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This title is printed to order. This book may have been self-published. If so, we cannot guarantee the quality of the content. In the main most books will have gone through the editing process however some may not. We therefore suggest that you be aware of this before ordering this book. If in doubt check either the author or publisher’s details as we are unable to accept any returns unless they are faulty. Please contact us if you have any questions.
The Sun: A Laboratory for Astrophysics presents an educational overview of many aspects of solar physics, in an astrophysical context, following two decades of major strides in solar studies from spacecraft and pioneering studies of the Sun as a star. The authors have experience in both theory and observation and some in instrumentation in this field. The first third of the book addresses the global physics of the Sun and its relation to other stars, covering energy generation, interior structure models, convection, magnetic field generation as well as constraints obtained from surface observations, both seismic and magnetic. The second portion comprises a mixture of theory and diagnostics of the solar atmosphere and of instrumentation for observations from radio wavelengths to high energies. The final third concerns solar activity and flares, their relation to stellar activity and their importance for the activities of humankind.
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This title is printed to order. This book may have been self-published. If so, we cannot guarantee the quality of the content. In the main most books will have gone through the editing process however some may not. We therefore suggest that you be aware of this before ordering this book. If in doubt check either the author or publisher’s details as we are unable to accept any returns unless they are faulty. Please contact us if you have any questions.
The Sun: A Laboratory for Astrophysics presents an educational overview of many aspects of solar physics, in an astrophysical context, following two decades of major strides in solar studies from spacecraft and pioneering studies of the Sun as a star. The authors have experience in both theory and observation and some in instrumentation in this field. The first third of the book addresses the global physics of the Sun and its relation to other stars, covering energy generation, interior structure models, convection, magnetic field generation as well as constraints obtained from surface observations, both seismic and magnetic. The second portion comprises a mixture of theory and diagnostics of the solar atmosphere and of instrumentation for observations from radio wavelengths to high energies. The final third concerns solar activity and flares, their relation to stellar activity and their importance for the activities of humankind.