Dorman, lev (120 risultati)

Lingua: Inglese
Editore: Little, Brown and Company, New York, 2020
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Hardcover. Condizione: Fine. Condizione sovraccoperta: Fine. 1st Edition. Blue cover with silver lettering and a vignette. 26 chapters; b/w illustrations. The front board's front corners are slightly bumped. Scans e-mailed upon request. Tracy Nishimura Bishop; Brandon Dorman (illustratore).
Altre immaginiLingua: Inglese
Editore: Little, Brown Books for Young Readers, 2020
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Da: Cross Genre Books, WEST LINN, OR, U.S.A.Cross Genre Books
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Hardcover. Condizione: Near Fine. Near Fine. 1st Edition. Signed by Author(s). The dust jacket is unclipped ($16.99).10 9 8 7 6 5 4 3 2 1 number line. Signed by the author on the title page. Brandon Dorman, jacket art. Tracy Nishimura Bishop, interior art (illustratore).

Lingua: Inglese
Editore: Dordrecht, Springer Netherland., 2004
Serie: Libro 8 di 228 - Astrophysics and Space Science Library
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16 x 24 cm. XXXII, 862 S. XXXII, 862 p. Hardcover. Versand aus Deutschland / We dispatch from Germany via Air Mail. Einband bestoßen, daher Mängelexemplar gestempelt, sonst sehr guter Zustand. Imperfect copy due to slightly bumped cover, apart from this in very good condition. Stamped. (Astrophysics and Space Science Library). Sprache: Englisch.…
Altre immaginiLingua: Inglese
Editore: Little, Brown Books for Young Readers, 2022
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Soft cover. Condizione: Near Fine. No Jacket as issued. 1st Edition. Signed by Author(s). This book is a Advance Reading Copy of the First Hardcover Edition. 10 9 8 7 6 5 4 3 2 1 number line. Signed by the author on the title page. Brandon Dorman, jacket art. Tracy Nishimura Bishop, interior art (illustratore).…

Lingua: Inglese
Editore: Springer, 2010
Serie: Libro 47 di 228 - Astrophysics and Space Science Library
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Condizione: Good. Your purchase helps support Sri Lankan Children's Charity 'The Rainbow Centre'. Ex-library, so some stamps and wear, but in good overall condition. Our donations to The Rainbow Centre have helped provide an education and a safe haven to hundreds of children who live in appalling conditions.…

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Condizione: Good. Your purchase helps support Sri Lankan Children's Charity 'The Rainbow Centre'. Ex-library, so some stamps and wear, but in good overall condition. Our donations to The Rainbow Centre have helped provide an education and a safe haven to hundreds of children who live in appalling conditions.…

Lingua: Inglese
Editore: Springer, 2006
Serie: Libro 32 di 228 - Astrophysics and Space Science Library
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Da: Phatpocket Limited, Waltham Abbey, HERTS, Regno UnitoPhatpocket Limited
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Condizione: Good. Your purchase helps support Sri Lankan Children's Charity 'The Rainbow Centre'. Ex-library, so some stamps and wear, but in good overall condition. Our donations to The Rainbow Centre have helped provide an education and a safe haven to hundreds of children who live in appalling conditions.…

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Condizione: New. This is a Brand-new US Edition. This Item may be shipped from US or any other country as we have multiple locations worldwide.

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Altre immaginiLingua: Inglese
Editore: Springer, 2016
Serie: Libro 32 di 228 - Astrophysics and Space Science Library
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Taschenbuch. Condizione: Neu. Cosmic Ray Interactions, Propagation, and Acceleration in Space Plasmas | Lev Dorman | Taschenbuch | Astrophysics and Space Science Library | xxxiii | Englisch | 2016 | Springer | EAN 9789402404531 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. …

Lingua: Inglese
Editore: Springer Netherlands, 2014
Serie: Libro 8 di 228 - Astrophysics and Space Science Library
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Da: Buchpark, Trebbin, GermaniaBuchpark
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Condizione: Hervorragend. Zustand: Hervorragend | Seiten: 896 | Sprache: Englisch | Produktart: Bücher | The present monograph as well as the next one (Dorman, M2005) is a result of more than 50 years working in cosmic ray (CR) research. After graduation in December 1950 Moscow Lomonosov State University (Nuclear and Elementary Particle Physics Division, the Team of Theoretical Physics), my supervisor Professor D. I. Blokhintsev planned for me, as a winner of a Red Diploma, to continue my education as an aspirant (a graduate student) to prepare for Ph. D. in his very secret Object in the framework of what was in those time called the Atomic Problem. To my regret the KGB withheld permission, and I, together with other Jewish students who had graduated Nuclear Divisions of Moscow and Leningrad Universities and Institutes, were faced with a real prospect of being without any work. It was our good fortune that at that time there was being brought into being the new Cosmic Ray Project (what at that time was also very secret, but not as secret as the Atomic Problem), and after some time we were directed to work on this Project. It was organized and headed by Prof. S. N. Vernov (President of All-Union Section of Cosmic Rays) and Prof. N. V. Pushkov (Director of IZMIRAN); Prof. E. L. Feinberg headed the theoretical part of the Project.…

