Paperback. Condition: Very Good. No Jacket. May have limited writing in cover pages. Pages are unmarked. ~ ThriftBooks: Read More, Spend Less.
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Seller: California Books, Miami, FL, U.S.A.
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Published by New India Publishing Agency, 2025
ISBN 10: 9358876050 ISBN 13: 9789358876055
Language: English
Seller: Majestic Books, Hounslow, United Kingdom
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Published by New India Publishing Agency, 2025
ISBN 10: 9358876050 ISBN 13: 9789358876055
Language: English
Seller: Biblios, Frankfurt am main, HESSE, Germany
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Seller: Ria Christie Collections, Uxbridge, United Kingdom
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Published by Notion Press 2021-03-04, 2021
ISBN 10: 1648506933 ISBN 13: 9781648506932
Language: English
Seller: Chiron Media, Wallingford, United Kingdom
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Published by Satish Serial Publishing House, 2019
ISBN 10: 9388020464 ISBN 13: 9789388020466
Language: English
Seller: Books Puddle, New York, NY, U.S.A.
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Published by Satish Serial Publishing House, 2019
ISBN 10: 9388020464 ISBN 13: 9789388020466
Language: English
Seller: Majestic Books, Hounslow, United Kingdom
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Add to basketHardcover. Condition: New. ISBN:9789358876055.
Published by Satish Serial Publishing House, 2019
ISBN 10: 9388020464 ISBN 13: 9789388020466
Language: English
Seller: Biblios, Frankfurt am main, HESSE, Germany
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Published by LAP LAMBERT Academic Publishing, 2021
ISBN 10: 6204728822 ISBN 13: 9786204728827
Language: English
Seller: Books Puddle, New York, NY, U.S.A.
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Published by GRIN Verlag Jan 2024, 2024
ISBN 10: 3964879665 ISBN 13: 9783964879660
Language: English
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
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Add to basketTaschenbuch. Condition: Neu. Neuware -Scientific Study from the year 2024 in the subject Physics - Astronomy, , language: English, abstract: An investigation has been made to study the cosmic-ray decreases occurring during 2006 with respect to the arrival times of interplanetary shocks and magnetic clouds. We have identified three interplanetary magnetic cloud events during 5 February 2006, 13 April 2006 and 14 April 2006. The interplanetary magnetic field (B), north-south component of interplanetary magnetic field (Bz), solar wind velocity, sunspot number (R) and disturbance storm time index (Dst) associated with these events has been studied in the present work. Data (neutron monitor count rate) from Newark Neutron Monitor 9NM64 has been used. The north-south component of IMF (Bz) produce large geomagnetic disturbance on the onset of interplanetary magnetic clouds. The deviations in the interplanetary and solar wind plasma parameters are significantly correlated to the magnetic cloud events. The increase in Dst index, sunspot number (R) and Bz after the magnetic cloud event produces increase in cosmic ray intensity.Books on Demand GmbH, Überseering 33, 22297 Hamburg 20 pp. Englisch.
Published by GRIN Verlag Dez 2023, 2023
ISBN 10: 3346988503 ISBN 13: 9783346988508
Language: English
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
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Add to basketTaschenbuch. Condition: Neu. Neuware -Scientific Essay from the year 2023 in the subject Physics - Astronomy, , language: English, abstract: This work aims to investigate the phenomenon of unusual variations in cosmic ray intensity in the period 1981-1994, particularly in the context of interplanetary magnetic clouds and low-amplitude anisotropic wave trains.The text provides a detailed analysis of the relationship between low-amplitude anisotropic wave trains and interplanetary perturbations, particularly with respect to changes in cosmic ray intensity. By analysing data from the Deep River Neutron Monitor, the interaction between high solar wind velocities, the orientation of the interplanetary magnetic field and the proton density is highlighted.Books on Demand GmbH, Überseering 33, 22297 Hamburg 24 pp. Englisch.
Published by GRIN Verlag Jan 2024, 2024
ISBN 10: 3346996204 ISBN 13: 9783346996206
Language: English
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germany
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Add to basketTaschenbuch. Condition: Neu. Neuware -Scientific Study from the year 2024 in the subject Physics - Astronomy, , language: English, abstract: This study investigates the phenomenon of Low Amplitude Anisotropic Wave Train Events (LAWEs) in cosmic ray intensity using data from the ground-based Deep River neutron monitor for the period 1991-94. The analysis reveals that the amplitude of diurnal anisotropy during LAWE events consistently remains low and statistically constant compared to the quiet day annual average amplitude for the majority of events. Furthermore, the timing of the maximum diurnal anisotropy for LAWE events shifts significantly towards earlier hours, aligning with the co-rotational direction and remaining consistent with the direction of quiet day annual average anisotropy for most events.Conversely, the amplitude of semi/tri-diurnal anisotropy remains statistically high and unchanged. However, the phase shift occurs towards later hours compared to the quiet day annual average values for the majority of LAWEs. Analysis of diurnal anisotropy vectors reveals a shift towards earlier hours in 50% of events and a shift towards later hours in the remaining 50%, relative to the average vector for the entire period. Additionally, it is observed that the amplitude of these vectors significantly increases with the shift towards later hours.The study suggests that high-speed solar wind streams do not play a significant role in causing LAWE events on a short-term basis, but they may contribute to these events on a long-term basis. The occurrence of LAWE is found to be dominant when the polarity of Bx and Bz remains positive, and the polarity of By remains negative ¿ a phenomenon not reported previously. Furthermore, the amplitude of the first harmonic exhibits a good anti-correlation with solar wind velocity, while the direction of the first and third harmonics shows nearly good anti-correlation. The direction of the second harmonic shows nearly good anti-correlation with interplanetary magnetic field strength.Books on Demand GmbH, Überseering 33, 22297 Hamburg 24 pp. Englisch.