Published online by Cambridge University Press: 26 October 2017
In this first part, we get oriented to the general subject matter of the book and the style of approach. The orientation in Chapter 1 includes a discussion of broader aspects, such as mathematical modeling, continuum mechanics, the role of energy in the universe and the apparent need of astronomical bodies to cool as rapidly as possible. Central to our study is the concept of a continuous body, as discussed in § 1.2.
The second chapter provides a bit more introductory detail, including the reference coordinate system, a definition of waves and flows, a summary of the scope of the book and brief introductions to a number of related issues.
To save this book to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
Find out more about the Kindle Personal Document Service.
To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.
To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.