Census of the Exact Sciences in Sanskrit (Series A, Vol. 5)
The fifth installment of a projected "Census of the Exact Sciences in Sanskrit," which will provide 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 math. & mathematical astronomy, & samhita or divination. This vol. contains entries on authors whose names being with the Sanskrit semivowels (y, r, l, & v). This material is preceded by additional abbrev. of journals, additional biblio., & additional manuscript catalogs, as well as entries supplemental to those in vols. I-IV of Series A. No new material after Spring of 1992.
Mechanical Universe
This is a print on demand edition of an important, hard-to-find publication.
Planetary, Lunar, and Solar Positions, A.D. 2 to A.D. 1649, at Five-Day and Ten-Day Intervals
These tables for A.D. 2 to A.D. 1649 are an extension, with some improvements, of earlier ones for 601 B.C. to A.D. 1. As before, they give the geocentric positions (tropic celestial longitudes & latitudes, i.e. with respect to the mean equinox of date), in units of 0 degrees.01 for the Sun & planets, & 0 degrees.1 for the Moon, at 16h Universal Time - 4 P.M. Greenwich Civil Time - 7 P.M. local mean time of 45 degrees East longitude (Babylon), on the indicated dates, all in the Julian calendar, hence for Julian dates 5n + 1/6 for the Moon, Mercury, & Venus, & 1-n + 1/6 for the Sun, Mars, Jupiter, & Saturn. The same adaptation of the theories of Leverrier, Gaillot, & Hansen, with modified elements by Schoch, was used as before, except as noted below. The chief change has been to improve the positions of Jupiter & Saturn. Tables.
Egyptian Planetary Texts
This is a print on demand edition of an important, hard-to-find publication. 27 plates.
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.
Arabic Version of Ptolemy's Planetary Hypotheses
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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.
Velocity of Light
This is a print on demand edition of a hard to find publication. Illustrations.
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.
Survey of Islamic Astronomical Tables
The source material for the study of medieval oriental astronomy consists of Byzantine Greek, Sanscrit, Hebrew, Arabic, Persian, and Turkish astronomical and astrological manuscripts. If one desires to build up a detailed picture of Islamic astronomy, one can choose material from these available manuscripts. Of these manuscripts it is possible to isolate a group of works, the "zijes". A "zij" consists of the numerical tables and accompanying explanation sufficient to measure time and to compute planetary and stellar positions, appearance, and eclipses. This paper is a survey of the number, distribution, contents, and relations between "zijes" written in Arabic or Persian during the period from the 8th through the 15th centuries. Illustrations. Oversize.
Theoretical Issues on Systems Science
In "Theoretical Issues on Systems Science", we present theoretical issues including theoretical incompleteness, multiplicity, systems as networks and chaos, game theory, and meta-structures. Other less explored research topics include equivalence and tolerance in systems, pending systems, recurrence and self-reflexivity, remote synchronization, and the significance of using complex numbers in system models.The first group of papers addresses theoretical aspects, including 1) the role of noise in complex systems; 2) the potential of general systems theory to serve as a theory of everything; 3) the drawbacks of applying classical axiomatic deductive mathematical approaches to topics such as control evolution by rewriting DNA "instructions"; 4) the near non-existence of purely "theory-free" approaches and the balance between theoretical and empirical contributions; 5) the neglect in reductionism in that systems acquire properties and the assumption that multiple, variable interactions of complexity can be analytically "zipped"; and 6) tree-based methods for statistical learning, for which the author presents a systems theory-based framework to speed up discrete event system stochastic simulations.The second group of papers examines theoretical aspects within specific fields, including 1) human dynamics; 2) human cognition; 3) complex physiological processes; 4) medicine; 5) chemical organization theory; and 6) psychotherapy.
ARC Spectrum of Iron
This is a print on demand edition of an important, hard-to-find publication.
Construction of Isobaric Charts for High Levels in the Earth's Atmosphere and Their Dynamic Significance
This is a print on demand edition of an important, hard-to-find publication.
