We report comprehensive studies of the crystallographic, magnetic, and thermal properties of a spinel-type magnetically frustrated compound, CoAl 2 O 4 , and a magnetically diluted system, Co 1 -x Zn x Al 2 O 4 . These studies revealed the effects of dilution and disorder when the tetrahedral magnetic Co ion was replaced by the nonmagnetic Zn ion. Low-temperature anomalies were observed in magnetic susceptibility at x < 0.6. A multicritical point was apparent at T = 3.4 K and x = 0.12, where the antiferromagnetic, spin-glass-like, and paramagnetic phases met. At that point, the quenched ferromagnetic component induced by a magnetic field during cooling was sharply enhanced and was observable below x = 0.6. At x ∼ 0.6, magnetic susceptibility and specific heat were described by temperature power laws, χ ∼ C/T ∼ T −δ , in accord with the site percolation threshold of the diamond lattice. This behavior is reminiscent of a quantum critical singularity. We propose an x-temperature phase diagram in the range 0 x 1 for Co 1 -x Zn x Al 2 O 4 . The transition temperature of CoAl 2 O 4 determined from magnetic susceptibility measured under hydrostatic pressure increased with increasing pressure.
[1] The SS-520-2 sounding rocket skimmed over the high-latitude part of the cusp region and observed fine-scale field-aligned electron precipitations in the vicinity of the inverted-V structures with the Low Energy Particle-Electron Spectrum Analyzer (LEP-ESA). There are at least two types of fine-scale electron precipitations, namely ''edge-type electron bursts'' and ''multiple energy-time dispersions.'' Edge-type electron bursts were observed only at the edge of the inverted-V region, whereas multiple energy-time dispersions were observed separately from the inverted-V region as well as within or overlapping it. The latter was characterized by field-aligned precipitations with falling energies from $200 eV down to $20 eV at a repetition rate of 1-2 Hz. Source altitudes were estimated using the energy-time and pitch angle-time dispersions. As a result, we found that the source altitudes were distributed along the geomagnetic field at altitudes of several thousand kilometers, depending on the accelerated energies of electrons. Higher-energy electrons are generated at higher altitudes. The source temperature of the energy-time dispersion was much higher than that of ionospheric cold electrons. We suggest that electrons injected from the magnetosheath were accelerated by inertial Alfvén waves at altitudes of several thousands of kilometers.
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