The PUILS series delivers up-to-date reviews of progress in Ultrafast Intense Laser Science, a newly emerging interdisciplinary research field spanning atomic and molecular physics, molecular science and optical science which has been stimulated by the recent developments in ultrafast laser technologies. Each volume compiles peer-reviewed articles authored by researchers at the forefront of each their own subfields of UILS. Every chapter opens with an overview of the topics to be discussed, so that researchers unfamiliar to the subfield as well as graduate students can grasp the importance and attractions of the research topic at hand. These are followed by reports of cutting-edge discoveries. This eighth volume covers a broad range of topics from this interdisciplinary research field, focusing on molecules interacting with ultrashort and intense laser fields, advanced technologies for the characterization of ultrashort laser pulses and their applications, laser plasma formation and laser acceleration.

"Dynamics of Soft Matter: Neutron Applications" provides an overview of neutron scattering techniques that measure temporal and spatial correlations simultaneously, at the microscopic and/or mesoscopic scale. These techniques offer answers to new questions arising at the interface of physics, chemistry, and biology. Knowledge of the dynamics at these levels is crucial to understanding the soft matter field, which includes colloids, polymers, membranes, biological macromolecules, foams, emulsions towards biological & biomimetic systems, and phenomena involving wetting, friction, adhesion, or microfluidics.

Emphasizing the complementarities of scattering techniques with other spectroscopic ones, this volume also highlights the potential gain in combining techniques such as rheology, NMR, light scattering, dielectric spectroscopy, as well as synchrotron radiation experiments. Key areas covered include polymer science, biological materials, complex fluids and surface science.

Over the past two decades auroral science has developed from a somewhat mysterious and imprecise specialty into a discipline central in the study of the ionosphere and magnetosphere. The investigation of aurora unites scientists with very different backgrounds and interests so that it is difficult to write a self-contained account of the field in a book of reasonable length. In this work I have attempted to include those aspects of theory which I have found valuable in predicting the effects on the atmosphere of auroral particle precipitation. In addition I have attempted to describe the techniques of observation with particular emphasis on optical methods which have been useful. While the aeronomy of aurora has been regarded as central, the mechanisms by which particles are accelerated and precipitated into the atmosphere is of no less interest. This aspect of the subject has however been treated in a briefer fashion since it is a part of the immense and rapidly developing field of magnetospheric science. Generally I have attempted to provide a coherent introduction to auroral science with an emphasis on relatively simple physical interpretations and models. References are given to enable the reader to find more extensive or rigorous discussions of particular topics. A fairly complete, quantitative atlas of the auroral spectrum is included.

IAU Symposium No. 134 on Active Galactic Nuclei was hosted by the Lick Observatory, as part of the celebration of its centennial, for the Observatory went into operation as part of the University of California on June 1, 1888. Twenty years later, in 1908, Lick Observatory graduate student Edward A. Fath recognized the unusual emission-line character of the spectrum of the nucleus of the spiral "nebula" NGC 1068, an object now well-known as one of the nearest and brightest Seyfert galaxies and active galactic nuclei. Ten years after that, and seventy years before this Symposium, Lick Observatory faculty member Heber D. Curtis published his description of the "curious straight ray" in M 87, "apparently connected with the nucleus by a thin line of matter," which we now recognize as an example of one of the jets which are the subject of so much current AGN research. The symposium was held at Kresge College on the campus of the University of California, Santa Cruz, only a short walk through the redwood groves to the Lick Observatory offices. A total of 232 astronomers and astrophysicists from 24 countries attended and took part in the Symposium. About 200 more had applied to come, but could not be accepted in order to keep the meeting at a reasonable size. Most of the participants lived in the Kresge College apartments immediately adjacent to the Kresge Town Hall in which the oral sessions took place.

This textbook is a basic introduction to kinetic plasma phenomena in solar and stellar coronae. The author unifies observations and theory which gives a wide perspective to the subject. An important feature is the lucidly written presentation of the fundamentals of plasma physics. The basic theory developed is then extended to some exemplary and important observations of coronal dynamics, such as coronal current, particle acceleration, propagation of particle beams, and shocks. The book has grown from the author's introductory courses on plasma astrophysics at the Swiss Federal Institute of Technnology (ETH). It is aimed at advanced undergraduates and first-year graduate students without a background in plasma physics. It should also be of interest to more senior research workers involved in coronal physics, solar/stellar winds, and various other fields of plasma astrophysics. Problems suitable for class use are included at the end of each chapter.

This thesis explores the possibility of searching for new effects of dark matter that are linear in g, an approach that offers enormous advantages over conventional schemes, since the interaction constant g is very small, g<<1. Further, the thesis employs an investigation of linear effects to derive new limits on certain interactions of dark matter with ordinary matter that improve on previous limits by up to 15 orders of magnitude. The first-ever limits on several other interactions are also derived. Astrophysical observations indicate that there is five times more dark matter-an 'invisible' form of matter, the identity and properties of which still remain shrouded in mystery-in the Universe than the ordinary 'visible' matter that makes up stars, planets, dust and interstellar gases. Conventional schemes for the direct detection of dark matter involve processes (such as collisions with, absorption by or inter-conversion with ordinary matter) that are either quartic (g4) or quadratic (g2) in an underlying interaction constant g.

The book summarizes international progress over the last few decades in upper atmosphere airglow research. Measurement methods, theoretical concepts and empirical models of a wide spectrum of upper atmospheric emissions and their variability are considered. The book contains a detailed bibliography of studies related to the upper atmosphere airglow. Readers will also benefit from a lot of useful information on emission characteristics and its formation processes found the book.

Most of the specialists working in this interdisciplinary field of physics, biology, biophysics and medicine are associated with "The International Institute of Biophysics" (IIB), in Neuss, Germany, where basic research and possibilities for applications are coordinated. The growth in this field is indicated by the increase in financial support, interest from the scientific community and frequency of publications.

Audience: The scientists of IIB have presented the most essential background and applications of biophotonics in these lecture notes in biophysics, based on the summer school lectures by this group. This book is devoted to questions of elementary biophysics, as well as current developments and applications. It will be of interest to graduate and postgraduate students, life scientists, and the responsible officials of industries and governments looking for non-invasive methods of investigating biological tissues.

This book pays tribute to two pioneers in the field of Mathematical physics, Jiri Patera and Pavel Winternitz of the CRM. Each has contributed more than forty years to the subject of mathematical physics, particularly to the study of algebraic methods.

Reflector antennas are widely used in the microwave and millimeter wavelength domain. Radio astronomers have developed techniques of calibration of large antennas with radio astronomical methods. These have not been comprehensively described. This text aims to fill this gap. It takes a practical approach to the characterisation of antennas. All calculations and results in the form of tables and figures have been made with Mathematica by Wolfram Research. The reader can use the procedures for the implementation of his own input data. The book should be of use to all who are involved in the design and calibration of large antennas, like ground station managers and engineers, practicing radio astronomers and graduate students in radio astronomy and communication technology.

This NATO Advanced Study Institute course provided an updated understanding, from a fundamental and deep point of view, of the progress and current problems in the early universe, cosmic microwave background radiation, large-scale struc ture, dark matter problem, and the interplay between them. Emphasis was placed on the mutual impact of fundamental physics and cosmology, both at the theo retical and experimental or observational levels, within a deep and well defined programme, and a global unifying view, which, in addition, provides of careful inter-disciplinarity. In addition, each course of this series introduced and promoted topics or sub jects which, although not of a purely astrophysical or cosmological nature, were of relevant physical interest for astrophysics and cosmology. Deep understanding, clarification, synthesis, and careful interdisciplinarity within a fundamental physics framework, were the main goals of the course. Lectures ranged from a motivation and pedagogical introduction for students and participants not directly working in the field to the latest developments and most recent results. All lectures were plenary, had the same duration, and were followed by a discus sion. The course brought together experimentalists and theoreticans physicists, astro physicists and astronomers from a wide variety of backgrounds, including young scientists at the post-doctoral level, senior scientists and advanced graduate stu dents as well."

Proceedings of the 128th Symposium of the International Astronomical Union, held in Coolfont, West Virginia, USA, October 20-24, 1986.

This book offers an overview of state-of-the-art in non amplified DNA detection methods and provides chemists, biochemists, biotechnologists and material scientists with an introduction to these methods. In fact all these fields have dedicated resources to the problem of nucleic acid detection, each contributing with their own specific methods and concepts. This book will explain the basic principles of the different non amplified DNA detection methods available, highlighting their respective advantages and limitations. Non-amplified DNA detection can be achieved by adopting different techniques. Such techniques have allowed the commercialization of innovative platforms for DNA detection that are expected to break into the DNA diagnostics market. The enhanced sensitivity required for the detection of non amplified genomic DNA has prompted new strategies that can achieve ultrasensitivity by combining specific materials with specific detection tools. Advanced materials play multiple roles in ultrasensitive detection. Optical and electrochemical detection tools are among the most widely investigated to analyze non amplified nucleic acids. Biosensors based on piezoelectric crystal have been also used to detect unamplified genomic DNA. The main scientific topics related to DNA diagnostics are discussed by an outstanding set of authors with proven experience in this field.

The International Conference on the Theory of Machines and Mechanisms is organized every four years, under the auspices of the International Federation for the Promotion of Mechanism and Machine Science (IFToMM) and the Czech Society for Mechanics. This eleventh edition of the conference took place at the Technical University of Liberec, Czech Republic, 4-6 September 2012. This volume offers an international selection of the most important new results and developments, in 73 papers, grouped in seven different parts, representing a well-balanced overview, and spanning the general theory of machines and mechanisms, through analysis and synthesis of planar and spatial mechanisms, dynamics of machines and mechanisms, linkages and cams, computational mechanics, rotor dynamics, biomechanics, mechatronics, vibration and noise in machines, optimization of mechanisms and machines, control and monitoring systems of machines, accuracy and reliability of machines and mechanisms, robots and manipulators to the mechanisms of textile machines.

This book contains the expanded lecture notes of the 32nd Saas-Fee Advanced Course. The three contributions present the central themes in modern research on the cold universe, ranging from cold objects at large distances to the physics of dust in cold clouds.

