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Quiet Sun Magnetic Fields

AIP Conference Proceedings, 2003
The seemingly un‐magnetized part of the solar surface is not really un‐magnetized. It is occupied by magnetic structures producing low polarization which, therefore, escape detection in traditional measurements. Since most of the solar surface belongs to this category, the quiet Sun magnetic fields can easily carry most of the magnetic flux and energy ...
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The Sun's Magnetic Field

Annual Review of Astronomy and Astrophysics, 1963
The techniques and instruments for measuring the solar magnetic field are outlined. The poloidal field and lowlatitude fields are discussed. The magnetic fields associated with sunspots, flares, stable filaments, and granules are considered. The solar magnetic cycle and related phenomena are also discussed. (C.E.S.)
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The Sun’s Magnetic Fields

2015
In this introductory chapter we first briefly describe some overall characteristics of the sun, and then take a closer look at the sun’s magnetic surfaces. We shall see that highly advanced space and ground-based observations show various magnetic elements, their clusters, and mass flows in great detail. The chapter is concluded with the description of
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Magnetic field generation on the sun

Astronomical & Astrophysical Transactions, 2001
Abstract We consider the contradiction between the minimum entropy production theorem and the conception of the solar differential rotation being maintained by viscous forces. This difficulty can be overcome if the condition that the highest possible part of the total energy entering the convection zone from below is transformed into the magnetic field
Y. V. Vandakurov, E. M. Sklyarova
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Magnetic fields of the Sun and stars

Uspekhi Fizicheskih Nauk, 1966
CONTENTS Introduction 1 1. Methods and technique of measuring magnetic fields 2 2. General magnetic field of the Sun 7 3. Strong magnetic fields in active regions of the Sun 14 4.
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The Sun and Its Restless Magnetic Field

2004
The permanently changing magnetic field of the Sun is the ultimate driver of the various effects refered to as space weather. This chapter gives an overview of the physics of the solar magnetic field and its variability. This includes a brief description of the structure of the Sun, and a discussion of the origin of the solar magnetic field.
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Global wave patterns in the Sun's magnetic field

Astrophysics and Space Science, 1988
When the observed pattern of solar magnetic fields is decomposed in its spherical-harmonic components and a time series analysis is performed, a resonant global wave pattern is revealed. The power spectrum indicates modes with discrete frequencies, obeying a strict parity selection rule in the case of the zonal, rotationally-symmetric modes (with ...
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Local Magnetic Fields on the Sun

1972
The strongest magnetic fields on the sun are those of sunspots. Although their magnetic fields have been studied for a long time much remains unknown about the magnetism of these principal sources. At sufficiently large distances from a spot the magnetic field can, apparently, be well approximated as that of a dipole submerged below the solar ...
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Magnetic resonance linear accelerator technology and adaptive radiation therapy: An overview for clinicians

Ca-A Cancer Journal for Clinicians, 2022
William A Hal   +2 more
exaly  

Magnetic fields of 30 to 100 kG in the cores of red giant stars

Nature, 2022
Gang Li   +2 more
exaly  

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