Advanced Nanocomposites for Photonics and Optoelectronics and Mechanics
This reprint presents nine insightful articles focused on nanostructured materials and nanocomposites. Nanocomposites, which integrate nanosized materials into a standard material matrix, exhibit remarkable enhancements in properties across various domains, such as photonics, optoelectronics, and mechanics. The addition of nanomaterials brings about substantial changes in the electronic properties of normal nanomaterials with quantum size effects, leading to profound modifications in their photonic, optoelectronic, and mechanical performances compared to their bulk counterparts. This reprint comprises original research and review articles that address the preparation, characterization, and applications of nanostructured materials and nanocomposites, with a particular focus on photonic, optoelectronic, and mechanical aspects. We hope that this reprint will inspire further research, stimulate new ideas, and contribute to the advancement of the field of nanostructured materials and nanocomposites.
Mathematical Physics and Matrix Representations
This book expounds three kinds of matrices that are of physical interest, centering on physical examples. Stochastic matrices describe dynamical systems of many different types, involving (or not) phenomena like transience, dissipation, ergodicity, nonequilibrium and hypersensitivity to initial conditions. The main characteristic is growth by agglomeration, as in glass formation. Circulants are the building blocks of elementary Fourier analysis and provide a natural gateway quantum mechanics, noncommutative geometry and random walks, including some phenomenology like diffusion-advection equation and prey-predator chains.We also present two applications: chemical reaction and genetics. The last subject may seem specially out of place in "Mathematical Physics". Our excuse is that Mendelism and blood types are here presented by using just the same methods of the other chapters. Bell polynomials offer closed expressions for many formulas concerning Lie algebra invariants, differential geometry and real gases, and their matrices are instrumental in the study of chaotic mappings.
The Archive and the Aural City
In The Archive and the Aural City, Alejandro L. Madrid examines the possibilities for retrieving from the archive sounds that were not meant to be heard. Drawing on ?ngel Rama's notion of the Lettered City, Madrid proposes a notion of the Aural City-a Latin American urban intellectual elite for whom sound and listening are central to the creation, re-creation, and circulation of new types of knowledge. While many of these elites carry forward a nationalistic agenda, Madrid contends that the Aural City's archives and the ways they are listened to and conceived through sound and music can also help dismantle dominant frameworks of national or colonial culture and build more inclusive spaces for intellectual exchange and political mobilization. From national archives in Latin America and colonial institutions abroad to sound exhibits, instruments, and internet-based archival projects, Madrid demonstrates how the development of urban spaces is understood through sound. In this way, he expands understandings of the archive's social and sonic power.
Introduction to Special Functions for Applied Mathematics
Introduction to Special Functions for Applied Mathematics introduces readers to the topic of special functions, with a particular focus on applications.
Statistical Mechanics for Physicists and Mathematicians
Statistical mechanics employs the power of probability theory to shine a light upon the invisible world of matter's fundamental constituents, allowing us to accurately model the macroscopic physical properties of large ensembles of microscopic particles. This book delves into the conceptual and mathematical foundations of statistical mechanics to enhance understanding of complex physical systems and thermodynamic phenomena, whilst also providing a solid mathematical basis for further study and research in this important field. Readers will embark on a journey through important historical experiments in statistical physics and thermodynamics, exploring their intersection with modern applications, such as the thermodynamics of stars and the entropy associated with the mixing of two substances. An invaluable resource for students and researchers in physics and mathematics, this text provides numerous worked examples and exercises with full solutions, reinforcing key theoretical concepts and offering readers deeper insight into how these powerful tools are applied.
Crystals and Compounds
This is a print on demand edition of a hard-to-find monograph.
Nuclear Reactor Physics and Operation
This book serves as a thorough reference for students, researchers, and professionals in nuclear engineering and reactor physics, offering a detailed exploration of the core principles behind nuclear reactor theory, neutron transport, neutronic analysis, and reactor core design and calculations.
