Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

First in Situ Detection of the Magnetic Component of a Solar Type III Radio Wave

  • Authors: Matthieu Kretzschmar, Antonio Vecchio, Vladimir Krasnoselskikh, Milan Maksimovic, Jan Soucek, David Pisa, Claire Gasque, Stuart D. Bale, Thierry Dudok de Wit, Marc Pulupa, Yuri V. Khotyaintsev, Thomas Chust, Guillaume Jannet, Jean-Yves Brochot, Claire Revillet, Patrice Fergeau, Xavier Bonnin, Keith Goetz

Matthieu Kretzschmar et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 6.

SolO: time series of cBSCM (red), ﹩\sqrt{{E}_{y}^{2}{c}_{y}^{2}+{E}_{z}^{2}{c}_{z}^{2}}﹩ (black), and their ratio (purple, right axis), which is n = ck/ω when assuming that the wave is propagating from the Sun center toward SolO, for four frequencies: 136.5, 162.3, 193, and 229.5 kHz.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse