Suleiman Barkara (6 results)
- Softcover
Seller: preigu, Osnabrück, Germanypreigu
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Taschenbuch. Condition: Neu. Solar Wind-Earth's Magnetosphere Interaction:Halloween Event Modelling | Suleiman Barkara | Taschenbuch | 164 S. | Englisch | 2016 | LAP LAMBERT Academic Publishing | EAN 9783659928109 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[…dot]de | Anbieter: preigu.
- Softcover
Seller: Revaluation Books, Exeter, United KingdomRevaluation Books
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£ 105.57
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Paperback. Condition: Brand New. 164 pages. 8.66x5.91x0.37 inches. In Stock.
Language: English
Published by LAP Lambert Academic Publishing Aug 2016, 2016
- Softcover
- Print on Demand
Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, GermanyBuchWeltWeit Ludwig Meier e.K.
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£ 57.44
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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book describes the interaction between the solar wind and the EArth's magnetic field( magnetosphere). Interplanetary Magnetic Field (IMF) impact on this interaction is essential. Different IMF orientation and their consequentia…l influences on the said interaction were introduced in different chapters. The separation of these effects was meant to see what differences do that make on the driving parameters the solar wind-magnetosphere interaction. Our tool of the study was Particle-In-Cell (PIC), Electromagnetic and Relativistic code. This code was under development for more than three decades, originally written by Oscar Buneman, 1992 at Stanford University, CA, USA. The working version of the code we used, was developed within a framework of Franco-Polish protocol of cooperation. Nowadays, we have a better resolution in terms of grid size and number of particles per cells with real ion to electron mass ratios. The code lately was able to simulate very low energy and density of plasmasphere. 164 pp. Englisch.
- Softcover
- Print on Demand
Seller: moluna, Greven, Germanymoluna
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Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Barkara SuleimanBorn in 1965 in Banisuhaila, Gaza, PalestineWork in Public Relations 11 yearsB.Sc. in Physics Al Quds Univ., Jerusalem 1987Graduate Diploma, Public Admin Penn State, PA,USM.Sc. in Theore…tical Physics, Gaza, 2003PhD i.
Language: English
Published by LAP LAMBERT Academic Publishing Jul 2016, 2016
- Softcover
- Print on Demand
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germanybuchversandmimpf2000
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£ 57.44
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Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -This book describes the interaction between the solar wind and the EArth¿s magnetic field( magnetosphere). Interplanetary Magnetic Field (IMF) impact on this interaction is essential. Different IMF orientation and their consequential in…fluences on the said interaction were introduced in different chapters. The separation of these effects was meant to see what differences do that make on the driving parameters the solar wind-magnetosphere interaction. Our tool of the study was Particle-In-Cell (PIC), Electromagnetic and Relativistic code. This code was under development for more than three decades, originally written by Oscar Buneman, 1992 at Stanford University, CA, USA. The working version of the code we used, was developed within a framework of Franco-Polish protocol of cooperation. Nowadays, we have a better resolution in terms of grid size and number of particles per cells with real ion to electron mass ratios. The code lately was able to simulate very low energy and density of plasmasphere.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 164 pp. Englisch.
- Softcover
- Print on Demand
Seller: AHA-BUCH GmbH, Einbeck, GermanyAHA-BUCH GmbH
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£ 58.13
£ 52.68 shippingShips from Germany to U.S.A.Quantity: 1 available
Taschenbuch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - This book describes the interaction between the solar wind and the EArth's magnetic field( magnetosphere). Interplanetary Magnetic Field (IMF) impact on this interaction is essential. Different IMF orientation and their consequential inf…luences on the said interaction were introduced in different chapters. The separation of these effects was meant to see what differences do that make on the driving parameters the solar wind-magnetosphere interaction. Our tool of the study was Particle-In-Cell (PIC), Electromagnetic and Relativistic code. This code was under development for more than three decades, originally written by Oscar Buneman, 1992 at Stanford University, CA, USA. The working version of the code we used, was developed within a framework of Franco-Polish protocol of cooperation. Nowadays, we have a better resolution in terms of grid size and number of particles per cells with real ion to electron mass ratios. The code lately was able to simulate very low energy and density of plasmasphere.
