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Solar dynamo
Magnetism, Dynamo Action and the Solar-Stellar Connection
Rotational Cherecteristics of Solar Radio Emissions
Solar Dynamo Wu Xuanyi Adviser: Prof
Solar and Heliospheric Magnetism in 5D
Strength and Phase of the Solar Dynamo During the Last 12 Cycles
A Forecast of Reduced Solar Activity and Its Implications for Nasa
Solar Variability
Global Solar Dynamo Models: Simulations and Predictions
The Chaotic Solar Cycle
Solar Dynamo
Symmetries of Magnetic Fields Driven by Spherical Dynamos of Exoplanets and Their Host Stars
SOLAR CYCLE #24 and the SOLAR DYNAMO Kenneth Schatten* A.I. Solutions, Inc. Suite 215 10001 Derekwood Lane Lanham, MD 20706
Coupling the Solar Dynamo and the Corona: Solar Wind, Mass and Momentum Losses During the Solar Cycle Rui PINTO (
[email protected]
)1,2, L
An Experimental Plasma Dynamo Program for Investigations of Fundamental Processes in Heliophysics
Alleviating Α Quenching by Solar Wind and Meridional Flows
Solar Orbiter: Exploring the Sun-Heliosphere Connection
Heliophysics 2050 Workshop Preceding January 2021
The Solar Dynamo
Top View
The Solar Dynamo
Chaos in the Solar Cycle: Using Data to Drive Predictions
The Solar Dynamo
Arxiv:1908.06042V4 [Astro-Ph.SR] 21 Jan 2020 Which Are Born on the Interface Between the Tachocline and the Overshoot Layer, Are Developed
How Does the Shape and Thickness of the Tachocline Affect the Distribution of the Toroidal Magnetic fields in the Solar Dynamo?
The Unusual Minimum of Sunspot Cycle 23 a Consequence of Sun's
The Sun and Heliosphere in Three Dimensions
Evidence for a Shallow Thin Magnetic Structure and Solar Dynamo: the Driver of Torsional Oscillations
Solar-Type Dynamo Behaviour in Fully Convective Stars Without a Tachocline
Solar Magnetism - Dynamo
Solar Dynamics Observatory
Combining Models of Coronal Mass Ejections and Solar Dynamos Jörn Warnecke
Structure & Dynamics of the Solar Atmosphere
Solar Cycle #24 and the Solar Dynamo
Solar Dynamo and Geomagnetic Activity
From the Tachocline Into the Heliosphere Andrés Muñoz-Jaramillo Montana State University Anthony Yeates Durham University
Solar Dynamo
Coupling the Solar Dynamo and the Corona: Wind Properties, Mass, and Momentum Losses During an Activity Cycle Rui F
Lectures 4-6: Dynamo Models of the Solar Cycle the Solar Cycle Basic
IAU Symposium 354 “Solar and Stellar Magnetic Fields: Origins and Manifestations” 30 June ‐ 6 July, 2019, Copiapo, Chile
On the Role of Tachoclines in Solar and Stellar Dynamos
On the Origin of the Magnetic Energy in the Quiet Solar Chromosphere
The Pulse of the Sun
Solar Cycle: Observations
Magnetic Helicity and the Solar Dynamo
The Solar Magnetic Field
Characterizing Coronal Mass Ejections in Solar Cycle Analysis *1,2Ryan Manuel D
Demographics of the LWS Heliophysics Summer School (In Haiku Form)
Chromospheric and Coronal Activity in Solar-Like Stars
Solar Dynamo Models and Magnetic Flux Emergence
Exploring the Sun-Heliosphere Connection Solar Orbiter
North-South Asymmetry of the Location of the Heliospheric Current Sheet Revisited G
Exploring the Sun-Heliosphere Connection Solar Orbiter Exploring the Sun-Heliosphere Connection
Solar Dynamo Tutorial (SHINE Au
Radio Burst and Circular Polarization Studies of the Solar Corona at Low Frequencies
Physics of Space Weather Phenomena: a Review
The Solar Atmosphere at Radio Wavelengths
Causes of Solar Activity
The Sun As a Laboratory for Plasma Physics
Heliophysics the SOLAR and SPACE PHYSICS of a NEW ERA
The Magnetic Sun CESAR’S Booklet
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Lessons Learned from Predictions of Solar Cycle 24
The Solar Wind and Heliosphere
The Importance of Polar Observations in Understanding the Solar Dynamo
From the Sun to the Earth: Much More Than Light and Heat