3D Reconstruction of Coronal Loops by the Principal Component Analysis

3D Reconstruction of Coronal Loops by the Principal Component Analysis

Knowing the three dimensional structure of plasma filaments in the uppermost part of the solar atmosphere, known as coronal loops, and especially their length, is an important parameter in the wave-based diagnostics of this part of the Sun. The combination of observations of the Sun from different p...

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Bibliographic Details
Main Authors: Erwin Verwichte, Valery M. Nakariakov, Giuseppe Nisticò
Format: Article
Language:English
Published: MDPI AG 2013-10-01
Series:Entropy
Subjects:
solar corona
coronal loop
3D reconstruction
Online Access:http://www.mdpi.com/1099-4300/15/10/4520

Internet

http://www.mdpi.com/1099-4300/15/10/4520

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