Skip to main content Accessibility help
×
Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-08T00:18:13.737Z Has data issue: false hasContentIssue false

1 - Introduction

Published online by Cambridge University Press:  04 August 2010

Get access

Summary

‘Faced with something unusual our thought should not be “What next?” but “Why?”. By answering the second of these questions we can answer the first. And this, in brief, is the scientific method.’

Roger Scruton (c. 1990)

By definition, all exothermal reactors, including any fusion reactor one may envisage (tokamak, stellarator, etc.), produce both energy and spent reactants, or ash. In order for the reactor to operate in steady-state, (i) fresh fuel must be added at the rate at which it is consumed, (ii) this fuel must be heated, ideally by the reactions themselves, (iii) fuel must be confined, by whatever means are available, for sufficiently long to allow the exothermic processes to continue, (iv) the energy and ash must be removed from the system at the rate at which they are created, (v) the impurities released from the reactor walls must likewise be removed at the rate at which they are produced, and (vi) the reactor itself, primarily its walls, must not be damaged by all the exhaust processes. Translating the above to a D–T burning tokamak, conditions (i)–(iii) may be labelled loosely as the ignition criteria, and conditions (iv)–(vi) as the exhaust criteria. Taken together they constitute the criteria of mutual compatibility between the burning plasma and first wall materials/components.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 2009

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure [email protected] 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.

  • Introduction
  • Wojciech Fundamenski
  • Book: Power Exhaust in Fusion Plasmas
  • Online publication: 04 August 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511770609.002
Available formats
×

Save book 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 Dropbox.

  • Introduction
  • Wojciech Fundamenski
  • Book: Power Exhaust in Fusion Plasmas
  • Online publication: 04 August 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511770609.002
Available formats
×

Save book to Google Drive

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.

  • Introduction
  • Wojciech Fundamenski
  • Book: Power Exhaust in Fusion Plasmas
  • Online publication: 04 August 2010
  • Chapter DOI: https://doi.org/10.1017/CBO9780511770609.002
Available formats
×