Cantitate/Preț
Produs
Total produse
Vezi coșul
Mercury de A. Balogh

Mercury: Space Sciences Series of ISSI, cartea 26

Editat de A. Balogh, Leonid Ksanfomality Cuvânt înainte de L. Ksanfomality Editat de Rudolf Von Steiger Cuvânt înainte de R.v. Steiger
en Limba Engleză Hardback – 16 apr 2008
Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book reviews the progress made in Mercury studies since the flybys by Mariner 10 in 1974-75, based on the continued research using the Mariner 10 archive, on observations from Earth, and on increasingly realistic models of its interior evolution.
Citește tot Restrânge

Toate formatele și edițiile

Toate formatele și edițiile Preț Express
Paperback (1) 93340 lei  6-8 săpt.
  Springer – 25 noi 2010 93340 lei  6-8 săpt.
Hardback (1) 94364 lei  6-8 săpt.
  Springer – 16 apr 2008 94364 lei  6-8 săpt.

Din seria Space Sciences Series of ISSI

Preț: 94364 lei

Preț vechi: 115078 lei
-18% Nou

Puncte Express: 1415
Preț estimativ în valută:
18059€ • 18759$ • 15001£

Carte tipărită la comandă

Livrare economică 03-17 februarie 25

 Adaugă în coș

Wish list
Gift list
Am citit!
Adaugă în listă
Preluare comenzi: 021 569.72.76

Specificații

ISBN-13: 9780387775388
ISBN-10: 0387775382
Pagini: 468
Ilustrații: IV, 468 p. 168 illus., 72 illus. in color.
Dimensiuni: 160 x 240 x 23 mm
Greutate: 0.95 kg
Ediția:2008
Editura: Springer
Colecția Springer
Seria Space Sciences Series of ISSI

Locul publicării:New York, NY, United States

Public țintă

Research

Cuprins

The Origin of Mercury.- Mercury’s Interior Structure, Rotation, and Tides.- Interior Evolution of Mercury.- The Origin of Mercury’s Internal Magnetic Field.- The Surface of Mercury as Seen by Mariner 10.- Radar Imaging of Mercury.- Earth-Based Visible and Near-IR Imaging of Mercury.- Mercury’s Surface Composition and Character as Measured by Ground-Based Observations.- Processes that Promote and Deplete the Exosphere of Mercury.- Electromagnetic Induction Effects and Dynamo Action in the Hermean System.- Hermean Magnetosphere-Solar Wind Interaction.- Magnetosphere–Exosphere–Surface Coupling at Mercury.- Plasma Waves in the Hermean Magnetosphere.- Particle Acceleration in Mercury’s Magnetosphere.- Missions to Mercury.

Textul de pe ultima copertă

Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book reviews the progress made in Mercury studies since the flybys by Mariner 10 in 1974-75, based on the continued research using the Mariner 10 archive, on observations from Earth, and on increasingly realistic models of its interior evolution.

Caracteristici

Only book on Mercury which balances the wide range of Earth-based observations, made under difficult conditions, with the only available space-based data from Mariner 10 Contains an in-depth review of the most up-to-date research concerning Mercury’s interior, its evolution and the origin of its unexpected magnetic field Mercury’s environment, from its surface to its magnetosphere, is reviewed in detail, based on a comparative reinterpretation of phenomena and processes in the Earth’s magnetosphere