Lanzerotti / Schulz | Particle Diffusion in the Radiation Belts | Buch | 978-3-642-65677-4 | sack.de

Buch, Englisch, Band 7, 218 Seiten, Format (B × H): 155 mm x 235 mm, Gewicht: 365 g

Reihe: Physics and Chemistry in Space

Lanzerotti / Schulz

Particle Diffusion in the Radiation Belts


Softcover Nachdruck of the original 1. Auflage 1974
ISBN: 978-3-642-65677-4
Verlag: Springer

Buch, Englisch, Band 7, 218 Seiten, Format (B × H): 155 mm x 235 mm, Gewicht: 365 g

Reihe: Physics and Chemistry in Space

ISBN: 978-3-642-65677-4
Verlag: Springer


The advent of artificial earth satellites in 1957-58 opened a new dimension in the field of geophysical exploration. Discovery of the earth's radiation belts, consisting of energetic electrons and ions (chiefly protons) trapped by the geomagnetic field, followed almost immediately [1,2]' This largely unexpected development spurred a continuing interest in magnetospheric exploration, which so far has led to the launching of several hundred carefully instrumented spacecraft. Since their discovery, the radiation belts have been a subject of intensive theoretical analysis also. Over the years, a semiquantitative understanding of the governing dynamical processes has gradually evol­ ved. The underlying kinematical framework of radiation-belt theory is given by the adiabatic theory of charged-particle motion [3J, and the interesting dynamical phenomena are associated with the violation of one or more of the kinematical invariants of adiabatic motion. Among the most important of the operative dynamical processes are those that act in a stochastic manner upon the radiation-belt particles. Such stochastic processes lead to the diffusion of particle distributions with respect to the adiabatic invariants. The observational data indicate that some form of particle diffusion plays an essential role in virtually every aspect of the radiation belts.

Lanzerotti / Schulz Particle Diffusion in the Radiation Belts jetzt bestellen!

Zielgruppe


Research

Weitere Infos & Material


I. Adiabatic Invariants and Magnetospheric Models.- I.1 Preliminary Considerations.- I.2 Action-Angle Variables.- I.3 Liouville’s Theorem.- I.4 The Dipole Field.- I.5 The Distorted Field.- I.6 Magnetospheric Electric Fields.- I.7 Flux Mapping and Shell Tracing.- II. Pitch-Angle Diffusion.- II.1 Violation of an Adiabatic Invariant.- II.2 Collisions.- II.3 Wave-Particle Interactions.- II.4 Bounce Resonance.- II.5 Cyclotron Resonance.- II.6 Limit on Trapped Flux.- II.7 Weak Diffusion and Strong Diffusion.- III. Radial Diffusion.- III.1 Violation of the Third Invariant.- III.2 Magnetic Impulses.- III.3 Electrostatic Impulses.- III.4 Bounce Resonance.- III.5 Cyclotron Resonance.- III.6 Bohm Diffusion.- III.7 Shell Splitting.- III.8 Diffusion in More Than One Mode.- IV. Prototype Observations.- IV.1 Preliminary Considerations.- IV.2 Decay of Particle Flux (Inner Zone).- IV.3 Decay of Particle Flux (Outer Zone).- IV.4 Statistical Observations.- IV.5 Static Flux Profiles.- IV.6 Time-Varying Flux Profiles.- I V.7 Fluctuating Magnetospheric Fields.- IV.8 Drift Echoes.- V. Methods of Empirical Analysis.- V.1 Basic Objectives.- V.2 Pitch-Angle Eigenmodes.- V.3 Quadrature (Spatial).- V.4 Quadrature (Temporal).- V.5 Variational Method.- V.6 Temporal Integration.- V.7 Spatial Integration.- VI. Summary.- References.- Frequently used Symbols.



Ihre Fragen, Wünsche oder Anmerkungen
Vorname*
Nachname*
Ihre E-Mail-Adresse*
Kundennr.
Ihre Nachricht*
Lediglich mit * gekennzeichnete Felder sind Pflichtfelder.
Wenn Sie die im Kontaktformular eingegebenen Daten durch Klick auf den nachfolgenden Button übersenden, erklären Sie sich damit einverstanden, dass wir Ihr Angaben für die Beantwortung Ihrer Anfrage verwenden. Selbstverständlich werden Ihre Daten vertraulich behandelt und nicht an Dritte weitergegeben. Sie können der Verwendung Ihrer Daten jederzeit widersprechen. Das Datenhandling bei Sack Fachmedien erklären wir Ihnen in unserer Datenschutzerklärung.