3D Coronal Slow Modes: Towards 3D Seismology (2009)
Attributed to:
Determining the fundamental nature of the solar atmosphere: applying Bayesian analysis methods to Hinode observations
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.0903.4039
Publication URI: https://arxiv.org/abs/0903.4039
Type: Other