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Prestack depth migration and velocity model building, 


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Название:  Prestack depth migration and velocity model building
Перевод названия: Миграция глубин, предшествующая замерам, и построение скоростной модели
ISBN: 9781560801474
Издательство: Mare Nostrum (Eurospan)
Классификация:

ISBN-10: 1560801476
Обложка/Формат: Paperback
Страницы: 880
Вес: 1.99 кг.
Дата издания: 30.12.2008
Серия: Geophysics reprints
Язык: English
Издание: 4 revised edition
Иллюстрации: Includes a cd rom
Размер: 279 x 216
Читательская аудитория: General (us: trade)
Подзаголовок: Bound with: orthographe pratique des langues africaines; the distribution of the semitic and cushitic languages of africa; the distribution of the nilotic and nilo-hamitic languages of africa; and linguistic analyses
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Поставляется из: Англии
Описание: The traditional compartmentalized approach has been superseded by a multidisciplinary collaborative workflow to build iteratively a subsurface velocity model suitable for detailed and quantitative imaging. Works that have had the most practical industrial application are emphasized, with a bias is away from R & D and toward industrial practice.

Sedimentation Velocity Analytical U

Автор: Schuck
Название: Sedimentation Velocity Analytical U
ISBN: 1138035289 ISBN-13(EAN): 9781138035287
Издательство: Taylor&Francis
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Цена: 148010.00 T
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Описание: Building on the previous two volumes by Dr. Schuck, this new volume is devoted to the theory and practical data analysis of dynamically coupled sedimentation processes. It will be an invaluable resource for students interested in the application of analytical ultracentrifugation in the study of interacting systems.

Radial-velocity Searches for Planets Around Active Stars

Автор: Haywood
Название: Radial-velocity Searches for Planets Around Active Stars
ISBN: 3319412728 ISBN-13(EAN): 9783319412726
Издательство: Springer
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Цена: 95770.00 T
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Описание: This thesis develops new and powerful methods for identifying planetary signals in the presence of “noise” generated by stellar activity, and explores the physical origin of stellar intrinsic variability, using unique observations of the Sun seen as a star. In particular, it establishes that the intrinsic stellar radial-velocity variations mainly arise from suppression of photospheric convection by magnetic fields. With the advent of powerful telescopes and instruments we are now on the verge of discovering real Earth twins in orbit around other stars. The intrinsic variability of the host stars themselves, however, currently remains the main obstacle to determining the masses of such small planets. The methods developed here combine Gaussian-process regression for modeling the correlated signals arising from evolving active regions on a rotating star, and Bayesian model selection methods for distinguishing genuine planetary signals from false positives produced by stellar magnetic activity.

The findings of this thesis represent a significant step towards determining the masses of potentially habitable planets orbiting Sun-like stars.

Hyper-Velocity Impacts on Rubble Pile Asteroids

Автор: Jakob Deller
Название: Hyper-Velocity Impacts on Rubble Pile Asteroids
ISBN: 3319479849 ISBN-13(EAN): 9783319479842
Издательство: Springer
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Цена: 130430.00 T
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Описание:

The thesis presents a tool to create rubble pile asteroid simulants for use in numerical impact experiments, and provides evidence that the asteroid disruption threshold and the resultant fragment size distribution are sensitive to the distribution of internal voids. This thesis represents an important step towards a deeper understanding of fragmentation processes in the asteroid belt, and provides a tool to infer the interior structure of rubble pile asteroids.
Most small asteroids are 'rubble piles' – re-accumulated fragments of debris from earlier disruptive collisions. The study of fragmentation processes for rubble pile asteroids plays an essential part in understanding their collisional evolution. An important unanswered question is “what is the distribution of void space inside rubble pile asteroids?” As a result from this thesis, numerical impact experiments can now be used to link surface features to the internal structure and therefore help to answer this question.
Applying this model to asteroid ?teins, which was imaged from close range by the Rosetta spacecraft, a large hill-like structure is shown to be most likely primordial, while a catena of pits can be interpreted as evidence for the existence of fracturing of pre-existing internal voids.


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