1 Grundlagen.- 1.1 Allgemeine Grundlagen.- 1.1.1 Ziele und Aufgaben.- 1.1.2 Methoden.- 1.1.3 Geschichte und Einordnung.- 1.1.3.1 Geschichte der Bauwerksvermessung.- 1.1.3.2 Geschichte des Vermessungswesens.- 1.1.3.3 Geschichte der Architekturphotogrammetrie.- 1.1.4 Rechtliche Grundlagen und Rahmenbedingungen.- 1.1.4.1 Internationale Vereinbarungen und Organisationen.- 1.1.4.2 Baugesetzbuch, Denkmalpflegegesetze, Vermessungsgesetze.- 1.2 Messgroessen und Masseinheiten.- 1.2.1 Strecken.- 1.2.2 Winkel.- 1.3 Bezugssysteme und Koordinaten.- 1.3.1 Bezugsflachen.- 1.3.2 Koordinaten.- 1.3.3 Koordinatensysteme.- 1.3.3.1 Polarkoordinaten.- 1.3.3.2 Lokale Koordinatensysteme.- 1.3.3.3 Regionale Koordinatensysteme.- 1.3.3.4 Globale Koordinatensysteme.- 1.3.3.5 Geographische Koordinaten.- 1.3.3.6 Geozentrische Koordinaten.- 1.3.4 Koordinatentransformationen.- 1.3.4.1 Translation (2D).- 1.3.4.2 Massstabslose Transformation (2D).- 1.3.4.3 AEhnlichkeitstransformation (2D).- 1.3.4.4 Vereinfachte AEhnlichkeitstransformation mit 2 Passpunkten (2D).- 1.3.4.5 Affintransformation (2D).- 1.3.4.6 Weitere ebene Koordinatentransformationen.- 1.3.4.7 Raumliche Koordinatentransformation (3D).- 1.3.5 Festpunktfelder.- 1.3.5.1 Netz trigonometrischer Punkte zur Lagedefinition.- 1.3.5.2 Hoehennetz.- 1.3.6 Vermessungsnetze fur die Bauwerksvermessung.- 1.3.6.1 Netzdesign.- 1.3.6.2 Vermarkung.- 1.3.6.3 Design und Fertigung von Punktsignalisierungen.- 1.3.6.4 Auswahl naturlicher Passpunkte.- 1.3.6.5 Schnurnetz zur temporaren Vermarkung.- 1.3.6.6 Punktubersichten und Einmessskizzen.- 1.4 Fehlerlehre und Statistik.- 1.4.1 Fehlerarten und ihre Wirkung.- 1.4.1.1 Zufallige Fehler.- 1.4.1.2 Systematische Fehler.- 1.4.1.3 Grobe Fehler.- 1.4.2 Fehlerfortpflanzung und Ausgleichsrechnung.- 1.4.3 Rechenscharfe und Rundung.- 1.4.4 Toleranzen im Bauwesen.- 2 Dokumentation von Gebauden und Ensembles.- 2.1 Amtliche Dokumentation.- 2.1.1 Katasterunterlagen.- 2.1.2 Amtliche Karten.- 2.1.3 Lageplan.- 2.1.4 Geoinformationssysteme (GIS).- 2.2 Plane.- 2.2.1 Grundriss.- 2.2.2 Schnitt.- 2.2.3 Ansicht.- 2.2.4 Detaildarstellungen.- 2.2.5 Massstabe und Detaillierungsgrad.- 2.2.6 Materialien und Aufbewahrung.- 2.3 3D-Beschreibungen.- 2.3.1 CAD-Modell.- 2.3.2 Animation.- 2.3.3 Virtual Reality.- 2.3.4 Augmented Reality.- 2.4 Fotografie.- 2.4.1 Analoge Fotografie.- 2.4.1.1 Fotografisches Material.- 2.4.1.2 Kameras.- 2.4.1.3 Objektive.- 2.4.1.4 Licht.- 2.4.1.5 Belichtung.- 2.4.1.6 Archivierungen von Fotomaterialien.- 2.4.2 Digitale Bilder.- 2.4.2.1 Flachensensoren.- 2.4.2.2 Zeilenkameras.- 2.4.2.3 Spezialkameras.- 2.4.3 Scannen analoger Fotovorlagen.- 2.4.4 Digitale Bildverarbeitung.- 2.5 Textliche und hybride Beschreibungen.- 2.5.1 Raumbuch.- 2.5.2 Hypertext Dokumente.- 2.5.3 Informationssystem.- 2.6 Archivierung digitaler Daten.- 2.6.1 Datentrager.- 2.6.2 Datenformate.- 2.6.2.1 Texte.- 2.6.2.2 Datenbanken.- 2.6.2.3 Vektordaten.- 2.6.2.4 Rasterdaten.- 2.6.2.5 Hypermedia.- 3 Erfassung von Messelementen.- 3.1 Messprinzipien.- 3.1.1 Vom-Grossen-ins-Kleine.- 3.1.2 UEberbestimmungen.- 3.1.3 Vermeidung von systematischen Fehlern.- 3.2 Gerate und Instrumente.- 3.2.1 Bauteile, Kleingerate und Zubehoer.- 3.2.1.1 Lote und Libellen.- 3.2.1.2 Fernrohr.- 3.2.1.3 Stative.- 3.2.1.4 Fluchtstab.- 3.2.1.5 Nivellierlatten und Kleingerat.- 3.2.1.6 Aufstellen eines Instruments.- 3.2.2 Winkelmessung.- 3.2.2.1 Bestimmung rechter Winkel.- 3.2.2.2 Theodolit.- 3.2.2.3 Satzmessung.- 3.2.2.4 Berechnung von Richtungswinkeln aus Koordinaten.- 3.2.3 Streckenmessung.- 3.2.3.1 Streckenmessung mit dem Messband.- 3.2.3.2 Optische Streckenmessung.- 3.2.3.3 Elektro-optische Entfernungsmessung (EDM).- 3.2.4 Hoehenmessung.- 3.2.4.1 Einfache Werkzeuge.- 3.2.4.2 Nivellement.- 3.2.4.3 Rotationslaser.- 3.3 Beschaffung einer Vermessungsausrustung.- 4 Messverfahren.- 4.1 Schrittskizze.- 4.2 Handaufmass.- 4.3 Punktbestimmung ohne Theodolit.- 4.3.1 Bogenschlag.- 4.3.2 Einbindeverfahren.- 4.3.3 Orthogonalverfahren.- 4.3.4

