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Discover cutting edge theory and applications of modern remote sensing in geology, oceanography, atmospheric science, ionospheric studies, and more    The thoroughly revised third edition of the  Introduction to the Physics and Techniques of Remote Sensing  delivers a comprehensive update to the authoritative textbook, offering readers new sections on radar interferometry, radar stereo, and planetary radar. It explores new techniques in imaging spectroscopy and large optics used in Earth orbiting, planetary, and astrophysics missions. It also describes remote sensing instruments on, as well as data acquired with, the most recent Earth and space missions.  Readers will benefit from the brand new and up-to-date concept examples and full-color photography, 50% of which is new to the series. You’ll learn about the basic physics of wave/matter interactions, techniques of remote sensing across the electromagnetic spectrum (from ultraviolet to microwave), and the concepts behind the remote sensing techniques used today and those planned for the future.  The book also discusses the applications of remote sensing for a wide variety of earth and planetary atmosphere and surface sciences, like geology, oceanography, resource observation, atmospheric sciences, and ionospheric studies. This new edition also incorporates:  A fulsome introduction to the nature and properties of electromagnetic waves An exploration of sensing solid surfaces in the visible and near infrared spectrums, as well as thermal infrared, microwave, and radio frequencies A treatment of ocean surface sensing, including ocean surface imaging and the mapping of ocean topography A discussion of the basic principles of atmospheric sensing and radiative transfer, including the radiative transfer equation Perfect for senior undergraduate and graduate students in the field of remote sensing instrument development, data analysis, and data utilization,  Introduction to the Physics and Techniques of Remote Sensing  will also earn a place in the libraries of students, faculty, researchers, engineers, and practitioners in fields like aerospace, electrical engineering, and astronomy.

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Build your knowledge of SAR/ISAR imaging with this comprehensive and insightful resource   The newly revised Second Edition of  Inverse Synthetic Aperture Radar Imaging with MATLAB Algorithms  covers in greater detail the fundamental and advanced topics necessary for a complete understanding of inverse synthetic aperture radar (ISAR) imaging and its concepts. Distinguished author and academician, Caner Özdemir, describes the practical aspects of ISAR imaging and presents illustrative examples of the radar signal processing algorithms used for ISAR imaging. The topics in each chapter are supplemented with MATLAB codes to assist readers in better understanding each of the principles discussed within the book.  This new edition incudes discussions of the most up-to-date topics to arise in the field of ISAR imaging and ISAR hardware design. The book provides a comprehensive analysis of advanced techniques like Fourier-based radar imaging algorithms, and motion compensation techniques along with radar fundamentals for readers new to the subject.  The author covers a wide variety of topics, including:  Radar fundamentals, including concepts like radar cross section, maximum detectable range, frequency modulated continuous wave, and doppler frequency and pulsed radar The theoretical and practical aspects of signal processing algorithms used in ISAR imaging The numeric implementation of all necessary algorithms in MATLAB ISAR hardware, emerging topics on SAR/ISAR focusing algorithms such as bistatic ISAR imaging, polarimetric ISAR imaging, and near-field ISAR imaging, Applications of SAR/ISAR imaging techniques to other radar imaging problems such as thru-the-wall radar imaging and ground-penetrating radar imaging Perfect for graduate students in the fields of electrical and electronics engineering, electromagnetism, imaging radar, and physics,  Inverse Synthetic Aperture Radar Imaging With MATLAB Algorithms  also belongs on the bookshelves of practicing researchers in the related areas looking for a useful resource to assist them in their day-to-day professional work.

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«Publish» – журнал о современных издательских и полиграфических технологиях, от графического дизайна и допечатных процессов до послепечати. В номере: Тема номера: К безлюдному производству Популярная автоматизация Универсальный УФ-инструмент для бизнеса с человеческим лицом От цифровой печати к резке по цифрам Лучшая картонная упаковка Тайный покупатель: визитки высокой печатью Обзоры. Riso ComColor FT5230 Детали. Xerox Adaptive CMYK Plus для Versant и многое другое

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"Ich erkläre dir mein Zuhause” widmet sich einem Thema, welches das unmittelbare Lebensumfeld der Kinder betrifft. Sie wohnen in einem Haus oder einer Wohnung; zusammen mit Mama und/oder Papa, mit Geschwistern und vielleicht sogar Tieren. Daraus könnten sich folgende Fragen ergeben: Wohnen denn alle Menschen gleich? Sehen alle Häuser auf der Welt genau gleich aus oder gibt es da Unterschiede? Wie entsteht eigentlich so ein Haus? Wie kommt denn das Wasser in den Wasserhahn oder der Strom in die Steckdose? Warum muss ich im Winter nicht frieren? Usw.
Kindliche Fragen, die durch dieses Projekt gemeinsam mit den Kindern bearbeitet werden können.
"Ich erkläre dir mein Zuhause” bietet eine Auswahl an Möglichkeiten, Sachwissen zu vermitteln, Sprache zu fördern, Sozialkompetenz zu erweitern, Denkanstöße zu geben, Feinmotorik zu trainieren, Freude an der Bewegung zu fördern, uvm.
Dieses Projekt eignet sich für Kinder von 2-6 Jahren. Empfohlener Zeitraum: 4-6 Wochen.

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Das Überbringen einer schlechten Nachricht stellt für viele Ärzte eine belastende Situation dar. Mit dieser Fibel erhalten sie ein Grundgerüst das hilft, ein solches Gespräch gut strukturiert zu führen. Zahlreiche praktische Tipps und Ideen zu Formulierungen bieten eine Unterstützung, die eigenen kommunikativen Fähigkeiten zu reflektieren und ggf. auszubauen.

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Galaxies are vast ensembles of stars, gas and dust, embedded in dark matter halos. They are the basic building blocks of the Universe, gathered in groups, clusters and super-clusters. They exist in many forms, either as spheroids or disks. Classifications, such as the Hubble sequence (based on mass concentration and gas fraction) and the colormagnitude diagram (which separates a blue cloud from a red sequence) help to understand their formation and evolution. Galaxies spend a large part of their lives in the blue cloud, forming stars as spiral or dwarf galaxies. Then, via a mechanism that is still unclear, they stop forming stars and quietly end in the red sequence, as spheroids. This transformation may be due to galaxy interactions, or because of the feedback of active nuclei, through the energy released by their central super-massive black holes. These mechanisms could explain the history of cosmic star formation, the rate of which was far greater in the first half of the Universe's life. <p><i>Galaxies</i> delves into all of these surrounding subjects in six chapters written by dedicated, specialist astronomers and researchers in the field, from their numerical simulations to their evolutions.

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