To Be Spirituel - The Theories
This is Ashtars theories that in the end, ends up in direction of instructions for a construct of free energy. More the theoretical part. The is the second part of "To Be Spirituel" It moves around in many areas within the laws of basic mathematics. And he has his whole own view on how he see an "Atom". And the why's behind. He has his own unique way of thinking. And he did not have any help or aid doing this theory. Other that his basic learnings and teachings in life. He has an education as electrician. Even though, he also calls himself a "Zero-point engineer". Ashtar do not believe in "Perfection" or "Perfect". "Theres no suchs thing in this universe". He says. Maybe when You have gone trough this theory, you will agree . About "Perfect" and what that is. It also is explainations on "How" he being spirituel, also looks at it with a scientific point-of-view and perspective. And it is ofcourse his believes and claims. He forces no-one to believe him. With his writtings. He believes there is a "Spirituel Evolution" on the horizen, in more than one way. A one, without being violent.
Enhancement of Heat Transfer in Solar Air Heater
An investigation is done in relation to heat transfer enhancement in solar air heaters with circular V-shaped down ribs. Ribs were attached to the absorber plate, having an angle of attack (α= 60 ⁰). The ratio of rib height to hydraulic diameter (e/D) was 0.047, while the range of rib pitch-to-height ratio was (P/e = 4, 8, and 16) mm for three different sheets, with the Reynolds number ranging from (Re = 1825-7759). The roughened wall of the duct is heated by direct sunlight, while the remaining three walls are insulated. The concept of a V-shaped rib was developed to capitalise on this span-wise variation of heat transfer for inclined ribs. The V-shaped rib reduced the span-wise variation of heat transfer and increased average heat transfer.
Exoplanets and the Search for Alien Life
What if we're not alone in the universe? What if the answer has already been discovered-light years away? This captivating deep dive explores one of humanity's greatest quests: the search for life beyond Earth. With new exoplanets discovered almost daily and space telescopes peering into distant galaxies, the age-old question-"Are we alone?"-is becoming a scientific investigation rather than pure speculation. Inside, you'll explore: - How astronomers detect planets around other stars - What makes a world "habitable" and why Earth-like isn't the only model - The role of water, atmospheres, and biosignatures in the hunt for life - How missions like Kepler, TESS, and JWST are rewriting what's possible - The philosophical and cultural implications of finding alien life From the chemistry of life to the silence of the void, this book invites you to witness the epic, unfolding journey to understand our place in the cosmos. Whether you're a stargazer, science lover, or deep thinker, this is your gateway to the thrilling frontier of planetary exploration.
A Compton Scatter Camera for Spectral Imaging of 0.5 to 3.0 MeV Gamma Rays
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Elements of Astronomy;
"Elements of Astronomy" by Selim H. Peabody offers a comprehensive overview of astronomical principles suitable for students and general readers. Originally published in 1897, this book provides a detailed exploration of celestial bodies, the solar system, and the laws governing their movements. Peabody's work covers essential topics such as the use of telescopes, the nature of stars, and the measurement of astronomical distances. With clear explanations and diagrams, "Elements of Astronomy" serves as an invaluable resource for understanding the fundamentals of astronomy. This edition retains the original text and illustrations, offering both historical insights and a solid foundation in astronomical science.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Census of the Exact Sciences in Sanskrit (Series A, Vol. 3)
This installment of the "Census" provides all available biblio. info. concerning works in jyotihsastra & related fields & bio. info. concerning their authors. Jyotihsastra is traditionally divided into 3 skandhas or branches: hora or genethlialogy & other forms of horoscopic astrology, ganita or mathematics & mathematical astronomy, & samhita or divination. This vol. is devoted to those authors whose names begin with a cerebral (c, ch, j, & jh), a reflexive (t, th, d, & dh), or a dental (t, th, d dh, & n). Preceding the material relating to these authors is a section supplemental to vols. I & II. This section contains abbrev. of new periodicals & series that have been consulted, a biblio. of books & articles that have appeared or have been belatedly noticed since vol. II went to press, & a list of catalogs it has been possible to utilize. The rest of the vol. contains supplementary info. concerning 100 authors already noted in the two previous vols. & all the data currently available concerning almost 800 new authors. Reprinted 1992.