This text presents a comprehensive account of the magnetic fields of various celestial bodies - the Sun, the Moon, planets, stars, the Milky Way, and galaxies, as well as the interplanetary, interstellar and intergalactic media. The original Chinese edition was published in Beijing in 1978. The present English edition has been enhanced and thoroughly rewritten. This monograph is characterized by its detail and may be used as a reference and textbook for scientific researchers and students of astronomy, space physics, geophysics and other related sciences.

The mono graph contains 8 chapters, and their contents cover all principal aspects of the problem: 1. Introduction and brief his tory ofthe radiation problem and background information ofradiation hazard in the near-Earth and interplanetary space. 2. General description of radiation conditions and main sources of charged partic1es in the Earth's environment and interplanetary space, effects of space environment on spacecraft. 3. Basic information about physical conditions in space and main sources of charged particles in the Earth's environment and interplanetary space, in the context of "Space W eather" monitoring and prediction. 4. Trapped radiation belts of the Earth (ERB): theory of their origin, spatial and temporal dynamics, and experimental and statistical models. 5. Galactic cosmic rays (GCR): variations of energetic, temporal and spatial characteristics, long-term modulation, and anomalous cosmic ray (ACR) component, modeling oftheir dynamics. 6. Production of energetic particles (SEPs) at/ne ar the Sun: available databases, acceleration, propagation, and prediction of individual SEP event, statistical models of solar cosmic rays (SCR). 7. Existing empirical techniques of estimating, prediction and modeling of radiation hazard, methodical approaches and constraints, some questions of changes in the Earth's radiation environment due to changes of the solar activity level. 8. Unresolved problems of radiation hazard prediction and spacecraft protection, radiation experiments on board the spacecraft, estimating of radiation conditions during interplanetary missions. Space does not allow us to explain every time the solar-terrestrial and radiation physics nomencIature used in current English-language literature.

Continuum Mechanics of Anisotropic Materials(CMAM) presents an entirely new and unique development of material anisotropy in the context of an appropriate selection and organization of continuum mechanics topics. These features will distinguish this continuum mechanics book from other books on this subject. Textbooks on continuum mechanics are widely employed in engineering education, however, none of them deal specifically with anisotropy in materials. For the audience of Biomedical, Chemical and Civil Engineering students, these materials will be dealt with more frequently and greater accuracy in their analysis will be desired. Continuum Mechanics of Anisotropic Materials' author has been a leader in the field of developing new approaches for the understanding of anisotropic materials.

