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Lion roars and nonoscillatory drift mirror waves in the magnetosheath

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TLDR
In this paper, it was shown that Extremely Low Frequency (low frequency) or "lion" roars are closely coupled to quasi-periodic, large scale magnetosheath structures.
Abstract
It is shown that Extremely Low Frequency, or 'lion' roars are closely coupled to quasi-periodic, large scale magnetosheath structures. Because the latter are waves generated by the drift mirror instability, an attempt is made to identify and describe the magnetic and plasma features associated with this instability. Observations and analyses of the large scale structures using ISEE 1 and 2 data for the earth's magnetosheath and Pioneer 11 data for Jupiter and Saturn are presented, along with the background of the drift mirror waves. The cyclotron and drift mirror instabilities occurring in the magnetosheath are natural relaxation processes which reduce the plasma pressure anisotropies created by preferential heating of the solar wind plasma as it passes through the bow shock, as well as the compression occurring when the plasma and fields approach the near-subsolar magnetopause.

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Citations
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The Cassini Magnetic Field Investigation

TL;DR: The dual technique magnetometer system onboard the Cassini orbiter is described in this paper, which consists of vector helium and fluxgate magnetometers with the capability to operate the helium device in a scalar mode.
Journal ArticleDOI

The magnetosheath region adjacent to the dayside magnetopause: AMPTE/IRM observations

TL;DR: In this paper, the magnetic shear across the magnetopause has been investigated and the magnetic field in the magnetosheath region adjacent to the dayside magnetosphere has been found to depend strongly on the angle between the magnetoheath magnetic field and the geomagnetic field.
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Great magnetic storms

TL;DR: In this paper, the five largest magnetic storms that occurred between 1971 to 1986 were studied to determine their solar and interplanetary causes, and all of the events were associated with high speed solar wind streams led by collisionless shocks.
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Mirror instability: 1. Physical mechanism of linear instability

TL;DR: In this paper, the authors review the physics of the linear instability and point out that the instability mechanism hinges on the special behavior of particles with small velocity along the field, called resonant particles.
Journal ArticleDOI

The heliospheric magnetic field over the South polar region of the sun.

TL;DR: Magnetic field measurements from the Ulysses space mission showed that the structure and properties of the three-dimensional heliosphere were determined by the fast solar wind flow and magnetic fields from the large coronal holes in the polar regions of the sun.
References
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Journal ArticleDOI

Limit on stably trapped particle fluxes

TL;DR: The limit on stably trapped particle fluxes determined theoretically and compared with data from Explorer satellites was first established in this paper, and the limit was later confirmed by the International Journal of Astronautics.
Journal ArticleDOI

Drift Mirror Instability in the Magnetosphere

Akira Hasegawa
- 01 Jan 1969 - 
TL;DR: In this article, a new theory of the mirror instability is developed which includes the effects of ∇B and ∇n, finite Larmor radius, and a coexisting cold plasma, and it is shown that the instability becomes overstable with a frequency equal to the drift wave frequency, which may be determined by the wave number that gives the maximum growth rate.
Journal ArticleDOI

Depletion of solar wind plasma near a planetary boundary

TL;DR: In this paper, a mathematical model is presented that describes the squeezing of solar wind plasma out along interplanetary magnetic field lines in the region between the bow shock and the effective planetary boundary (in the case of the earth, the magnetopause).
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