Academic literature on the topic 'Magnetopshere'

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Journal articles on the topic "Magnetopshere"

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Eriksson, P. T. I., L. G. Blomberg, A. D. M. Walker, and K. H. Glassmeier. "Poloidal ULF oscillations in the dayside magnetosphere: a Cluster study." Annales Geophysicae 23, no. 7 (2005): 2679–86. http://dx.doi.org/10.5194/angeo-23-2679-2005.

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Abstract. Three ULF wave events, all occurring in the dayside magnetopshere during magnetically quiet times, are studied using the Cluster satellites. The multi-point measurements obtained from Cluster are used to determine the azimuthal wave number for the events by means of the phase shift and the azimuthal separation between the satellites. Also, the polarisation of the electric and magnetic fields is examined in a field-aligned coordinate system, which, in turn, gives the mode of the oscillations. The large-inclination orbits of Cluster allow us to examine the phase relationship between th
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Rajwade, K. M., B. W. Stappers, A. G. Lyne, et al. "Long term radio and X-ray evolution of the magnetar Swift J1818.0-1607." Monthly Notices of the Royal Astronomical Society 512, no. 2 (2022): 1687–95. http://dx.doi.org/10.1093/mnras/stac446.

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ABSTRACT We report on the the long term monitoring campaign of the seemingly youngest magnetar Swift J1818.0–1607 at radio and X-ray wavelengths over a span of one year. We obtained a coherent timing solution for the magnetar over the same time span. The frequency derivative of the magnetar shows systematic variation with the values oscillating about a mean value of −1.37 × 10−11 Hz s−1. The magnitude of the variation in the frequency derivative reduces with time before converging on the mean value. This corresponds to a characteristic age of ∼ 860 years, 2–4 times more than previously estimat
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Fung, Shing F. "Specification of multiple geomagnetic responses to variable solar wind and IMF input." Annales Geophysicae 26, no. 3 (2008): 639–52. http://dx.doi.org/10.5194/angeo-26-639-2008.

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Abstract. This paper shows that the state of the magnetosphere, resulting from continuous but variable forcing of the solar wind and the interplanetary magnetic field (IMF), can be empirically specified by a magnetospheric state vector Ψ, consisting of a set of hourly-averaged magnetospheric driver and response parameters. It is demonstrated that there exists a correspondence between the magnetospheric driver and multiple geomagnetic response parameters. This parameter correspondence allows different magnetopsheric states to be specified by means of a look-up table, provided that the relative
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Inceoglu, Fadil, and Paul T. M. Loto’aniu. "Detection of solar QBO-like signals in earth’s magnetic field from multi-GOES mission data." Scientific Reports 13, no. 1 (2023). http://dx.doi.org/10.1038/s41598-023-46902-6.

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AbstractThrough variations in its magnetic activity at different timescales, the Sun strongly influences the space weather conditions throughout the heliosphere. The most known solar activity variation is the Schwabe Cycle, also known as the Sunspot Cycle (SCs), period of which ranges from 9 to 13 years. The Sun also shows shorter quasi-periodic variations, such as the quasi-biennial oscillations (QBOs), superposed on the SCs. The QBOs are thought to be a global phenomena extending from the subsurface layers of the Sun to Earth and throughout the Heliosphere with a period generally between 1.3
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Dissertations / Theses on the topic "Magnetopshere"

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Barik, Krushna Chandra. "Generation of low frequency electromagnetic waves in the magnetosphere." Thesis, IIG, 2021. http://library.iigm.res.in:8080/xmlui/handle/123456798/74.

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