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Hardcover. Condizione: new. Hardcover. The importance and actuality of the Geomagnetosphere's research are based on following three factors: 1. The Geomagnetosphere is the nearest giant natural Laboratory, where is possible by a lot of satellites and ground measurements investigate in details many different plasmas and energetic processes in space, caused finally by interaction of high kinetic energy solar wind plasmas and its perturbations (Interplanetary Coronal Mass Ejections - ICMEs, Interplanetary Shock Waves - ISWs, Interplanetary Interaction Regions - IIR) with frozen in Interplanetary Magnetic Fields - IMF with the rotated main geomagnetic field. This interaction leads to dynamic transformation magnetic fields in Geomagnetosphere, generation and trapping high energy particles (which can be called as Magnetospheric Cosmic Rays - MCR), generation of many types instabilities and electromagnetic radiations. These processes are in principle similar to processes in magnetospheres of other planets and their moons, in the atmosphere of the Sun and other stars, in interplanetary and in interstellar space, in many different astrophysical objects, i.e. this research is important basis for fundamental Space and Astrophysical science. 2. In the modern time the Technology, Economics, Navigation, TV, Internet, Radio-Connections, Military aspects, and the life of people on our planet are strong connected with the work of many satellites, moving inside the Geomagnetosphere. Different processes and MCR in the Geomagnetosphere influenced on the satellites work and often lead to satellite malfunctions up to full destroying work of their electronics - satellites became 'dead'. The described research can be considered as basis for developing methods of forecasting dangerous situation for satellites on different orbits and to decrease the risk of satellite malfunctions and loosing, i.e. this research has important practical application. 3. The interaction of ICME, ISW, and IIR with Geomagnetosphere leads to generation big magnetic storms accompanied with Forbushdecreases and precursory effects in Galactic Cosmic Ray (GCR) intensity. These magnetic storms are dangerous not only for satellites, but also on the Earth's surface for technology, radio-connections, car accidents, people health (e.g., increasing frequency of infarct myocardial and brain strokes). Investigations of causes of magnetic storms can help to develop methods of their forecasting and decreasing the level of magnetic storms hazards. Therefore, the other practical application of this research is connected with the problem of space weather and space climate influence on the technology, radio-connections, navigation, transportation, and people health on the Earth in dependence of altitude and geomagnetic latitude. The present book "Energetic Particles in Geomagnetosphere/Ionosphere" contains the following Chapters: Chapter 1. Experimental Evidences on Energetic Particles in the Earth's Environment Chapter 2. Theories/Models/Simulations of Energetic Particles Acceleration and Propagation in the Geomagnetosphere Chapter 3. Energetic Particles in Geomagnetosphere and Ionosphere: Related Phenomena Chapter 4. Auroras and Magnetospheric/Ionospheric Acceleration Processes Chapter 5. Magnetospheric/Ionospheric Acceleration and Propagation Processesat High-Latitudes and in Polar Regions We hope that this review-book will be interesting and useful for researches, engineers, students of corresponding specialties, and all people interested in developing of modern technologies in space and in problems of Geomagnetosphere, Ionosphere, Upper and Low Atmosphere, Space Weather and Space Climate, and how they influence on the Earth's Civilization. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.…

Lingua: Inglese
Editore: Springer, 2016
Serie: Libro 47 di 228 - Astrophysics and Space Science Library
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Lingua: Inglese
Editore: Springer, 2016
Serie: Libro 32 di 228 - Astrophysics and Space Science Library
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Lingua: Inglese
Editore: Springer, 2010
Serie: Libro 47 di 228 - Astrophysics and Space Science Library
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Lingua: Inglese
Editore: Springer, 2006
Serie: Libro 32 di 228 - Astrophysics and Space Science Library
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Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The problem of cosmic ray (CR) geomagnetic effects came to the fore at the beg- ning of the 1930s after the famous expeditions by J. Clay onboard ship (Slamat) between the Netherlands and Java using an ionization chamber. Many CR la- tude expeditions were organized by the famous scientists and Nobel Laureates R. Millikan and A. Compton. From the obtained latitude curves it follows that CRs cannot be gamma rays (as many scientists thought at that time), but must be charged particles. From measurements of azimuthally geomagnetic effect at that time it also followed that these charged particles must be mostly positive (see Chapter 1, and for more details on the history of the problem see monographs of Irina Dorman, M1981, M1989). The rst explanations of obtained results were based on the simple dipole - proximation of the geomagnetic eld and the theory of energetic charged particles moving in dipole magnetic elds, developed in 1907 by C. Stormer to explain the aurora phenomenon. Let us note that it was made about 5 years before V. Hess discovered CRs, and received the Nobel Prize in 1936 together with K. Anderson (for the discovery of CR and positrons in CR).…