Popular Lectures and Addresses
Popular Lectures and Addresses, Volume 3 presents a collection of essays and speeches by the eminent physicist William Thomson, Baron Kelvin. Spanning a range of topics within physics and engineering, these lectures offer insights into the scientific thought of the late 19th century. Kelvin's accessible style makes complex subjects understandable, revealing the practical applications of scientific principles.This volume showcases Kelvin's contributions to thermodynamics, electricity, and molecular physics. His ability to connect theoretical concepts to real-world problems demonstrates his commitment to advancing scientific knowledge. "Popular Lectures and Addresses" remains a valuable resource for those interested in the history of science and the foundations of modern physics.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.
New and Full Moons, 1001 B.C. to A.D. 1651
Originally pub. in 1973; reprinted in 1994. Presents tables giving the dates of all new and full moons during an historical era when these data were of considerable interest and importance. The longitudes of the moon at each of these times is also given, as is a consecutive enumeration of the conjunctions and a similar one of the oppositions. All dates are reckoned in the Julian calendar. These dates and times are calculated for an observer in Babylon, or equivalently Baghdad, since this location is fairly centrally located for the historians of the period. The time used is civil time and is based on a 24-hour clock with its origin at midnight. Since this vol. may be considered as a suppl. to Tuckerman's tables, all fundamental astronomical elements have been taken from them.
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.
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.
Solving the Planetary CO2 Problem
In this book, we highlight key dogmatic beliefs in mainstream physics that contradict well-established experimental results. Grounded in these facts, we reveal that a unification will come to electromagnetism, gravitation, and inertia after realizing that they are all phenomena of the same material fluid (not of the molecular matter but of the finer field-matter). This leads to a corrected, nonlinear, non-Maxwellian form of electromagnetism, unified with a non-Einsteinian approach to gravitation and inertia. The classical theories of Maxwell, of Newton, and even of Einstein's special relativity emerge as special cases or approximations after the true Navier-Stokes non-linear equations of the fieldmatter fluid. We also present the prediction that solar energy is continuously stored in the gravitational field and can be harnessed using methods similar to Nikola Tesla's inventions-technologies that remain largely misunderstood in academic physics. This approach opens a path to solving the CO₂ problem through access to constant, low-cost solar energy. It also suggests the potential for new electromagnetic propulsion systems, reminiscent of the alleged flying discs.
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.
Revolution in Measurement
Zupco presents the legacies of the Middle Ages to the pioneering reformers of the Scientific Revolution; the monumental impact of math, physics, chemistry, astronomy, & technology on modern metrology; the creations, struggles, & successes of the Metric System; & the intense battles between metrics & customary metrologies that have waged since the end of the 18th cent. Includes insights into the personalities involved in metrological events: scientists, technologists, bureaucrats, ministers, members of scientific soc., & shows the impact of scientific experimentation & social revolutions. Includes a comprehensive biblio. of European metrology & the sources relevant to the underpinnings for this period in weights & measures history. Illus.
Spectrum of Beta Lyrae
This is a print on demand edition of an important, hard-to-find publication. Over 150 illustrations.
Sanskrit Astronomical Tables in the United States
This is a print on demand edition of an important, hard-to-find publication.
Spin Moir矇 Engineering and Emergent Electromagnetism in Topological Spin Crystals
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.
Recurrence Plots and Their Quantifications: Methodological Breakthroughs and Interdisciplinary Discoveries
This book collects selected contributions from the 10th Recurrence Plot Symposium, held at the University of Tsukuba, Japan (August 28-30, 2023). It reflects on the achievements of the previous nine symposia while exploring future prospects of recurrence plots and their quantifications in combination with other key research strategies. The book provides a comprehensive bibliographic overview of the methodology, offering a solid foundation for both new and experienced researchers. It discusses the mathematical foundations of recurrence plots and recurrence microstates and links them to future directions, such as machine learning, highlighting the potential for innovative applications. The text also presents an alternative approach to representing recurrences, offering fresh perspectives on this well-established technique. Additionally, it explores the two-dimensional projections of three-dimensional chromosomal structures as dot maps, opening the door to unique chromosomal descriptions in terms of recurrence quantifiers. Numerous other contributed chapters highlight the active development of this method and its clever applications to real-world systems. The book is intended for researchers working in various fields such as physics, statistics, and mathematics, with its interdisciplinary applications also benefiting experts from psychology, physiology, geosciences, finance, and engineering.
