ISBN-13: 9789402416473 / Angielski / Miękka / 2019 / 426 str.
ISBN-13: 9789402416473 / Angielski / Miękka / 2019 / 426 str.
Editorial: Measuring Solar Magnetic Fields—An Outline of History, Current Status and Challenges.- History of Solar Magnetic Fields Since George Ellery Hale.- Measurements of Photospheric and Chromospheric Magnetic Fields.- Polar Field Reversals and Active Region Decay.- Radiative Diagnostics in the Solar Photosphere and Chromosphere.- Magnetic Diagnostics of the Solar Corona: Synthesizing Optical and Radio Techniques.- The Physics and Diagnostic Potential of Ultraviolet Spectropolarimetry.- Minimal Magnetic States of the Sun and the Solar Wind: Implications for the Origin of the Slow Solar Wind.- Coronal Magnetic Field Models.- Solar Magnetoconvection and Small-Scale Dynamo.- The Life Cycle of Active Region Magnetic Fields.- Surface Flux Transport and the Evolution of the Sun’s Polar Fields.- The Global Solar Dynamo.- Prospects of Solar Magnetometry—From Ground and in Space.
André Balogh is Emeritus Professor of Space Physics, Imperial College, London.Through his career since the 1960s he led or participated in numerous space investigations into the physics of the heliospheric magnetic field and its interaction with the solar wind and the Earth’s space environment. As Principal Investigator of the magnetic field investigation on the joint ESA/NASA Ulysses (1990-2009) mission he led numerous research projects to discover the dynamics and evolution of the three-dimensional heliospheric magnetic field and its connection with solar magnetism through the solar activity cycle. From 2005 to 2010 he was a Director of the International Space Science Institute where he initiated and organised a series of workshops on magnetic fields in the solar system and beyond, and has been the editor of 12 volumes in the Space Science Series of ISSI.
This volume provides an in-depth review of all aspects of solar magnetic fields. Written by world-leading experts, these thirteen papers cover all regions of the subject from the solar interior, photosphere, chromosphere, active regions, and corona out to the solar wind. The history of solar magnetic fields as well as the necessary instrumentation are also covered. The volume serves as both a reference for researchers and a starting point for graduate students.
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