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Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The problem of cosmic ray (CR) geomagnetic effects came to the fore at the beg- ning of the 1930s after the famous expeditions by J. Clay onboard ship (Slamat) between the Netherlands and Java using an ionization chamber. Many CR la- tude expeditions were organized by the famous scientists and Nobel Laureates R. Millikan and A. Compton. From the obtained latitude curves it follows that CRs cannot be gamma rays (as many scientists thought at that time), but must be charged particles. From measurements of azimuthally geomagnetic effect at that time it also followed that these charged particles must be mostly positive (see Chapter 1, and for more details on the history of the problem see monographs of Irina Dorman, M1981, M1989). The rst explanations of obtained results were based on the simple dipole - proximation of the geomagnetic eld and the theory of energetic charged particles moving in dipole magnetic elds, developed in 1907 by C. Stormer to explain the aurora phenomenon. Let us note that it was made about 5 years before V. Hess discovered CRs, and received the Nobel Prize in 1936 together with K. Anderson (for the discovery of CR and positrons in CR). …

Lingua: Inglese
Editore: Springer, 2016
Serie: Libro 32 di 228 - Astrophysics and Space Science Library
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Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - xxii CONTENTS In 1957 I was invited to work on special problems in Magnetic Laboratory of the Academy of Sciences of USSR as a Head of Department of Magnetic Hydrodynamics. In few years this Laboratory was transfered into the I. V. Kurchatov Institute of Atomic Energy, and I continued to work in this Institute up to 1965. In parallel I also worked at Moscow State University as Professor in the CR and Space Research Team. I also gave lectures in Irkutsk, Alma-Ata, Nalchik, Tbilisi, Erevan, Samarkand, and others places. Over about 40 years of teaching under my supervision more than hundred graduate students and scientists in USSR and some other countries gained their Ph. D. and several tenths became Doctors of Science. As my hobby I continued to work in CR research, and as Vice-President of All-Union Section of Cosmic Rays and Radiation Belts, took an active part in preparing the Soviet net of CR stations to the IGY (International Geophysical Year, 1957-1958): we equipped all soviet stations in USSR and in Antarctica with standard cubic and semi-cubic muon telescopes and with neutron monitors of IGY (or Simpson's) type. In connection with preparing for the IQSY (the International Quiet Sun Year, 1964-1965), the soviet net of CR stations was extended about two fold and they were equipped with neutron super-monitors of IQSY type (with an effective surface about 10 times bigger than the previous monitor of IGY type).…

Lingua: Inglese
Editore: Springer, 2016
Serie: Libro 47 di 228 - Astrophysics and Space Science Library
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Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - Short Historical Overview In the 1940s, two phenomena in the eld of cosmic rays (CR) forced scientists to think that the Sun is a powerful source of high-energy particles. One of these was discovered because of the daily solar variation of CR, which the maximum number of CR observed near noon (referring to the existence of continuous ux of CR from the direction of the Sun); this became the experimental basis of the theory that CR's originate from the Sun (or, for that matter, from within the solar system) (Alfven 1954). The second phenomenon was discovered when large uxes of high energy particles were detected from several solar ares, or solar CR. These are the - called ground level events (GLE), and were rst observed by ionization chambers shielded by 10 cm Pb (and detected mainly from the secondary muon-component CR that they caused) during the events of the 28th of February 1942, the 7th of March 1942, the 25th of July 1946, and the 19th of November 1949. The biggest such event was detected on the 23rd of February 1956 (see the detailed description in Chapters X and XI of Dorman, M1957). The rst phenomenon was investigated in detail in Dorman (M1957), by rst correcting experimental data on muon temperature effects and then by using coupling functions to determine the change in particle energy caused by the solar-diurnal CR variation.…

Lingua: Inglese
Editore: Springer, 2010
Serie: Libro 47 di 228 - Astrophysics and Space Science Library
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Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - Short Historical Overview In the 1940s, two phenomena in the eld of cosmic rays (CR) forced scientists to think that the Sun is a powerful source of high-energy particles. One of these was discovered because of the daily solar variation of CR, which the maximum number of CR observed near noon (referring to the existence of continuous ux of CR from the direction of the Sun); this became the experimental basis of the theory that CR's originate from the Sun (or, for that matter, from within the solar system) (Alfven 1954). The second phenomenon was discovered when large uxes of high energy particles were detected from several solar ares, or solar CR. These are the - called ground level events (GLE), and were rst observed by ionization chambers shielded by 10 cm Pb (and detected mainly from the secondary muon-component CR that they caused) during the events of the 28th of February 1942, the 7th of March 1942, the 25th of July 1946, and the 19th of November 1949. The biggest such event was detected on the 23rd of February 1956 (see the detailed description in Chapters X and XI of Dorman, M1957). The rst phenomenon was investigated in detail in Dorman (M1957), by rst correcting experimental data on muon temperature effects and then by using coupling functions to determine the change in particle energy caused by the solar-diurnal CR variation.…