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.
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.
Flowers of the Sky
"Flowers of the Sky" by Richard A. Proctor, originally published in 1879, offers a fascinating glimpse into the popular understanding of astronomy during the late 19th century. Proctor, a renowned astronomer and science communicator, explores the wonders of the celestial sphere, detailing constellations, nebulae, and other astronomical phenomena in a clear and engaging style. This work showcases the knowledge and appreciation of the night sky as it was understood at the time, providing both a historical record of scientific thought and an accessible introduction to the beauty of the universe. A valuable read for anyone interested in the history of science and the enduring appeal of astronomy.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.
Cuneiform Uranology Texts
Presents a newly recovered group of cuneiform texts from first millennium Babylonia and Assyria that provide prose descriptions of the drawing (eseru) of Mesopotamian constellations. Describes these constellations in terms of their parts: body parts for constellations in human or animal form, parts of a wagon for "The Wagon" and "The Wagon of Heaven" (the Big and Little Dipper), and so forth. The descriptions also typically speak of the clothing that constellations in human form wear, their beards if they are male, and paraphernalia that they hold or carry. In the case of "The Crab" and "The Wagon," there is also reference to the Babylonian geometric shape apsamakku, a four-sided figure. Illustrations.
The Mechanism of the Heavens
"The Mechanism of the Heavens" offers a detailed exploration of astronomy and celestial mechanics as understood in the mid-19th century. Written by Denison Olmsted, this book provides insights into the mathematical and physical principles governing the movements of celestial bodies. It is a valuable resource for those interested in the history of science, particularly the evolution of astronomical thought. Olmsted's work reflects the scientific understanding of his time, making it a fascinating read for historians of science and anyone curious about the development of our understanding of the cosmos.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.
An Investigation of Shock Wave Physics via Hybrid CFD-BGK Solution Methods for Nonequilibrium Flows
The Unified Flow Solver, a hybrid continuum-rarefied code, is used to investigate the internal structure of a normal shock wave for a Mach range of 1.55 to 9.0 for Argon, and 1.53 to 3.8 for diatomic Nitrogen. Reciprocal shock thickness, density, temperature, heat flux, and the velocity distribution function are calculated for a one-dimensional shock wave and compared with experimental data from Alsmeyer and DSMC results from Bird. Using the Euler, Navier-Stokes, BGK model, and Three-Temperature BGK model schemes, results from UFS compare well with experiment and DSMC. The Euler scheme shows atypical results, possibly resulting from modifications made to include internal energies. An entropy spot is introduced into a two-dimensional domain to investigate entropy-shock interactions over a range of Knudsen numbers (Kn=0.01, 0.1, and 1.0) for Mach 2.0 in Argon. Previous work on entropy-shock interactions has only been performed using an Euler scheme. Here, results are presented in Argon using coupled BGK and Navier-Stokes solvers. Density, pressure, and temperature profiles, as well as the profiles of their gradients, are reported at certain times after the entropy spot convects through the shock.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.
Heat, Considered as a Mode of Motion; From the Second London Ed., Rev., With Additions Embracing the Author's Latest Researches
Explore the groundbreaking theories of John Tyndall in "Heat, Considered as a Mode of Motion." This edition, revised and expanded from the second London printing, incorporates Tyndall's latest research, providing a comprehensive look at his investigations into the nature of heat. Tyndall, a towering figure in 19th-century science, elucidates his revolutionary ideas linking heat and motion, offering insights that reshaped the understanding of thermodynamics. This work remains a valuable resource for students and scholars interested in the history of physics and the development of thermal science. Delve into the experiments and observations that underpinned Tyndall's conclusions, and trace the evolution of his thinking on this fundamental aspect of the physical world. This classic text offers a unique window into the scientific thought of the Victorian era.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 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.
