Numerical Radiative Transfer
Numerical Radiative Transfer
- Authorized Dealer
- 30-Day Returns on Eligible Items
- Secure & Encrypted Checkout
Details
"Numerical Radiative Transfer" by Wolfgang Kalkofen is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.
First published in 1988, this book is a manual of methods for solving problems in radiative transfer. Several of the methods, on operator perturbation as well as on polarised radiative transfer, appeared for the first time in this volume, and the sections dealing with these topics each include introductory articles. The methods described are principally directed at astrophysical plasmas, but the methods are easily adaptable to applications involving other media where self-absorption of the radiation is important. The book is primarily intended for graduate students and research workers in the field of radiative transfer.
Shipping + Returns
Shipping
Shipping costs and estimated fulfillment times are displayed on the product page or at checkout. Some items ship directly from our trusted suppliers, and processing times may vary by product.
Returns
Returns are accepted on eligible products within 30 days of delivery, subject to our return policy. Please review our full return policy for eligibility, exclusions, and instructions.
If you have questions about shipping or returns, please contact Snowflake Skies before placing your order.
"Numerical Radiative Transfer" by Wolfgang Kalkofen is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.
Topic: Deep Sky & Solar System
Author: Wolfgang Kalkofen
Who this is for:
- Teachers and classroom instructors
- Students building subject mastery
- Readers looking for practical learning support
Why this book matters: It stands out as a practical math resource that helps explain concepts, strengthen problem-solving, and support classroom or independent learning.
First published in 1988, this book is a manual of methods for solving problems in radiative transfer. Several of the methods, on operator perturbation as well as on polarised radiative transfer, appeared for the first time in this volume, and the sections dealing with these topics each include introductory articles. The methods described are principally directed at astrophysical plasmas, but the methods are easily adaptable to applications involving other media where self-absorption of the radiation is important. The book is primarily intended for graduate students and research workers in the field of radiative transfer.
| Author | Wolfgang Kalkofen |
| Publisher | Cambridge University Press |
| Published | 1988-01-07 |
| ISBN-13 | 9780521341004 |
| Binding | Hardcover |
| Pages | 382 |
| Language | English |
| Subjects | Science |
| Topic | Deep Sky & Solar System |
Format: Hardcover
Length: 382 pages
Language: English
Shop by collection
Books