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Babcock Model
Dissertation Franz
General Disclaimer One Or More of The
Predicting the Sun's Polar Magnetic Fields with A
Solar Activity Reconstruction from Historical Observations of Sunspots
Light and Telescopes
The Tayler Instability at Low Magnetic Prandtl Numbers: Chiral Symmetry Breaking and Synchronizable Helicity Oscillations F
Examining Differential Rotation on Stars Using the Matrix
Hydrogen Burning in More Massive Stars
Solar Magnetism
Hydrogen Burning in More Massive Stars and The
The Maunder Minimum
Magnetic Fields in the Sun D. J. Mullan Bartol Research Foundation
PLANETARY RESONANCES, B-I-STABLE OSCILLATION MODES, and SOLAR ACTIVITY CYCLES by El
The Solar Cycle Is Magnetic in Nature and Is Produced by Dynamo Processes Within the Sun (For a Review of the Solar Dynamo See Charbonneau, 2010)
Forecasting Solar Cycle 24 Using Neural Networks
11/6/2018 1 Chapter 8 The
Solar Dynamo Tutorial (SHINE Au
Arxiv:1508.03312V1 [Astro-Ph.SR] 13 Aug 2015
Top View
Habbal Astro110-01 Lecture 19
Non-Axisymmetric Magnetic Flux Transport in the Sun David Martín
Sunspot - Wikipedia, the Free Encyclopedia
The Role of the Sun in Climate Change
Akasofu SI. a New Morphological Theory on the Formation of Sunspots
Hydrogen Burning in More Massive Stars