Get Free Shipping on orders over $79
Cosmic Ray Interactions, Propagation, and Acceleration in Space Plasmas - Lev Dorman

Cosmic Ray Interactions, Propagation, and Acceleration in Space Plasmas

By: Lev Dorman

eText | 2 September 2006

At a Glance

eText


$319.00

or 4 interest-free payments of $79.75 with

 or 

Instant online reading in your Booktopia eTextbook Library *

Why choose an eTextbook?

Instant Access *

Purchase and read your book immediately

Read Aloud

Listen and follow along as Bookshelf reads to you

Study Tools

Built-in study tools like highlights and more

* eTextbooks are not downloadable to your eReader or an app and can be accessed via web browsers only. You must be connected to the internet and have no technical issues with your device or browser that could prevent the eTextbook from operating.
The book consists of four Chapters. Chapter 1 shortly describes main properties of space plasmas and primary CR, different types of CR interactions with space plasmas components (matter, photons, and frozen in magnetic fields). Chapter 2 considers the problem of CR propagation in space plasmas described by the kinetic equation and different types of diffusion approximations (diffusion in momentum space and in pitch-angle space, anisotropic diffusion, anomaly CR diffusion and compound diffusion, the influence of magnetic clouds on CR propagation, non-diffusive CR particle pulse transport). Chapter 3 is devoted to CR non-linear effects in space plasmas caused by CR pressure and CR kinetic stream instabilities with the generation of Alfv??n turbulence (these effects are important in galaxies, in the Heliosphere, in CR and gamma-ray sources and in the processes of CR acceleration). In Chapter 4 different processes of CR acceleration in space plasmas are considered: the development of the Fermi statistical mechanism, acceleration in the turbulent plasma, Alfv??n mechanism of magnetic pumping, induction mechanisms, acceleration during magnetic collapse and compression, cumulative acceleration mechanism near the zero lines of a magnetic field, acceleration in shear flows, shock-wave diffusion (regular) acceleration. The book ends with a list providing more than 1,300 full references, a discussion on future developments and unsolved problems, as well as Object and Author indexes. This book will be useful for experts and students in CR research, Astrophysics and Geophysics, and in Space Physics.
on
Desktop
Tablet
Mobile

Other Editions and Formats

Paperback

Published: 23rd August 2016

More in Astronomy, Space & Time

Coming of Age in the Milky Way - Timothy Ferris

eBOOK

RRP $33.99

$27.99

18%
OFF
Mars : A Survival Guide - Guy Murphy

eBOOK

The Ant and the Ferrari - Kerry Spackman

eBOOK

The Solar System : Kosmos - William Sheehan

eBOOK

RRP $67.57

$57.99

14%
OFF