Isbn: 9781118842348 - magnetotails in the solar system (17 risultati)

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  • Lingua: Inglese

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    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Editore: John Wiley & Sons 2015-03-24, 2015

    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Editore: American Geophysical Union 2015-02-16, 2015

    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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  • Lingua: Inglese

    Editore: American Geophysical Union, 2015

    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Hardback. Condizione: New. All magnetized planets in our solar system (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) interact strongly with the solar wind and possess well developed magnetotails. It is not only the strongly magnetized planets that have magnetotails. Mars and Venus have no global intrinsic magnetic field, yet they possess induced magnetotails. Comets have magnetotails that are formed by the draping of the interplanetary magnetic field. In the case of planetary  satellites (moons), the magnetotail refers to the wake region behind the satellite in the flow of either the solar wind or the magnetosphere of its parent planet. The largest magnetotail of all in our solar  system  is  the  heliotail,  the  "magnetotail" of  the heliosphere. The variety of solar wind conditions, planetary rotation rates, ionospheric conductivity, and physical dimensions provide an outstanding opportunity to extend our understanding of the influence of these factors on magnetotail processes and structures.  Volume highlights include:  Discussion on why a magnetotail is a fundamental problem of magnetospheric physicsUnique collection of tutorials on a large range of magnetotails in our solar systemIn-depth reviews comparing magnetotail processes at Earth with other magnetotail structures found throughout the heliosphere Collectively, Magnetotails in the Solar System brings together for the first time in one book a collection of tutorials and current developments addressing different types of magnetotails. As a result, this book should appeal to a broad community of space scientists, and it should also be of interest to astronomers who are looking at tail-like structures beyond our solar system.

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    Editore: American Geophysical Union, 2015

    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Serie: Libro 179 di 266 - Geophysical Monograph

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    Serie: Libro 179 di 266 - Geophysical Monograph

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    Condizione: New. All magnetized planets in our solar system interact strongly with the solar wind and possess well developed magneto tails. This book includes a discussion of why a magnetotail is a fundamental issue in magneto spheric physics. It is a collection of tutorials that cover a large range of magneto tails in our solar system; and more. Editor(s): Keiling, Andreas; Jackman, Caitriona; Delamere, Peter. Series: Geophysical Monograph Series. Num Pages: 424 pages. BIC Classification: PGS; PHK. Category: (P) Professional & Vocational. Dimension: 288 x 225 x 26. Weight in Grams: 1378. . 2015. 1st Edition. Hardcover. . . . .

  • Lingua: Inglese

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    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Hardcover. Condizione: Brand New. 1st edition. 424 pages. 12.00x9.00x1.00 inches. In Stock.

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    Serie: Libro 179 di 266 - Geophysical Monograph

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    Gebunden. Condizione: New. All magnetized planets in our solar system (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) interact strongly with the solar wind and possess well developed magnetotails. However, Mars and Venus have no global intrinsic magnetic field, yet they posses.

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    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Condizione: New. All magnetized planets in our solar system interact strongly with the solar wind and possess well developed magneto tails. This book includes a discussion of why a magnetotail is a fundamental issue in magneto spheric physics. It is a collection of tutorials that cover a large range of magneto tails in our solar system; and more. Editor(s): Keiling, Andreas; Jackman, Caitriona; Delamere, Peter. Series: Geophysical Monograph Series. Num Pages: 424 pages. BIC Classification: PGS; PHK. Category: (P) Professional & Vocational. Dimension: 288 x 225 x 26. Weight in Grams: 1378. . 2015. 1st Edition. Hardcover. . . . . Books ship from the US and Ireland.

  • Lingua: Inglese

    Editore: John Wiley and Sons Inc, US, 2015

    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Hardback. Condizione: New. All magnetized planets in our solar system (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) interact strongly with the solar wind and possess well developed magnetotails. It is not only the strongly magnetized planets that have magnetotails. Mars and Venus have no global intrinsic magnetic field, yet they possess induced magnetotails. Comets have magnetotails that are formed by the draping of the interplanetary magnetic field. In the case of planetary  satellites (moons), the magnetotail refers to the wake region behind the satellite in the flow of either the solar wind or the magnetosphere of its parent planet. The largest magnetotail of all in our solar  system  is  the  heliotail,  the  "magnetotail" of  the heliosphere. The variety of solar wind conditions, planetary rotation rates, ionospheric conductivity, and physical dimensions provide an outstanding opportunity to extend our understanding of the influence of these factors on magnetotail processes and structures.  Volume highlights include:  Discussion on why a magnetotail is a fundamental problem of magnetospheric physicsUnique collection of tutorials on a large range of magnetotails in our solar systemIn-depth reviews comparing magnetotail processes at Earth with other magnetotail structures found throughout the heliosphere Collectively, Magnetotails in the Solar System brings together for the first time in one book a collection of tutorials and current developments addressing different types of magnetotails. As a result, this book should appeal to a broad community of space scientists, and it should also be of interest to astronomers who are looking at tail-like structures beyond our solar system.

  • Lingua: Inglese

    Editore: John Wiley & Sons Inc Mär 2015, 2015

    1118842340 / 9781118842348

    Serie: Libro 179 di 266 - Geophysical Monograph

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    Buch. Condizione: Neu. Neuware - All magnetized planets in our solar system (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) interact strongly with the solar wind and possess well developed magnetotails. It is not only the strongly magnetized planets that have magnetotails. Mars and Venus have no global intrinsic magnetic field, yet they possess induced magnetotails. Comets have magnetotails that are formed by the draping of the interplanetary magnetic field. In the case of planetary satellites (moons), the magnetotail refers to the wake region behind the satellite in the flow of either the solar wind or the magnetosphere of its parent planet. The largest magnetotail of all in our solar system is the heliotail, the 'magnetotail' of the heliosphere. The variety of solar wind conditions, planetary rotation rates, ionospheric conductivity, and physical dimensions provide an outstanding opportunity to extend our understanding of the influence of these factors on magnetotail processes and structures.Volume highlights include:\* Discussion on why a magnetotail is a fundamental problem of magnetospheric physics\* Unique collection of tutorials on a large range of magnetotails in our solar system\* In-depth reviews comparing magnetotail processes at Earth with other magnetotail structures found throughout the heliosphereCollectively, Magnetotails in the Solar System brings together for the first time in one book a collection of tutorials and current developments addressing different types of magnetotails. As a result, this book should appeal to a broad community of space scientists, and it should also be of interest to astronomers who are looking at tail-like structures beyond our solar system.