logo

EbookBell.com

Most ebook files are in PDF format, so you can easily read them using various software such as Foxit Reader or directly on the Google Chrome browser.
Some ebook files are released by publishers in other formats such as .awz, .mobi, .epub, .fb2, etc. You may need to install specific software to read these formats on mobile/PC, such as Calibre.

Please read the tutorial at this link:  https://ebookbell.com/faq 


We offer FREE conversion to the popular formats you request; however, this may take some time. Therefore, right after payment, please email us, and we will try to provide the service as quickly as possible.


For some exceptional file formats or broken links (if any), please refrain from opening any disputes. Instead, email us first, and we will try to assist within a maximum of 6 hours.

EbookBell Team

Dawndusk Asymmetries In Planetary Plasma Environments Forsyth

  • SKU: BELL-6839444
Dawndusk Asymmetries In Planetary Plasma Environments Forsyth
$ 31.00 $ 45.00 (-31%)

4.0

26 reviews

Dawndusk Asymmetries In Planetary Plasma Environments Forsyth instant download after payment.

Publisher: American Geophysical Union
File Extension: PDF
File size: 26.06 MB
Pages: 360
Author: Forsyth, Colin; Haaland, Stein; Runov, Andrei
ISBN: 9781119216322, 9781119216346, 9781119216353, 9781119216513, 111921632X, 1119216346, 1119216354, 1119216516
Language: English
Year: 2017

Product desciption

Dawndusk Asymmetries In Planetary Plasma Environments Forsyth by Forsyth, Colin; Haaland, Stein; Runov, Andrei 9781119216322, 9781119216346, 9781119216353, 9781119216513, 111921632X, 1119216346, 1119216354, 1119216516 instant download after payment.

"Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other. For example, recent observations indicate that Earth's magnetopause is thicker at dawn than at dusk. Likewise, auroral breakups at Earth are more likely to occur in the pre-midnight than post-midnight sectors. Increasing availability of remotely sensed and in situ measurements of planetary ionospheres, magnetospheres and their interfaces to the solar wind have revealed significant and persistent dawn-dusk asymmetries. As yet there is no consensus regarding the source of many of these asymmetries, nor the physical mechanisms by which they are produced and maintained. Volume highlights include: A comprehensive and updated overview of current knowledge about dawn-dusk asymmetries in the plasma environments of planets in our solar system and the mechanisms behind them; Valuable contributions from internationally recognized experts, covering both observations, simulations and theories discussing all important aspects of dawn-dusk asymmetries; Space weather effects are caused by processes in space, mainly the magnetotail, and can be highly localized on ground. Knowing where the source, i.e., where dawn-dusk location is will allow for a better prediction of where the effects on ground will be most pronounced" -- Provided by publisher.
Abstract: Dawn-Dusk Asymmetries in Planetary Plasma Environments Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other.

Related Products