Radio spectrum of two active regions
- 1 August 1970
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 13 (2), 357-371
- https://doi.org/10.1007/bf00153557
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Interpretation of XUV spectroheliogramsSolar Physics, 1969
- Le rayonnement x du soleil lors de l'éclipsé du 20 Mai 1966Solar Physics, 1969
- The spectrum of the slowly varying component of solar radio emission at wavelengths of 3.3 mm ? 21 cmSolar Physics, 1968
- Some characteristics of an S-component of solar radiation identified on November 1966 eclipse at 4.28-cm wavelengthSolar Physics, 1968
- Experimental results from measurements performed during the 12 November 1966 total solar eclipse with a 4.28-cm radio polarimeterIcarus, 1967
- Theoretical Line Intensities. V. Solar UV Emission Lines of Heavy ElementsThe Astrophysical Journal, 1966
- A Model for the Sources of the Slowly Varying Component of Microwave Solar Radiation.The Astrophysical Journal, 1962
- The Solar Corona in Active Regions and the Thermal Origin of the Slowly Varying Component of Solar Radio Radiation.The Astrophysical Journal, 1961
- Etude interferometrique des sources d'activite solaire sur 3 cm de longueur d'ondeSymposium - International Astronomical Union, 1959
- The Origin of Galactic Radio-Frequency RadiationMonthly Notices of the Royal Astronomical Society, 1951