Riemannian and filamentary geometries..
Garcia de Andrade
TL;DR
This paper explores the application of Riemannian and filamentary geometries to analyze stretched filamentary dynamos in the solar corona, aiming to better understand solar magnetic phenomena.
Contribution
It introduces a novel geometric framework combining Riemannian and filamentary geometries for studying solar coronal dynamos.
Findings
Enhanced understanding of magnetic field structures in the solar corona
Potential insights into solar dynamo mechanisms
New geometric tools for solar physics analysis
Abstract
Riemannian and filamentary geometries are used to investigate the stretched filamentary dynamos against solar data in solar corona.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Geomagnetism and Paleomagnetism Studies