Bültmann & Gerriets
Aurora
von A. V. Jones
Verlag: Springer Netherlands
Reihe: Geophysics and Astrophysics Monographs Nr. 9
Hardcover
ISBN: 9789027702739
Auflage: Softcover reprint of the original 1st ed. 1974
Erschienen am 31.12.1974
Sprache: Englisch
Format: 235 mm [H] x 155 mm [B] x 18 mm [T]
Gewicht: 493 Gramm
Umfang: 324 Seiten

Preis: 160,49 €
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Klappentext
Inhaltsverzeichnis

Over the past two decades auroral science has developed from a somewhat mysterious and imprecise specialty into a discipline central in the study of the ionosphere and magnetosphere. The investigation of aurora unites scientists with very different backgrounds and interests so that it is difficult to write a self-contained account of the field in a book of reasonable length. In this work I have attempted to include those aspects of theory which I have found valuable in predicting the effects on the atmosphere of auroral particle precipitation. In addition I have attempted to describe the techniques of observation with particular emphasis on optical methods which have been useful. While the aeronomy of aurora has been regarded as central, the mechanisms by which particles are accelerated and precipitated into the atmosphere is of no less interest. This aspect of the subject has however been treated in a briefer fashion since it is a part of the immense and rapidly developing field of magnetospheric science. Generally I have attempted to provide a coherent introduction to auroral science with an emphasis on relatively simple physical interpretations and models. References are given to enable the reader to find more extensive or rigorous discussions of particular topics. A fairly complete, quantitative atlas of the auroral spectrum is included.



1. Introduction.- 1.1. Basic Ideas.- 1.2. Brief History of Auroral Studies.- 1.3. Aurora and the Magnetosphere.- 2. Techniques of Observation.- 2.1. Observations of Total Intensity.- 2.2. Spectroscopic Techniques.- 2.3. Particle Measurements.- 2.4. Radio Reflection Techniques.- 2.5. Magnetic Field Measurements.- 2.6. Other Observing Techniques.- 3. Occurrence and Morphology.- 3.0. Introduction.- 3.1. Occurrence of Visible Aurora.- 3.2. Individual Displays - Auroral Substorms.- 3.3. Detailed Morphology of Auroral Forms.- 3.4. Proton Aurora.- 3.5. Relation of Aurora to Solar Events.- 3.6. Magnetic Disturbances and Aurora.- 3.7. Relation Between Auroral Substorms and the Magnetosphere.- 3.8. Particle Fluxes in the Auroral Oval.- 4. Optical Emissions from Aurora.- 4.1. Optical Transitions and the Auroral Spectrum.- 4.2. Electron Aurora.- 4.3. Proton Aurora.- 5. Aurora and the Ionosphere.- 5.1. Auroral Ionization and Its Effects.- 5.2. Electrical Conductivity, Electric Fields and Currents.- 5.3. Heating Effects in Aurora.- 5.4. Reflection of Radio Waves from the Auroral Ionosphere.- 5.5. Radio Absorption.- 5.6. X-Rays from Auroral Electrons.- 5.7. Radio Emission from Aurora.- 5.8. Infrasonic Emission from Aurora.- 6. Mechanisms of Precipitation of Auroral Particles.- 6.0. Introduction.- 6.1. The Steady State Magnetosphere.- 6.2. Transient Effects and Substorms.- 6.3. Fine Structure of Auroral Precipitation.- 6.4. Conclusion.- Appendices.- 2A. Use of Filter Photometers for Measurement of Absolute Total Intensity of Emission Bands.- 3A. Geomagnetic Latitude and Time.- 3B. Magnetic Disturbance Indices.- 6A. Trajectories of Particles Trapped in a Dipole Field.- References.


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