Aeronomy of Mars
Haider, S. A.
- 出版商: Springer
- 出版日期: 2024-08-19
- 售價: $5,950
- 貴賓價: 9.5 折 $5,653
- 語言: 英文
- 頁數: 248
- 裝訂: Quality Paper - also called trade paper
- ISBN: 9819931401
- ISBN-13: 9789819931408
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相關主題
商品描述
"Mangalyaan was launched on November 5, 2013, to Mars by Indian Space Research Organization (ISRO). On October 2, 2022, ISRO declared that Mangalyaan had lost communications with Earth. Mars Color Camera (MCC) on-board Mangalyaan has taken thousands pictures of Mars. A full disk of Mars image observed by Viking is shown on the cover page of this book. Mars is covered by the dust as observed by Mangalyaan (from Arya et al., 2015). This book presents the atmospheric and ionospheric results obtained from all missions to Mars. It also covers various atmospheric and ionospheric models of Mars. Broadly speaking, the planet's atmosphere can be divided into two regions: lower and upper. These two regions can be coupled due to the propagation of energy from the lower to the upper atmosphere. The first-ever book on the aeronomy of Mars, this work is intended to help students and researchers familiarize themselves with the field of aeronomy. In addition, it helps planetary probe designers, engineers, and other users in the scientific community, e.g., planetary geologists and geophysicists".
商品描述(中文翻譯)
《Mangalyaan》於2013年11月5日由印度空間研究組織（ISRO）發射至火星。ISRO在2022年10月2日宣佈《Mangalyaan》已與地球失去聯繫。搭載於《Mangalyaan》的火星彩色相機（MCC）拍攝了數千張火星的圖片。本書封面展示了由維京號觀測到的火星全盤影像。根據《Mangalyaan》的觀測，火星表面覆蓋著塵埃（來自Arya等，2015）。本書呈現了所有火星任務所獲得的大氣和電離層結果，並涵蓋了火星的各種大氣和電離層模型。廣義而言，火星的大氣可分為兩個區域：下層和上層。由於能量從下層大氣向上層大氣的傳播，這兩個區域可能會相互耦合。這是第一本關於火星氣象學的書籍，旨在幫助學生和研究人員熟悉氣象學領域。此外，它還幫助行星探測器設計師、工程師及其他科學社群的使用者，例如行星地質學家和地球物理學家。
作者簡介
Prof. S.A. Haider has worked at the Physical Research Laboratory, Ahmedabad, India, for 25 years on the modeling studies of Martian atmosphere. During this period, he has published over eighty scientific papers in peer-reviewed journals, several review papers and book chapters. He has also edited a book on Modeling of Planetary Atmospheres, published by Macmillan. He is a recipient of several prestigious fellowships like the Russian Academy of Sciences Fellowship (Russia), JSPS Fellowship (Japan) and FAPESP Fellowship (Brazil). Based on his innovative work, he was elected fellow of all three academy of sciences in India and has also been elected president of planetary sciences 2012-2014 by Asia Oceania Geosciences Society.
作者簡介(中文翻譯)
S.A. Haider 教授在印度艾哈邁達巴德的物理研究實驗室工作了 25 年，專注於火星大氣的建模研究。在此期間，他在同行評審的期刊上發表了超過八十篇科學論文，以及幾篇綜述論文和書籍章節。他還編輯了一本由麥克米倫出版的《行星大氣建模》一書。他獲得了多項著名的獎學金，如俄羅斯科學院獎學金（俄羅斯）、JSPS 獎學金（日本）和 FAPESP 獎學金（巴西）。基於他的創新工作，他被選為印度三個科學院的院士，並於 2012 至 2014 年被亞洲大洋洲地球科學學會選為行星科學會長。
