Abstract:Abstract. Electric fields, magnetic fields, and plasmas measured on the Polar satellite are studied to determine the altitude extent of the upward field-aligned current portion of the auroral acceleration region and the physical processes that populate it with parallel electric fields. This region extends upward to a geocentric altitude of 3 or 3.5 Earth radii at premidnight local times during the spring and fall. In a model for this region a necessary but not sufficient condition for the appearance of paralle… Show more
“…In areas of upward current, large amplitude electromagnetic waves with frequencies within 5% of the local proton gyrofrequency p and its harmonics are often observed where an upstreaming ion beam exist (Chaston et al, 2002). The upgoing ion beams are reported by the S3-3 satellite (Shelley et al, 1976;Mozer et al, 1977) and by the Polar satellite data (Mozer and Hull, 2001). Ions are often observed to have been accelerated transversely to the background magnetic field in the auroral region (Sharp et al, 1977;Lund et al, 2001).…”
Section: Introductionmentioning
confidence: 99%
“…Horne and Thorne (1997) have found a correlation between periods of EMIC waves activity and pitch angle distributions, which resembles an "X" in velocity space and may be the signature of loss-cone G. Ahirwar et al: Beam effect on electromagnetic ion-cyclotron waves 559 distributions. The ion beam measured by Mozer and Hull (2001) has been considered to enter the plasma which follows the loss-cone distribution function. The results are compared with those derived by Kennel and Petschek (1966).…”
Abstract. The effect of upgoing ion beam and temperature anisotropy on the dispersion relation, growth rate, parallel and perpendicular resonant energies, and marginal instability of the electromagnetic ion cyclotron (EMIC) waves, with general loss-cone distribution function, in a low β homogeneous plasma, is discussed by investigating the trajectories of the charged particles. The whole plasma is considered to consist of resonant and non-resonant particles. The resonant particles participate in an energy exchange with the waves, whereas the non-resonant particles support the oscillatory motion of the waves. The effects of the steepness of the loss-cone distribution, ion beam velocity, with thermal anisotropy on resonant energy transferred, and the growth rate of the EMIC waves are discussed. It is found that the effect of the upgoing ion beam is to reduce the energy of transversely heated ions, whereas the thermal anisotropy acts as a source of free energy for the EMIC waves and enhances the growth rate. It is found that the EMIC wave emissions occur by extracting energy of perpendicularly heated ions in the presence of an upflowing ion beam and a steep loss-cone distribution function in the anisotropic magnetoplasma. The effect of the steepness of the loss-cone is also to enhance the growth rate of the EMIC waves. The results are interpreted for EMIC emissions in the auroral acceleration region.
“…In areas of upward current, large amplitude electromagnetic waves with frequencies within 5% of the local proton gyrofrequency p and its harmonics are often observed where an upstreaming ion beam exist (Chaston et al, 2002). The upgoing ion beams are reported by the S3-3 satellite (Shelley et al, 1976;Mozer et al, 1977) and by the Polar satellite data (Mozer and Hull, 2001). Ions are often observed to have been accelerated transversely to the background magnetic field in the auroral region (Sharp et al, 1977;Lund et al, 2001).…”
Section: Introductionmentioning
confidence: 99%
“…Horne and Thorne (1997) have found a correlation between periods of EMIC waves activity and pitch angle distributions, which resembles an "X" in velocity space and may be the signature of loss-cone G. Ahirwar et al: Beam effect on electromagnetic ion-cyclotron waves 559 distributions. The ion beam measured by Mozer and Hull (2001) has been considered to enter the plasma which follows the loss-cone distribution function. The results are compared with those derived by Kennel and Petschek (1966).…”
Abstract. The effect of upgoing ion beam and temperature anisotropy on the dispersion relation, growth rate, parallel and perpendicular resonant energies, and marginal instability of the electromagnetic ion cyclotron (EMIC) waves, with general loss-cone distribution function, in a low β homogeneous plasma, is discussed by investigating the trajectories of the charged particles. The whole plasma is considered to consist of resonant and non-resonant particles. The resonant particles participate in an energy exchange with the waves, whereas the non-resonant particles support the oscillatory motion of the waves. The effects of the steepness of the loss-cone distribution, ion beam velocity, with thermal anisotropy on resonant energy transferred, and the growth rate of the EMIC waves are discussed. It is found that the effect of the upgoing ion beam is to reduce the energy of transversely heated ions, whereas the thermal anisotropy acts as a source of free energy for the EMIC waves and enhances the growth rate. It is found that the EMIC wave emissions occur by extracting energy of perpendicularly heated ions in the presence of an upflowing ion beam and a steep loss-cone distribution function in the anisotropic magnetoplasma. The effect of the steepness of the loss-cone is also to enhance the growth rate of the EMIC waves. The results are interpreted for EMIC emissions in the auroral acceleration region.
“…FAST observations also suggest both highand low-altitude acceleration regions ]. Recent Polar observations now conclude that the majority of auroral acceleration is below 2 R E in altitude [Mozer and Hull, 2000].…”
“…[2] Double layers (DLs) and electron holes (EHs) play significant roles in auroral acceleration processes [Ergun et al, 1998;Carlson et al, 1998;Mozer and Kletzing, 1998;McFadden et al, 1999;Mozer and Hull, 2001;Hull et al, 2010]. The formation of EHs in plasma permeated by electron beams has been known since the early work of Roberts and Berk [1967] and Morse and Nielson [1969].…”
[1] We study the dynamical behavior of potential structures in the auroral upward current region. The study is based on a large two-dimensional particle-in-cell simulation. A double layer (DL) forms in the auroral potential structure in the counterstreaming expansion of cold and hot plasmas from bottom (ionospheric side) and top (magnetospheric side), respectively. Transversely nonuniform converging perpendicular electric field drives the plasma from the top, generating V-shaped potential structure within the expanding plasmas. The dynamical features include (1) recurring formation of the DL, (2) downward motion of the DL over the distance of thousands of Debye lengths, (3) collapse of the existing double layer after the reformation of a new one near the top in the hot magnetospheric plasma, and (4) generation of electron holes (EHs) on the high-potential side of the DL and their downward propagation over a few thousand of Debye lengths, where they are dissipated. The EHs are associated with broadband plasma waves with spectrum peaked near the lower hybrid frequency. The EH turbulence is temporally modulated by low-frequency plasma waves near the ion cyclotron frequency W i . Electrostatic ion cyclotron waves above W i occur on the low-potential side of the DL. Transverse and parallel acceleration/heating of both electrons and ions are studied. The fast moving electron holes are found effective in transverse heating of the cold ionospheric electrons trapped below the DL. Relevance of our results to satellite observations in the auroral plasma is discussed.Citation: Singh, N., S. Araveti, and E. B. Wells (2011), Mesoscale PIC simulation of double layers and electron holes affecting parallel and transverse accelerations of electrons and ions,
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