The World of Comets
Explore the wonders of the cosmos with "The World of Comets" by Am矇d矇e Guillemin. Originally published in 1877, this volume offers a fascinating glimpse into the 19th-century understanding of comets, their nature, and their place in the solar system. Guillemin's work provides a detailed account of these celestial wanderers, blending scientific observation with accessible prose. This book is a valuable resource for anyone interested in the history of astronomy, offering insights into the evolution of scientific thought and the enduring allure of comets. Delve into the historical perspective on these mesmerizing objects and discover the captivating world of cometary science as it was understood over a century ago.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Application of KAM Theorem to Earth Orbiting Satellites
An orbit that lies on a Kolmogorov, Arnold, and Moser (KAM) Torus will remain on that torus until and unless it experiences a force that causes it to leave the torus. Earth satellites that are subject only to the Earth's gravity field may lie on such KAM tori. Analyzing on orbit satellite position data should allow for the identification of the fundamental frequencies needed to define the KAM tori for modeling Earth satellite orbits. KAM Tori are created for the Gravity Recovery and Climate Experience (GRACE) and Jason-1 satellites to model their orbital motion. Precise position data for the satellites is analyzed using a modified Laskar frequency algorithm to determine the fundamental frequencies of the orbits. The fundamental frequencies along with a set of Fourier coefficients completely describe the tori. These tori are then compared to the precise orbital position data for the satellites to determine how well they model the orbits. The KAM torus created for the Jason-1 satellite is able to represent the position of the satellites to within 1 km.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Planetary, Lunar, and Solar Positions, New and Full Moons, A.D. 1650-1805
These tables cover the period from the mid-17th to the 19th cent. when astronomical ephemerides were evolving most rapidly. These tables resemble those previously pub. by the APS: Tuckerman's "Planetary, Lunar, and Solar Positions, 601 B.C. to A.D. 1" and "A.D. 2 to A.D. 1649" and Goldstine's "New and Full Moon, 1001 B.C. to A.D. 1651." The tables contain features consistent with the almanacs and ephemerides pub. in this period: planetary positions are computed for 12 hours U.T. (noon); and the Julian day number is given for new and full moons. An analytical essay examines the theoretical and computational developments in almanac-making in the period that bridges between Kepler and Laplace.
Spin Moir矇 Engineering and Emergent Electromagnetism in Topological Spin Crystals
Stability Domains in Nonlinear Point Reactor Dynamics
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Astronomical Papyri from Oxyrhynchus (Vol. I and II)
Presents 200 hitherto unpub. astronomical texts & horoscopes written in Greek on papyrus, which were excavated a century ago in the rubbish heaps of Oxyrhynchus, a district capital of Roman Egypt. Through these documents we obtain the first coherent picture of the range of astronomical activity, chiefly in the service of astrology, during the Roman Empire. The astronomy of this period turns out to have been much more varied than we previously thought, with Babylonian arithmetical methods of prediction coexisting with tables based on geometrical models of orbits. Editions of the texts are accomp. by facing translations & explanatory & philological commentaries. The intro. provides the first comprehensive treatment of astronomical papyri, explaining their contents & purpose, the underlying astronomical theories, & strategies for analyzing & dating them. Tables & graphs.
