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Fine Structure and Dynamics of the Solar Photosphere (IAU S327)

unprecedented temporal and spatial resolutions. This volume includes recent results in solar physics research presented at the IAU Symposium 327, the;

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Physics of the Sun

Imaging Spectrograph (IRIS), and Parker Solar Probe * Presents step-by-step explanations for calculating numerical models of the photosphere;

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The Sunrise Balloon-Borne Stratospheric Solar Observatory

The central aim of the Sunrise project is to understand the structure and dynamics of the magnetic field in the solar atmosphere. The;

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Solar Surface Magnetism

While the emergence and evolution of solar surface magnetic flux reveals what goes on in the solar interior, the interplay of convection;

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Dynamic Sun

Dynamic Sun presents a comprehensive and authoritative overview of the Sun, from its deep core to the outer corona, and the solar wind;

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Dynamic Sun

Dynamic Sun presents a comprehensive and authoritative overview of the Sun, from its deep core to the outer corona, and the solar wind;

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Fine Structure of Solar Radio Bursts

The study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a;

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Galactic Dynamics in the Era of Large Surveys (IAU S353)

that all aspects of galaxy evolution are strongly influenced by the interplay between the dynamics of stars, gas, and dark matter. IAU;

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Polarimetry (Iau S305)

The advances in solar, planetary, and extrasolar science employing polarimetric tools are far-reaching, and the pace of discovery;

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Physics Of Sun And Star Spots (Iau S273)

made in the fields of solar and stellar magnetism. Sunspots are responsible for the time-varying properties of the Sun, including the solar;

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Solar and Stellar Magnetic Fields (IAU S354)

solar and stellar magnetism is necessary to advance our understanding of magnetic fields. The Proceedings of IAU Symposium 354 present recent;

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Sunspots and Starspots

field and the prevalence of polar spots on stars. The book includes a substantial historical introduction and treats solar and stellar magnetic;

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Proceedings of the International Astronomical Union Symposia and Colloquia

Solar prominences and filaments are large gaseous features extending outward hundreds of thousands of kilometres from the Sun's surface;

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Solar and Stellar Flares and Their Effects on Planets (IAU S

the origin and evolution of life. IAU Symposium 320 discusses the recent advances in observations and theories of solar and stellar flares;

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Solar And Astrophysical Dynamos And Magnetic Activity (Iau S

turbulence, the origin of magnetic fields, and current and future observational projects. The proceedings of IAU S294 are an important asset for;

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The Dynamic Sun

Our Sun is the nearest star and thus an ideal laboratory to study dynamic processes which are related to solar terrestrial physics;

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Precision Asteroseismology (Iau S301)

IAU Symposium 301 highlights the recent advances in the field of asteroseismology and was the twenty-first in a series of pulsation;

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Advances in Plasma Astrophysics (IAU S274)

the scientific community. IAU Symposium 274 discusses recent observational, theoretical and experimental efforts in understanding the basic;

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Multi-Wavelength Observations of Coronal Structure and Dynamics

. The title of the meeting was Multi-Wavelength Observations of Coronal Structure and Dynamics. In these proceedings the many and varied;

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From Interstellar Clouds to Star-Forming Galaxies (IAU S315)

The link between the structure of the interstellar medium in galaxies and the star formation process is a fast-growing area;

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Astrophysical Dynamics (IAU S271)

an essential and revealing tool for assessing the often subtle highly nonlinear regime of such models. In IAU S271 world experts share their;

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The Solar Tachocline

Helioseismology has enabled us to probe the internal structure and dynamics of the Sun, including how its rotation varies in the solar;

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The Solar Tachocline

Helioseismology has enabled us to probe the internal structure and dynamics of the Sun, including how its rotation varies in the solar;

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Adaptive Control of Solar Energy Collector Systems

This book describes methods for adaptive control of distributed-collector solar fields: plants that collect solar energy and deliver it;

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Complex Planetary Systems (IAU S310)

IAU Symposium 310 takes a broad look at the complexity of planetary systems, in terms of the formation and dynamical evolution of planets;

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Formation Evolution and Dynamics of Young Solar Systems

confronted with, and paves the way for a comprehensive understanding of the formation, evolution, and dynamics of young solar systems. The;

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Chromospheric Fine Structure

cells and associated network structures constitute a fundamental and singularly important feature of solar structure in the boundary layers;

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