Solar Radius Variations at 48 GH[CLC]z[/CLC] Correlated with Solar Irradiance-Reference-Cited by-同舟云学术

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Solar Radius Variations at 48 GH[CLC]z[/CLC] Correlated with Solar Irradiance

Published:1999-07-20 Issue:1 Volume:520 Page:L63-L66
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Costa J. E. R.,Silva A. V R.,Makhmutov V. S.,Rolli E.,Kaufmann P.,Magun A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference29 articles.

1. Bevington, P. R. 1969, Data Reduction and Error Analysis for the Physical Sciences (New York: McGraw-Hill)

2. Accurate Determination of the Solar Photospheric Radius

3. A method for arc-second determination of solar burst emission centers with high time resolution and sensitivity at 48 GHz

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1. Study of solar brightness profiles in the 18–26 GHz frequency range with INAF radio telescopes;Astronomy & Astrophysics;2024-04

2. Study of solar brightness profiles in the 18–26 GHz frequency range with INAF radio telescopes;Astronomy & Astrophysics;2024-04

3. Solar Observations with Single-Dish INAF Radio Telescopes: Continuum Imaging in the 18 – 26 GHz Range;Solar Physics;2022-07

4. Subterahertz radius and limb brightening of the Sun derived from SST and ALMA;Monthly Notices of the Royal Astronomical Society;2021-10-02

5. The Subterahertz Solar Cycle: Polar and Equatorial Radii Derived from SST and ALMA;The Astrophysical Journal;2021-03-01

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