High-Frequency Stark Effect and its Application to Plasma Diagnostics
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.
An Account of the Salt Springs at Salina
"An Account of the Salt Springs at Salina" by Lewis C. Beck offers a detailed historical and scientific examination of the salt springs located in Salina, New York. Published in 1826, this work provides valuable insights into the geological and chemical properties of these springs, as well as their economic and industrial significance in the early 19th century.Beck's account meticulously describes the process of salt production, the composition of the brine, and the surrounding geological formations. This book serves as a primary source for understanding the early industrial practices and scientific investigations related to natural resources in the United States. It is a must-read for historians, geologists, and anyone interested in the industrial history of New York.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.
Time Dependent Discrete Ordinates Neutron Transport Using Distribution Iteration in XYZ Geometry
The DI algorithm is an alternative to source iteration that, in our testing, does not require an accelerator. I developed a formal verification plan and executed it to verify the results produced by my code that implemented DI with the above features. A new, matrix albedo, boundary condition treatment was developed and implemented so that infinite-medium benchmarks could be included in the verification test suite. The DI algorithm was modified for parallel efficiency and the prior instability of the refinement sweep was corrected. The testing revealed that DI performed as well or faster than source iteration with DSA and that DI continued to work where DSA failed. Performance did degrade when the diamond-difference (without fixup) spatial quadrature was used. Because diamond-difference is a non-positive spatial quadrature, it can produce nonphysical negative fluxes, particularly in higher dimensions. I developed a new fixup scheme to accommodate the negative fluxes, but it did not improve performance in XYZ geometry when the scattering ratio was near unity.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.
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.
Characterization of Neutron-Induced Defects in Isotopically Enriched Lithium Tetraborate
Lithium Tetraborate (LTB) is assessed for use as a material for neutron detection. LTB isotopically enriched in either Li-6 or B-10 provides a medium that efficiently captures and transmutes neutrons into more readily detected forms of material or energy. Neutron detection is desirable to detect elicit movement of special nuclear material or nuclear weapons. Single crystals of LTB, Li-6 or B-10 enriched, were neutron irradiated, and electron paramagnetic resonance was used to detect point defects induced by the neutrons. Multiple defects were noted in the irradiated crystals. Two particular defects, perturbed lithium vacancies and lithium clusters are proposed as induced by thermal neutrons. Parallel experiments on silver doped LTB indicated that fast neutrons induce interstitial defects including interstitial oxygen, lithium, and silver atoms in silver doped crystals. Electron paramagnetic resonance, electron-nuclear double resonance, pulsed anneal, and thermo luminescence studies prior to neutron irradiation concluded that silver doped LTB crystals contain silver point defects that trap both electrons and holes. Pulsed anneal and thermo luminescence studies of all crystal types prior to neutron irradiation suggest neutron induced defects are significantly more stable that as grown defects.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.
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.
To the Sun? a Journey Through Planetary Space
Embark on an extraordinary voyage through the solar system with "To the Sun? a Journey Through Planetary Space," a captivating work attributed to Jules Verne. First conceived in the 19th century, this work invites readers to explore the planets and celestial wonders through the eyes of visionary thinkers. This edition, translated by Edward Roth, captures the spirit of scientific curiosity and imaginative storytelling that defines the era. "To the Sun?" explores themes of scientific discovery, technological innovation, and the boundless human desire to explore the unknown. Experience the thrill of interplanetary travel and the allure of the cosmos in this pioneering work of science fiction that continues to inspire generations.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.
Parameter Studies for a Two-Component Fusion Experiment
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.
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.
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.
Fourier Transform Photoelectron Diffraction and its Application to Molecular Orbitals and Surface Structure
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.
