Fine Structures of Solar Radio Type III Bursts and their Possible Relationship with Coronal Density Turbulence (2018)

First Author: Chen X
Attributed to:  Consolidated Grant in Solar and Plasma Astrophysics funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1801.07545

Publication URI: https://arxiv.org/abs/1801.07545

Type: Other