Debojyoti halder (87 résultats)

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

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Taschenbuch. Etat : Neu. Astronomical Studies on SETI | Debojyoti Halder (u. a.) | Taschenbuch | Englisch | 2025 | KS Omniscriptum Publishing | EAN 9786208426378 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu. …

Taschenbuch. Etat : Neu. Cometary Impacts on Jovian Magnetosphere | Some studies on the plasma processes in the Jovian magnetosphere and Cometary Impacts on it. | Debojyoti Halder (u. a.) | Taschenbuch | Englisch | 2024 | LAP LAMBERT Academic Publishing | EAN 9786207843268 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu.…

paperback. Etat : New. NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

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Taschenbuch. Etat : Neu. Émission radio décamétrique du soleil et variations du cycle solaire | Debojyoti Halder | Taschenbuch | Französisch | 2023 | Editions Notre Savoir | EAN 9786206421399 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu. …

Taschenbuch. Etat : Neu. Impacts cométaires sur la magnétosphère jovienne | Quelques études sur les processus plasmatiques dans la magnétosphère jovienne et les impacts cométaires sur celle-ci | Debojyoti Halder (u. a.) | Taschenbuch | Französisch | 2024 | Editions Notre Savoir | EAN 9786208177126 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu.…

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Taschenbuch. Etat : Neu. Emissione radio decametrica solare e variazioni del ciclo solare | Debojyoti Halder | Taschenbuch | Italienisch | 2023 | Edizioni Sapienza | EAN 9786206421412 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu. …

Taschenbuch. Etat : Neu. Emissão Rádio Decamétrica Solar e Variações do Ciclo Solar | Debojyoti Halder | Taschenbuch | Portugiesisch | 2023 | Edições Nosso Conhecimento | EAN 9786206421429 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu. …

Taschenbuch. Etat : Neu. Dekametrische Radioemission der Sonne und Variationen des Sonnenzyklus | Debojyoti Halder | Taschenbuch | 140 S. | Deutsch | 2023 | Verlag Unser Wissen | EAN 9786206421382 | Verantwortliche Person für die EU: BoD - Books on Demand, In de Tarpen 42, 22848 Norderstedt, info[at]bod[dot]de | Anbieter: preigu. …

Taschenbuch. Etat : Neu. Impatti cometari sulla magnetosfera gioviana | Alcuni studi sui processi di plasma nella magnetosfera gioviana e sugli impatti cometari su di essa | Debojyoti Halder (u. a.) | Taschenbuch | Einband - flex.(Paperback) | Italienisch | 2024 | Edizioni Sapienza | EAN 9786208177133 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu.…

Taschenbuch. Etat : Neu. Impactos Cometários na Magnetosfera Joviana | Alguns estudos sobre os processos de plasma na magnetosfera Joviana e os Impactos Cometários na mesma | Debojyoti Halder (u. a.) | Taschenbuch | Einband - flex.(Paperback) | Portugiesisch | 2024 | Edições Nosso Conhecimento | EAN 9786208177096 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu.…

Taschenbuch. Etat : Neu. Kometeneinschläge auf die Jovianische Magnetosphäre | Einige Studien über die Plasmaprozesse in der jovianischen Magnetosphäre und Kometeneinschläge darauf | Debojyoti Halder (u. a.) | Taschenbuch | 320 S. | Deutsch | 2024 | Verlag Unser Wissen | EAN 9786208177102 | Verantwortliche Person für die EU: SIA OmniScriptum Publishing, Brivibas Gatve 197, 1039 RIGA, LETTLAND, customerservice[at]vdm-vsg[dot]de | Anbieter: preigu.…

Taschenbuch. Etat : 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.…

PAP. Etat : New. New Book. Shipped from UK. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.

PAP. Etat : New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.

PAP. Etat : New. New Book. Shipped from UK. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.

PAP. Etat : New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.

Taschenbuch. Etat : 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.…

Etat : 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.…

Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -El Sol es uno de los primeros objetos estudiados por los primeros radioastrónomos. En 2009, el Sol ha alcanzado su máximo número de manchas solares y el nivel de actividad solar correspondiente. Eso significa que debería haber una gran cantidad de erupciones solares en la superficie del Sol y la Tierra debería recibir una serie de tormentas geomagnéticas como resultado. Por tanto, es un buen momento para empezar a vigilar el Sol con receptores de radio. Las erupciones solares se producen por la liberación repentina de energía magnética almacenada en la corona. La misma liberación de energía puede producir eyecciones de masa coronal (CME), aunque la relación entre las CME y las erupciones solares aún no está bien establecida. La emisión directa de radio en longitudes de onda decamétricas puede perturbar el funcionamiento de radares y otros dispositivos que utilizan esas frecuencias. La frecuencia de aparición de las erupciones solares varía desde varias al día cuando el Sol está particularmente activo hasta menos de una cada semana cuando el Sol está en calma, siguiendo el ciclo de 11 años denominado ciclo solar. Cuando se produce una erupción solar en la superficie del Sol, a menudo va acompañada de un estallido de energía de radio proyectada hacia el espacio. Podemos monitorizar estos estallidos con receptores VHF estándar con antenas modestas. 128 pp. Spanisch.…