Aschwanden Markus (112 results)

Condition: Very Good. 236 pp., hardcover, hand stamp to the front free endpaper, else very good. - If you are reading this, this item is actually (physically) in our stock and ready for shipment once ordered. We are not bookjackers. Buyer is responsible for any additional duties, taxes, or fees required by recipient's country.…

Hardcover. Condition: Fine. "This book presents a synthesis of what we learned about particle acceleration and kinematics from recent solar flare observations with the Yokkoh, SOHO, TRACE, CGRO spacecraft and radio instruments over the last decade." Reprinted from Space Science Reviews, Volume 101, Nos. 1-2, 2002. Octavo: 227 p. with 129 figures (some color) and 13 tables. Original glossy boards; issued without a dust jacket. A fine copy. …

Hardcover. Octavo, xiv, 416 pages. In Very Good condition. Spine is black with orange and white print. Boards in glossy illustrated paper. Illustrated: b&w drawings, graphs, color photographs. NOTE: Shelved in Netdesk Column W. 1404343. FP New Rockville Stock.

Hardcover. Condition: Like New. First Edition. A firm and square hardback with strong joints, just showing a few very minor cosmetic rubs. Hence a non-text page has a small 'damaged' stamp. Despite such this book is actually in nearly new condition and appears unread. Thus the contents are crisp, fresh and tight; no pen-marks. Now offered for sale at a very sensible price. …

Condition: New. In.

Paperback. Condition: Good condition. good condition,fast ship.

paperback. Condition: New. In shrink wrap. Looks like an interesting title.

Condition: New. A brand new book in pristine condition. Showing zero signs of shelf wear, creases, or damage.

Condition: New. In.

Condition: New. Presents a synthesis of what we learned about particle acceleration and kinematics from solar flare observations with the Yohkoh, SoHO, TRACE, CGRO spacecraft and radio instruments over the last decade. This book is intended for graduate students and researchers in the field of solar physics, astrophysics, and magnetospheric physics. Num Pages: 228 pages, biography. BIC Classification: PGS. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 15. Weight in Grams: 563. . 2002. Reprinted from SPACE SCIENCE REVIEWS, 101:1-2, 200. hardcover. . . . .…

Condition: New.

Gebunden. Condition: New.

Condition: New. pp. viii + 227.

Condition: New. pp. 236.

Condition: As New. Unread book in perfect condition.

Condition: New.

Hardcover. Condition: Brand New. 236 pages. 9.50x6.50x0.50 inches. In Stock.

Condition: New. Presents a synthesis of what we learned about particle acceleration and kinematics from solar flare observations with the Yohkoh, SoHO, TRACE, CGRO spacecraft and radio instruments over the last decade. This book is intended for graduate students and researchers in the field of solar physics, astrophysics, and magnetospheric physics. Num Pages: 228 pages, biography. BIC Classification: PGS. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 15. Weight in Grams: 563. . 2002. Reprinted from SPACE SCIENCE REVIEWS, 101:1-2, 200. hardcover. . . . . Books ship from the US and Ireland.…

Condition: New. In.

Paperback. Condition: New. 1st ed. 2005. 2nd printing 2006. Solar science has evolved rapidly over the past decade as the results of a new generation of solar space missions have become available. This book provides a thorough introduction to the subject of solar physics, based on those observations. The author introduces the solar corona, which has a temperature of several million degrees, and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation, fundamental processes in all stars, are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, with their potential effects on the Earth. The author gathers observations made at many wavelengths from hard X-rays, soft X-rays, extreme UV and radio wavelengths. This paperback study edition includes 50 pages of problems and solutions which will much enhance the value of the book to students.…

Condition: New.

Condition: New.

Condition: New. In.

Condition: New.

Condition: New.

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Over the last decade we entered a new exploration phase of solar flare physics, equipped with powerful spacecraft such as Yohkoh, SoHO, and TRACE that pro vide us detail-rich and high-resolution images of solar flares in soft X-rays, hard X -rays, and extreme-ultraviolet wavelengths. Moreover, the large-area and high sensitivity detectors on the Compton GRO spacecraft recorded an unprecedented number of high-energy photons from solar flares that surpasses all detected high energy sources taken together from the rest of the universe, for which CGRO was mainly designed to explore. However, morphological descriptions of these beau tiful pictures and statistical catalogs of these huge archives of solar data would not convey us much understanding of the underlying physics, if we would not set out to quantify physical parameters from these data and would not subject these measurements to theoretical models. Historically, there has always been an unsatisfactory gap between traditional astronomy that dutifully describes the mor phology of observations, and the newer approach of astrophysics, which starts with physical concepts from first principles and analyzes astronomical data with the goal to confirm or disprove theoretical models. In this review we attempt to bridge this yawning gap and aim to present the recent developments in solar flare high-energy physics from a physical point of view, structuring the observations and analysis results according to physical processes, such as particle acceleration, propagation, energy loss, kinematics, and radiation signatures.…

Condition: As New. Unread book in perfect condition.

Paperback. Condition: Brand New. reprint edition. 235 pages. 8.90x6.00x0.60 inches. In Stock.

Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Over the last decade we entered a new exploration phase of solar flare physics, equipped with powerful spacecraft such as Yohkoh, SoHO, and TRACE that pro vide us detail-rich and high-resolution images of solar flares in soft X-rays, hard X -rays, and extreme-ultraviolet wavelengths. Moreover, the large-area and high sensitivity detectors on the Compton GRO spacecraft recorded an unprecedented number of high-energy photons from solar flares that surpasses all detected high energy sources taken together from the rest of the universe, for which CGRO was mainly designed to explore. However, morphological descriptions of these beau tiful pictures and statistical catalogs of these huge archives of solar data would not convey us much understanding of the underlying physics, if we would not set out to quantify physical parameters from these data and would not subject these measurements to theoretical models. Historically, there has always been an unsatisfactory gap between traditional astronomy that dutifully describes the mor phology of observations, and the newer approach of astrophysics, which starts with physical concepts from first principles and analyzes astronomical data with the goal to confirm or disprove theoretical models. In this review we attempt to bridge this yawning gap and aim to present the recent developments in solar flare high-energy physics from a physical point of view, structuring the observations and analysis results according to physical processes, such as particle acceleration, propagation, energy loss, kinematics, and radiation signatures.…

Condition: New.