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Pamphlet. Zustand: Very Good. Vol 76, No 25, pp. 6159-6171, Illus, Extracted from orig vol, thus begins with title page, trimmed & stapled pamphlet, else VG.

Gr.-8°, original hardcover. 1. ed. XVI, 554 p. Shelfmark on spine, Stamp on prelimininary page, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Hardcover. Zustand: Fair. The item might be beaten up but readable. May contain markings or highlighting, as well as stains, bent corners, or any other major defect, but the text is not obscured in any way.

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Zustand: Brand New. New. US edition. Expediting shipping for all USA and Europe orders excluding PO Box. Excellent Customer Service.

Zustand: Brand New. New. US edition. Expediting shipping for all USA and Europe orders excluding PO Box. Excellent Customer Service.

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Zustand: New. pp. 360.

Zustand: New. pp. 360.

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Zustand: New. Brand new! Please provide a physical shipping address.

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Zustand: New. Editor(s): Huba, J. D.; Schunk, R.W.; Khazanov, G. V. Series: Geophysical Monograph Series. Num Pages: 360 pages, illustrations. BIC Classification: PHVG; RBP. Category: (P) Professional & Vocational. Dimension: 277 x 220 x 28. Weight in Grams: 1278. . 2014. 1st Edition. Hardcover. . . . . …

Hardcover. Zustand: Brand New. 1st edition. 360 pages. 10.75x8.75x1.00 inches. In Stock.

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HRD. Zustand: New. New Book. Shipped from UK. Established seller since 2000.

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Hardcover. Zustand: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

Zustand: New. Editor(s): Huba, J. D.; Schunk, R.W.; Khazanov, G. V. Series: Geophysical Monograph Series. Num Pages: 360 pages, illustrations. BIC Classification: PHVG; RBP. Category: (P) Professional & Vocational. Dimension: 277 x 220 x 28. Weight in Grams: 1278. . 2014. 1st Edition. Hardcover. . . . . Books ship from the US and Ireland. …

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Hardcover. Zustand: New. Brand new book, sourced directly from publisher. Dispatch time is 6-7 days from our warehouse. Book will be sent in robust, secure packaging to ensure it reaches you securely.

Hardback. Zustand: New. Over a half century of exploration of the Earth's space environment, it has become evident that the interaction between the ionosphere and the magnetosphere plays a dominant role in the evolution and dynamics of magnetospheric plasmas and fields. Interestingly, it was recently discovered that this same interaction is of fundamental importance at other planets and moons throughout the solar system. Based on papers presented at an interdisciplinary AGU Chapman Conference at Yosemite National Park in February 2014, this volume provides an intellectual and visual journey through our exploration and discovery of the paradigm-changing role that the ionosphere plays in determining the filling and dynamics of Earth and planetary environments. The 2014 Chapman conference marks the 40th anniversary of the initial magnetosphere-ionosphere coupling conference at Yosemite in 1974, and thus gives a four decade perspective of the progress of space science research in understanding these fundamental coupling processes. Digital video links to an online archive containing both the 1974 and 2014 meetings are presented throughout this volume for use as an historical resource by the international heliophysics and planetary science communities. Topics covered in this volume include: Ionosphere as a source of magnetospheric plasmaEffects of the low energy ionospheric plasma on the stability and creation of the more energetic plasmasThe unified global modeling of the ionosphere and magnetosphere at the Earth and other planetsNew knowledge of these coupled interactions for heliophysicists and planetary scientists, with a cross-disciplinary approach involving advanced measurement and modeling techniques Magnetosphere-Ionosphere Coupling in the Solar System is a valuable resource for researchers in the fields of space and planetary science, atmospheric science, space physics, astronomy, and geophysics.Read an interview with the editors to find out more:https://eos.org/editors-vox/filling-earths-space-environment-from-the-sun-or-the-earth.…

Hardcover. Zustand: new. Hardcover. Over a half century of exploration of the Earths space environment, it has become evident that the interaction between the ionosphere and the magnetosphere plays a dominant role in the evolution and dynamics of magnetospheric plasmas and fields. Interestingly, it was recently discovered that this same interaction is of fundamental importance at other planets and moons throughout the solar system. Based on papers presented at an interdisciplinary AGU Chapman Conference at Yosemite National Park in February 2014, this volume provides an intellectual and visual journey through our exploration and discovery of the paradigm-changing role that the ionosphere plays in determining the filling and dynamics of Earth and planetary environments. The 2014 Chapman conference marks the 40th anniversary of the initial magnetosphere-ionosphere coupling conference at Yosemite in 1974, and thus gives a four decade perspective of the progress of space science research in understanding these fundamental coupling processes. Digital video links to an online archive containing both the 1974 and 2014 meetings are presented throughout this volume for use as an historical resource by the international heliophysics and planetary science communities. Topics covered in this volume include: Ionosphere as a source of magnetospheric plasmaEffects of the low energy ionospheric plasma on the stability and creation of the more energetic plasmasThe unified global modeling of the ionosphere and magnetosphere at the Earth and other planetsNew knowledge of these coupled interactions for heliophysicists and planetary scientists, with a cross-disciplinary approach involving advanced measurement and modeling techniques Magnetosphere-Ionosphere Coupling in the Solar System is a valuable resource for researchers in the fields of space and planetary science, atmospheric science, space physics, astronomy, and geophysics.Read an interview with the editors to find out more: Over a half century of exploration of the Earth s space environment, it has become evident that the interaction between the ionosphere and the magnetosphere plays a dominant role in the evolution and dynamics of magnetospheric plasmas and fields. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.…

Zustand: New. pp. 326.

Zustand: New. Over a half century of exploration of the Earth s space environment, it has become evident that the interaction between the ionosphere and the magnetosphere plays a dominant role in the evolution and dynamics of magnetospheric plasmas and fields. Editor(s): Chappell, Charles R.; Schunk, Robert W.; Banks, Peter M.; Thorne, Richard M.; Burch, James L. Series: Geophysical Monograph Series. Num Pages: 414 pages. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational. Dimension: 287 x 220 x 25. Weight in Grams: 1382. . 2016. 1st Edition. Hardcover. . . . . …

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