques. The system is described and initial data observations are presented.
Similar content being viewed by others
References
Ellis, G. R. A. and McCulloch, P. M.: 1966,Nature 211, 1070.
Ellis, G. R. A. and McCulloch, P. M.: 1967,Australian J. Phys. 20, 583.
De Groot, T. and Van Nieuwkoop, J.: 1968,Solar Phys. 4, 332.
De la Noë, J. and Boischot, A.: 1972,Astron. Astrophys. 20, 55.
Mosier, S. R. and Fainberg, J.: 1974, NASA/GSFC X-693-74-126.
Slottje, C.: 1974,Astron. Astrophys. 32, 107.
Thompson, R. F.: 1970, NASA/GSFC X-692-70-261.
Wild, J. P, and McCready, L. L.: 1950,Australian J. Sci. Res. A3, 387.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Mosier, S.R., Fainberg, J. A new high-speed solar spectrograph for meter and decameter wavelengths. Sol Phys 40, 501–510 (1975). https://doi.org/10.1007/BF00162394
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00162394