9783330023192 - Solar Decametric Radio Emission and Solar Cycle Variations di Halder, Debojyoti (10 risultati)

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Paperback. Condizione: Brand New. 176 pages. 8.66x5.91x0.40 inches. In Stock.

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Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The Sun is one of the first objects studied by the early radio astronomers. In 2009, the Sun has been risen to peak in sunspot number and the related solar activity level. That means there should be a lot of solar flares on the Sun's surface and the Earth should receive a number of geomagnetic storms as a result. So this is an exciting time to begin monitoring the Sun with radio receivers. Solar flares are powered by the sudden release of magnetic energy stored in the corona. The same energy release may produce coronal mass ejections (CME), although the relation between CMEs and solar flares is still not well established. Direct radio emission at decametric wavelengths may disturb the operation of radars and other devices that use those frequencies. The frequency of occurrence of solar flares varies from several per day when the Sun is particularly active to less than one every week when the Sun is quiet, following the 11-year cycle called the solar cycle. When there is a solar flare on the Sun's surface, there is often an accompanying burst of radio energy projected into space. We can monitor these bursts with standard VHF receivers with modest antennas. 176 pp. Englisch.

Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Halder DebojyotiDr. Debojyoti Halder passed his Masters degree from University of Kalyani, India with first class in 2010. He then completed his Doctorate degree in Observational Solar and Planetory Radio Astronomy in the same unive.

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Taschenbuch. Condizione: Neu. Solar Decametric Radio Emission and Solar Cycle Variations | Debojyoti Halder | Taschenbuch | 176 S. | Englisch | 2017 | LAP LAMBERT Academic Publishing | EAN 9783330023192 | Verantwortliche Person für die EU: BoD - Books on Demand, In de Tarpen 42, 22848 Norderstedt, info[at]bod[dot]de | Anbieter: preigu Print on Demand.

Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The Sun is one of the first objects studied by the early radio astronomers. In 2009, the Sun has been risen to peak in sunspot number and the related solar activity level. That means there should be a lot of solar flares on the Sun's surface and the Earth should receive a number of geomagnetic storms as a result. So this is an exciting time to begin monitoring the Sun with radio receivers. Solar flares are powered by the sudden release of magnetic energy stored in the corona. The same energy release may produce coronal mass ejections (CME), although the relation between CMEs and solar flares is still not well established. Direct radio emission at decametric wavelengths may disturb the operation of radars and other devices that use those frequencies. The frequency of occurrence of solar flares varies from several per day when the Sun is particularly active to less than one every week when the Sun is quiet, following the 11-year cycle called the solar cycle. When there is a solar flare on the Sun's surface, there is often an accompanying burst of radio energy projected into space. We can monitor these bursts with standard VHF receivers with modest antennas.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 176 pp. Englisch.

Taschenbuch. Condizione: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The Sun is one of the first objects studied by the early radio astronomers. In 2009, the Sun has been risen to peak in sunspot number and the related solar activity level. That means there should be a lot of solar flares on the Sun's surface and the Earth should receive a number of geomagnetic storms as a result. So this is an exciting time to begin monitoring the Sun with radio receivers. Solar flares are powered by the sudden release of magnetic energy stored in the corona. The same energy release may produce coronal mass ejections (CME), although the relation between CMEs and solar flares is still not well established. Direct radio emission at decametric wavelengths may disturb the operation of radars and other devices that use those frequencies. The frequency of occurrence of solar flares varies from several per day when the Sun is particularly active to less than one every week when the Sun is quiet, following the 11-year cycle called the solar cycle. When there is a solar flare on the Sun's surface, there is often an accompanying burst of radio energy projected into space. We can monitor these bursts with standard VHF receivers with modest antennas.