On the possibility of determining the coronal magnetic field from solar type III radio burst observations

ISSN： 0038-0938

Source： Solar Physics, Vol.185, Iss.1, 1999-03, pp. : 193-204

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Investigation of the Coronal Magnetic Field Using a Type II Solar Radio Burst

By Vasanth V. Umapathy S. Vršnak Bojan Žic Tomislav Prakash O.

Solar Physics, Vol. 289, Iss. 1, 2014-01 ,pp. : 251-261

Springer Publishing Company

Access to resources Recommend Favorite

Solar Radio Burst (Type III)

By Om Vats H.

Astrophysics and Space Science, Vol. 243, Iss. 1, 1996-01 ,pp. : 251-254

Springer Publishing Company

Access to resources Recommend Favorite

On the Gradient of Coronal Magnetic Fields from Radio Observations

By Gelfreikh G.B. Pilyeva N.A. Ryabov B.I.

Solar Physics, Vol. 170, Iss. 2, 1997-02 ,pp. : 253-264

Springer Publishing Company

Access to resources Recommend Favorite

Radio Observations of Gyroresonance Emission from Coronal Magnetic Fields

By White S.M. Kundu M.R.

Solar Physics, Vol. 174, Iss. 1-2, 1997-08 ,pp. : 31-52

Springer Publishing Company

Access to resources Recommend Favorite

An Estimation of the Coronal Magnetic Field Strength From Spectrographic Observations in the Microwave Range

By Ledenev V.G. Karlický M. Yan Y. Fu Q.

Solar Physics, Vol. 202, Iss. 1, 2001-08 ,pp. : 71-79

Springer Publishing Company

Access to resources Recommend Favorite