Astrophysics is facing challenging aims such as deep cosmology at redshift higher than 10 to constrain cosmology models, or the detection of exoplanets, and possibly terrestrial exoplanets, and several others. It requires unprecedented ambitious R&D programs, which have definitely to rely on a tight cooperation between astrophysics and optics communities. The book addresses most of the most critical interdisciplinary domains where they interact, or where they will do. A first need is to collect more light, i.e. telescopes still larger than the current 8-10 meter class ones. Decametric, and even hectometric, optical (from UV to IR wavelengths) telescopes are being studied. Whereas up to now the light collecting surface of new telescopes was approximately 4 times that of the previous generation, now this factor is growing to 10 to 100. This quantum leap urges to implement new methods or technologies developed in the optics community, both in academic labs and in the industry. Given the astrophysical goals and technological constraints, new generation adaptive optics with a huge number of actuators and laser guide stars devices have to be developed, from theoretical bases to experimental works. Two other newcomers in observational astrophysics are interferometric arrays of optical telescopes and gravitational wave detectors. Up-to-date reviews of detectors and of spectrographs are given, as well as forefront R&D in the field of optical coatings and of guided optics. Possible new ways to handle photons are also addressed, based on quantum physics. More and more signal processing algorithms are a part and parcel of any modern instrumentation. Thus finally the book gives two reviews about wavefront processing and about image restoration and deconvolution algorithms for ill conditioned cases.

The sine-Gordon model is a ubiquitous model of Mathematical Physics with a wide range of applications extending from coupled torsion pendula and Josephson junction arrays to gravitational and high-energy physics models. The purpose of this book is to present a summary of recent developments in this field, incorporating both introductory background material, but also with a strong view towards modern applications, recent experiments, developments regarding the existence, stability, dynamics and asymptotics of nonlinear waves that arise in the model. This book is of particular interest to a wide range of researchers in this field, but serves as an introductory text for young researchers and students interested in the topic. The book consists of well-selected thematic chapters on diverse mathematical and physical aspects of the equation carefully chosen and assigned.

Ocean engineering is generally considered to be concerned with studies on the effects of the ocean on the land and with the design, construction and operation of vehicles, structures and systems for use in the ocean or marine environment. The practice of engineering differs from that of science in both motivations and objectives. Science seeks understanding of the principles of nature in terms of generalizations expressed as laws and classifications. Engineering seeks the application of knowledge of the physical and natural world to produce a benefit expressed as a device, system, material, and/or process. From the standpoint of the financial sponsors of an engineering project, the ideal approach is one of minimal risk in which only proven knowledge, materials and procedures are employed. There is frequent departure from this ideal in anticipation of the increased benefit expected from a large increase in performance of a structure or device. The process of acquiring this new capability is engineering research. Historically, ocean engineering developed with the application of engineering principles and processes to the design of ships and, later, to the machinery that propels them. In most societies, naval architecture and marine engineering are recognised as the origin of ocean engineering. In fact, the design of a ship constitutes the original systems engineering programme involving hydrodynamics/fluid flow, structural design, machinery design, electrical engineering and so on as well as requiring knowledge of the ocean environment (waves, corrosion, etc.).

This concise and systematic account of the current state of this new branch of astrophysics presents the theoretical foundations of plasma astrophysics, magneto-hydrodynamics and coronal magnetic structures, taking into account the full range of available observation techniques -- from radio to gamma. The book discusses stellar loops during flare energy releases, MHD waves and oscillations, plasma instabilities and heating and charged particle acceleration. Current trends and developments in MHD seismology of solar and stellar coronal plasma systems are also covered, while recent progress is presented in the observational study of quasi-periodic pulsations in solar and stellar flares with radio, optical, X and gamma rays. In addition, the authors investigate the origin of coherent radio emission from stellar loops, paying special attention to their fine structure. For advanced students and specialists in astronomy, as well as theoretical and plasma physics.

Well logging has come a long way from the simple electrical devices of the early years. Today's tools are much more diverse in their applications. Among these are tools which characterize geological properties of rocks in the borehole in a way that was previously only possible with oriented cores. Thus, borehole imaging, nuclear spectroscopy, nuclear magnetic resonance, and paleomagnetic logging provide precise information on bedding, mineralogy, texture and age of the rocks traversed by the borehole. Many of these logs can not only be acquired in the traditional "wireline" mode, but also in logging-while-drilling mode where the sensors are placed directly behind the drill bit, and the measurements are transmitted in real-time to the surface. Combined with new technology to drill deviated wells, the geoscientist now has tools which enable him to specify and develop reservoirs more accurately. This book is for researchers, graduate students and practising geoscientists.