Nagaraju krishnappa (6 Ergebnisse)

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  • Sprache: Englisch

    Verlag: LAP LAMBERT Academic Publishing, 2010

    383837004X / 9783838370040

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    Taschenbuch. Zustand: Neu. Spectropolarimetry of Active Regions on the Sun | Magnetic Coupling Between the Photosphere and Chromosphere | Nagaraju Krishnappa | Taschenbuch | 144 S. | Englisch | 2010 | LAP LAMBERT Academic Publishing | EAN 9783838370040 | Verantwortliche Person für die EU: BoD - Books on Demand, In de Tarpen 42, 22848 Norderstedt, info[at]bod[dot]de | Anbieter: preigu. …

  • Sprache: Englisch

    Verlag: LAP LAMBERT Academic Publishing, 2010

    383837004X / 9783838370040

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    paperback. Zustand: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

  • Sprache: Englisch

    Verlag: LAP LAMBERT Academic Publishing Jun 2010, 2010

    383837004X / 9783838370040

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    Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, DeutschlandBuchWeltWeit Ludwig Meier e.K.

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    Taschenbuch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The upper layers of the solar atmosphere, namely the chromosphere and corona are hotter than the photosphere. This is against the second law of thermodynamics which, in simple words, states that the temperature decreases as one moves away from the heat source, which is every body's common experience. In that case, how these upper layers of solar atmosphere are heated to such high temperatures is a million dollar question. The magnetic field seems to be central to this problem. Apart from many other problems in solar physics, magnetic field on the sun is at the heart of space weather prediction which is governed by the solar activity. Hence the measurement of the magnetic field simultaneously at various heights is important. For this purpose multiline spectropolarimetry is a powerful observational technique. This thesis is about understanding the magnetic coupling between the photosphere and chromosphere above sunspots through multiline spectropolarimetry. 144 pp. Englisch.…

  • Sprache: Englisch

    Verlag: LAP LAMBERT Academic Publishing, 2010

    383837004X / 9783838370040

    • Softcover
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    Anbieter: AHA-BUCH GmbH, Einbeck, DeutschlandAHA-BUCH GmbH

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    Taschenbuch. Zustand: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The upper layers of the solar atmosphere, namely the chromosphere and corona are hotter than the photosphere. This is against the second law of thermodynamics which, in simple words, states that the temperature decreases as one moves away from the heat source, which is every body's common experience. In that case, how these upper layers of solar atmosphere are heated to such high temperatures is a million dollar question. The magnetic field seems to be central to this problem. Apart from many other problems in solar physics, magnetic field on the sun is at the heart of space weather prediction which is governed by the solar activity. Hence the measurement of the magnetic field simultaneously at various heights is important. For this purpose multiline spectropolarimetry is a powerful observational technique. This thesis is about understanding the magnetic coupling between the photosphere and chromosphere above sunspots through multiline spectropolarimetry.…

  • Sprache: Englisch

    Verlag: LAP LAMBERT Academic Publishing, 2010

    383837004X / 9783838370040

    • Softcover
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    Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Krishnappa NagarajuA postdoctoral fellow at the Max-Planck Institute for Solar System Research, Germany. Doctoral thesis work was carried out at the Indian Institute of Astrophysics, Bangalore and the PhD degree was awarded by the Ma.…

  • Sprache: Englisch

    Verlag: LAP LAMBERT Academic Publishing Jun 2010, 2010

    383837004X / 9783838370040

    • Softcover
    • Print-on-Demand

    Anbieter: buchversandmimpf2000, Emtmannsberg, BAYE, Deutschlandbuchversandmimpf2000

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    Taschenbuch. Zustand: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The upper layers of the solar atmosphere, namely the chromosphere and corona are hotter than the photosphere. This is against the second law of thermodynamics which, in simple words, states that the temperature decreases as one moves away from the heat source, which is every body''s common experience. In that case, how these upper layers of solar atmosphere are heated to such high temperatures is a million dollar question. The magnetic field seems to be central to this problem. Apart from many other problems in solar physics, magnetic field on the sun is at the heart of space weather prediction which is governed by the solar activity. Hence the measurement of the magnetic field simultaneously at various heights is important. For this purpose multiline spectropolarimetry is a powerful observational technique. This thesis is about understanding the magnetic coupling between the photosphere and chromosphere above sunspots through multiline spectropolarimetry.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 144 pp. Englisch.…