A. Balogh – författare
Visar alla böcker från författaren A. Balogh. Handla med fri frakt och snabb leverans.
22 produkter
Mercury
Av A. Balogh, Leonid Ksanfomality m. fl.
Inbunden, 2008
1637 kr
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Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book …
Mercury
Av Rudolf von Steiger, Leonid Ksanfomality m. fl.
E-bok, 2008
2111 kr
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Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book …
Comparative Aeronomy
Av Andrew F. Nagy, A. Balogh m. fl.
Inbunden, 2009
1637 kr
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Andrew F. Nagy Originally published in the journal Space Science Reviews, Volume 139, Nos 1–4. DOI: 10. 1007/s11214-008-9353-0 © Springer Science+Business Media B. V. 2008 Keywords Aeronomy The term “aeronomy” has been used widely for many decades, but its origin has mostly been lost over the …
Comparative Aeronomy
Av Ingo Muller-Wodarg, Michael Mendillo m. fl.
E-bok, 2008
2049 kr
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Andrew F. Nagy Originally published in the journal Space Science Reviews, Volume 139, Nos 1–4. DOI: 10. 1007/s11214-008-9353-0 © Springer Science+Business Media B. V. 2008 Keywords Aeronomy The term “aeronomy” has been used widely for many decades, but its origin has mostly been lost over the …
Corotating Interaction Regions
Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Av Andre Balogh, A. Balogh m. fl.
Inbunden, 2000
1637 kr
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A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. …
Origin and Dynamics of Solar Magnetism
Av M.J. Thompson, A. Balogh m. fl.
Inbunden, 2009
1095 kr
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Starting in 1995 numerical modeling of the Earth’s dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of …
Origin and Dynamics of Solar Magnetism
Av J.-P. Zahn, S.K. Solanki m. fl.
E-bok, 2009
1459 kr
Lägg i varukorg
Starting in 1995 numerical modeling of the Earth’s dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of …
Mercury
Av A. Balogh, Leonid Ksanfomality m. fl.
Häftad, 2010
1639 kr
Lägg i varukorg
Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book …
Comparative Aeronomy
Av Andrew F. Nagy, A. Balogh m. fl.
Häftad, 2010
1639 kr
Lägg i varukorg
Andrew F. Nagy Originally published in the journal Space Science Reviews, Volume 139, Nos 1–4. DOI: 10. 1007/s11214-008-9353-0 © Springer Science+Business Media B. V. 2008 Keywords Aeronomy The term “aeronomy” has been used widely for many decades, but its origin has mostly been lost over the …
Planetary Magnetism
Av U.R. Christensen, A. Balogh m. fl.
Inbunden, 2010
2183 kr
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The articles in this volume cover, for the first time, all aspects of planetary magnetism, from the observations made by space missions to their interpretation in terms of the properties of all the planets in the solar system. Studies of dynamo-generated magnetic fields in Mercury, the Earth, the …
Terrestrial Magnetism
Inbunden, 2011
1639 kr
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The articles in this volume provide a detailed review of all aspects of the main magnetic field of the Earth produced within the Earth’s core: its past history, its long and short term changes, the way it is generated. The book contains the combined knowledge of geomagnetism coming from …
Origin and Dynamics of Solar Magnetism
Av M.J. Thompson, A. Balogh m. fl.
Häftad, 2011
1095 kr
Lägg i varukorg
Starting in 1995 numerical modeling of the Earth’s dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of …
Planetary Magnetism
Av U.R. Christensen, A. Balogh m. fl.
Häftad, 2012
2183 kr
Lägg i varukorg
The articles in this volume cover, for the first time, all aspects of planetary magnetism, from the observations made by space missions to their interpretation in terms of the properties of all the planets in the solar system. Studies of dynamo-generated magnetic fields in Mercury, the Earth, the …
Terrestrial Magnetism
Häftad, 2014
1639 kr
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The articles in this volume provide a detailed review of all aspects of the main magnetic field of the Earth produced within the Earth’s core: its past history, its long and short term changes, the way it is generated. The book contains the combined knowledge of geomagnetism coming from …
Strongest Magnetic Fields in the Universe
Av Vasily S. Beskin, A. Balogh m. fl.
Inbunden, 2016
1639 kr
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This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, in …
Strongest Magnetic Fields in the Universe
Av R.A. Treumann, Tsvi Piran m. fl.
E-bok, 2016
2065 kr
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This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, in …
Strongest Magnetic Fields in the Universe
Av Vasily S. Beskin, A. Balogh m. fl.
Häftad, 2018
1639 kr
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This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, in …
Heliosphere through the Solar Activity Cycle
Av A. Balogh, Louis J. Lanzerotti m. fl.
Inbunden, 2007
1095 kr
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Understanding how the Sun changes though its 11-year sunspot cycle and how these changes affect the vast space around the Sun – the heliosphere – has been one of the principal objectives of space research since the advent of the space age. This book presents the evolution of the heliosphere through …
Heliosphere through the Solar Activity Cycle
Av Steve T. Suess, Louis J. Lanzerotti m. fl.
E-bok, 2007
1416 kr
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Understanding how the Sun changes though its 11-year sunspot cycle and how these changes affect the vast space around the Sun – the heliosphere – has been one of the principal objectives of space research since the advent of the space age. This book presents the evolution of the heliosphere through …
Heliosphere through the Solar Activity Cycle
Av A. Balogh, Louis J. Lanzerotti m. fl.
Häftad, 2010
1095 kr
Lägg i varukorg
Understanding how the Sun changes though its 11-year sunspot cycle and how these changes affect the vast space around the Sun – the heliosphere – has been one of the principal objectives of space research since the advent of the space age. This book presents the evolution of the heliosphere through …
Corotating Interaction Regions
Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Av A. Balogh, J.T. Gosling m. fl.
Häftad, 2010
1639 kr
Lägg i varukorg
A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. …
Corotating Interaction Regions
Proceedings of an ISSI Workshop 6–13 June 1998, Bern, Switzerland
Av H. Kunow, R. Kallenbach m. fl.
E-bok, 2013
2111 kr
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A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. …
