By Andreas Keiling, Dong-Hun Lee, Valery Nakariakov
Low-frequency waves in area plasmas were studied for a number of many years, and our wisdom achieve has been incremental with numerous paradigm-changing leaps ahead. In our sunlight procedure, such waves ensue within the ionospheres and magnetospheres of planets, and round our Moon. They take place within the sun wind, and extra lately, they've been proven within the Sun’s surroundings in addition. The target of wave study is to appreciate their iteration, their propagation, and their interplay with the encircling plasma. Low-frequency Waves in house Plasmas offers a concise and authoritative updated glance on the place wave learn stands: What have we discovered within the final decade? What are unanswered questions?
While some time past waves in numerous astrophysical plasmas were principally taken care of in separate books, the original function of this monograph is that it covers waves in lots of plasma areas, including:
- Waves in geospace, together with ionosphere and magnetosphere
- Waves in planetary magnetospheres
- Waves on the Moon
- Waves within the sunlight wind
- Waves within the sunlight atmosphere
Because of the breadth of issues coated, this quantity should still attract a wide neighborhood of house scientists and scholars, and it may even be of curiosity to astronomers/astrophysicists who're learning area plasmas past our sun System.
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Extra info for Low-frequency waves in space plasmas
Hayakawa (2002), Resonances in the Earth–Ionosphere Cavity, Kluwer, Dordrecht. , K. Takahashi, H. Fukunishi, T. Nagatsuma, H. Oya, A. Matsuoka, and D. K. Milling (1998), Pi2 pulsations observed from the Akebono satellite in the plasmasphere, J. Geophys. , 103, 17605–17615. , H. Lühr, and J. Rauberg (2013), Global characteristics of Pc1 magnetic pulsations during solar cycle 23 deduced from CHAMP data, Ann. , 31, 1507–1520. , M. Vellante, and E. Fedorov (2000), Distortion of the ULF wave spatial structure upon transmission through the ionosphere, J.
It should be emphasized that most magnetospheric observations of Pi2 waves, including those of the above‐ referenced studies, were made in the vicinity of the equa torial plane. The only exception is the case study by Osaki et al. (1998) of Pi2 waves detected on the ground and at ULF Waves and Transients in the Topside Ionosphere 21 Akebono satellite inside the plasmasphere, but away from the magnetospheric equator (geomagnetic latitudes 25 40 ). ) waves. This observation has suggested that simple cavity mode oscil lations excited by an impulsive source cannot be an appropriate model of low‐latitude Pi2, and that mode coupling should be taken into account.
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