Mossbauer Studies of the Transition Element Halides
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Solid-State Nuclear Magnetic Resonance Studies of Cross Polarization From Quadrupolar Nuclei
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
A Laboratory Course in Experimental Physics
"A Laboratory Course in Experimental Physics" offers a detailed guide to conducting physics experiments, reflecting the state of scientific education in the late 19th century. Authored by W. J. Loudon and J. C. McLennan, this book provides a structured approach to learning through hands-on experimentation. Designed for use in a laboratory setting, the course outlines various experiments covering fundamental principles of physics. Students are guided through the process of setting up equipment, taking measurements, and analyzing results. This hands-on approach aims to deepen understanding and reinforce theoretical knowledge. Originally published in 1895, this work offers a valuable glimpse into the history of physics education and the methods used to train aspiring scientists during that era. It remains relevant for those interested in historical scientific practices and the evolution of physics instruction.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Practical and Spherical Astronomy, for the Use Chiefly of Students in the Universities
"Practical and Spherical Astronomy" by Robert Main is a comprehensive guide intended primarily for university students. Originally published in 1863, this book offers a detailed exploration of practical astronomy, including methods for making astronomical observations and reducing them. Special emphasis is given to spherical astronomy, a branch of astronomy that deals with locating astronomical objects on the celestial sphere, without regard to their distance. This book provides a solid foundation in astronomy and continues to be a valuable resource for students and enthusiasts alike.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Determination of the Parallaxes of Fifty Stars
"Determination of the Parallaxes of Fifty Stars" presents the results of astronomical observations and calculations to determine the distances of fifty stars using the parallax method. This meticulous work, originally published in 1910, contributes valuable data to the field of astrometry and provides insights into the scale and structure of the universe as it was understood at the time. The study involves precise measurements and mathematical analysis, showcasing the scientific rigor of early 20th-century astronomical research. This book is a key resource for historians of science, astronomers, and anyone interested in the development of our understanding of stellar distances. The careful methodology and detailed results offer a glimpse into the challenges and achievements of early parallax determination, which remains a cornerstone of modern astrophysics.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Census of the Exact Sciences in Sanskrit (Series A, Vol. 4)
This fourth volume of the "Census" provides all available bibliographical info. concerning works in jyotihsastra & related fields & biographical info. concerning their authors. Jyotihsastra is traditionally divided into 3 skandhas or branches: hora or genethlialogy & other forms of horoscopic astrology, ganita or mathematics & mathematical astronomy, & samhita or divination. This volume contains articles on authors whose names being with labials (p, ph, b, bh, & m). These are preceded by material supplemental to vol. I, II, & III. This material consists of abbrev. of new periodicals & serials that have been consulted, a biblio. of books & articles that have been noticed since volume III went to press, & a list of additional catalogs that have been utilized.
Non-Coding RNA
Non-coding RNA, Volume 214 in the Progress in Molecular Biology and Translational Science series, highlights advances in the field, with this new volume presenting interesting chapters on topics such as An introduction to non-coding RNAs, Non-coding RNAs in Eutherians and Livestocks, Artificial intelligence and machine learning heuristics for discovery of ncRNAs in humans, Non-coding RNAs in Plants, Epigenetic and experimental approaches influencing ncRNAs, Noncoding RNAs in bacteria, Dissecting ncRNA pathways and omics integration, Structural prediction of potent ncRNAs, Artificial intelligence and machine learning heuristics for discovery of ncRNAs in humans, Tools and Databases for non-coding RNAs, and Physiogenomics and genetic landscape of ncRNAs.
Arabic Version of Ptolemy's Planetary Hypotheses
This is a print on demand edition of an important, hard-to-find publication.
Circular Magnetic X-Ray Dichroism in Rare Earth Compounds
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Scent of Time. a Study of the Use of Fire and Incense for Time Measurement in Oriental Countries
This is a print on demand edition of an important, hard-to-find publication. Over 40 illustrations.
Practical Measurements in Radioactivity
Practical Measurements in Radioactivity, by Walter Makower, offers a detailed examination of the methods and techniques used to measure radioactivity in the early 20th century. This comprehensive guide provides practical insights into the instruments and procedures employed to quantify radioactive substances, making it an invaluable resource for students, researchers, and professionals in the field. The book covers a range of topics, including ionization methods, the use of electroscopes, and the determination of radioactive decay rates. Makower's work is characterized by its clear explanations and meticulous attention to detail, ensuring that readers gain a solid understanding of the principles underlying radioactivity measurements. While reflecting the scientific understanding of its time, this book remains a significant historical document, offering a glimpse into the pioneering efforts to understand and quantify the phenomenon of radioactivity. A crucial addition to any collection focusing on the history of science and technology.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
A Cross Section Measurement of Charm Hyperons In 250 GeV p/K Nucleon Interactions
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Vibrations, Their Principles; Light and Colors, Their Uses ..
"Vibrations, Their Principles; Light and Colors, Their Uses" explores the fundamental principles of vibrations, sound, light, and color, delving into their scientific underpinnings and practical applications. Written by Ernest Jack. Stevens, this volume provides a comprehensive overview of these interconnected phenomena, elucidating their properties and behaviors. From the physics of sound waves to the nature of light and the perception of color, the book offers insights into the physical world.Readers interested in the science of acoustics, optics, and the broader field of physics will find this an informative read. Its value lies in providing a detailed explanation of these principles and their practical use.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Anelastic Study of Divacancy Damping in Gold
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
A Review of Methods Applied by the U.S. Geological Survey in the Assessment of Identified Geothermal Resources
The U. S. Geological Survey (USGS) is conducting an updated assessment of geothermal resources in the United States. The primary method applied in assessments of identified geothermal systems by the USGS and other organizations is the volume method, in which the recoverable heat is estimated from the thermal energy available in a reservoir. An important focus in the assessment project is on the development of geothermal resource models consistent with the production histories and observed characteristics of exploited geothermal fields. The new assessment will incorporate some changes in the models for temperature and depth ranges for electric power production, preferred chemical geothermometers for estimates of reservoir temperatures, estimates of reservoir volumes, and geothermal energy recovery factors. Monte Carlo simulations are used to characterize uncertainties in the estimates of electric power generation. These new models for the recovery of heat from heterogeneous, fractured reservoirs provide a physically realistic basis for evaluating the production potential of natural geothermal reservoirs.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
A Compton Scatter Camera for Spectral Imaging of 0.5 to 3.0 MeV Gamma Rays
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
The Detection and Measurement of the Electrical Mobility Size Distributions Associated With Radon Decay Products
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Determination of the Parallaxes of Fifty Stars
"Determination of the Parallaxes of Fifty Stars" presents the results of astronomical observations and calculations to determine the distances of fifty stars using the parallax method. This meticulous work, originally published in 1910, contributes valuable data to the field of astrometry and provides insights into the scale and structure of the universe as it was understood at the time. The study involves precise measurements and mathematical analysis, showcasing the scientific rigor of early 20th-century astronomical research. This book is a key resource for historians of science, astronomers, and anyone interested in the development of our understanding of stellar distances. The careful methodology and detailed results offer a glimpse into the challenges and achievements of early parallax determination, which remains a cornerstone of modern astrophysics.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Egyptian Planetary Texts
This is a print on demand edition of an important, hard-to-find publication. 27 plates.
Elements of Astronomy;
"Elements of Astronomy" by Selim H. Peabody offers a comprehensive overview of astronomical principles suitable for students and general readers. Originally published in 1897, this book provides a detailed exploration of celestial bodies, the solar system, and the laws governing their movements. Peabody's work covers essential topics such as the use of telescopes, the nature of stars, and the measurement of astronomical distances. With clear explanations and diagrams, "Elements of Astronomy" serves as an invaluable resource for understanding the fundamentals of astronomy. This edition retains the original text and illustrations, offering both historical insights and a solid foundation in astronomical science.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Radiation Damage From Internal Alpha Decay in Thorium
The Office of Scientific & Technical Information (OSTI), is a part of the U.S. Department of Energy (DOE) that houses research and development results from projects funded by the DOE. The information is generally an article, technical document, conference paper or dissertation. This is one of those publications.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Planetary, Lunar and Solar Positions, 601 B.C. to A.D. 1, at Five-Day and Ten Day Intervals
The need for these tables became pressing when hundreds of astronomical cuneiform tables in the British Museum became available for study, partly through the copies made in the 1880s and 1890s. All these texts originally came from some archive in Babylon which was discovered by Arabs in the middle of the 19th century. Most of the texts were written from about 330 B.C. to the first century A.D. Many of the texts are fragments of the original clay tables which have broken. In many cases, a fragment contains only parts of a few legible lines. Much of the information is of an astronomical character. It is evident that for investigations of these tablets the possibility of rapid scanning of accurately dated planetary positions is of primary importance.
Practical Astronomy With the Unaided Eye
"Practical Astronomy With the Unaided Eye" offers a comprehensive introduction to the wonders of the night sky, accessible to anyone with an interest in astronomy. Written by Hector Macpherson, this timeless guide provides readers with the knowledge to identify constellations, planets, and other celestial phenomena without the need for telescopes or other equipment. Macpherson's clear and engaging style makes complex concepts easy to understand, offering practical advice on how to observe the sky effectively. Whether you are a beginner or an experienced stargazer, this book will enhance your appreciation of the universe. Discover the joy of exploring the cosmos with just your eyes and this insightful guide.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
Spectrum of Beta Lyrae
This is a print on demand edition of an important, hard-to-find publication. Over 150 illustrations.
