318-324Whistler waves interacting with an assumed anti-loss cone (ALC) distribution is shown to become highly unstable at times of substorm onsets. This establishes the presence of ALC electrons at onset-time geomagnetosphere plasma sheet (PS). The stability analysis proves that the whistler instability resulting from ALC interactions arises at frequencies greater than the electron cyclotron frequency. The study establishes the role of plasma β as a factor determining the extent of whistler instability even at times of highly disturbed conditions. The major part of free energy available at PS during substorm onsets is proved to be the contribution due to the anisotropy of the ALC distribution function. Presence of a few cold electrons alo...
The Earth's magnetosheath (MSH) is governed by numerous physical processes which shape the particle ...
Abstract. Geomagnetotail is the main reservoir where the energy from the solar wind is accumulated a...
International audienceThe whistler-mode waves and electron temperature anisotropy play a key role pr...
We provide evidence of the simultaneous occurrence of large-amplitude, quasi-parallel whistler mode ...
38-41Using an anisotropic and loss cone velocity distribution for the electrons, the dependence of w...
International audienceWe provide evidence of the simultaneous occurrence of large-amplitude, quasi-p...
248-253The nature of the convective instability has been investigated for whistler wave propagation ...
Using the HOTRAY code, we demonstrate that lightning-generated whistlers which enter the magnetosphe...
Whistler mode chorus emissions are excited as plasma sheet electrons are injected into the inner mag...
There are two main theories for the origin of diffuse auroral electron precipitation: precipitation ...
Whistler emissions close to the magnetopause on the magnetospheric side are investigated using the f...
In the absence of efficient collisions, deviations from thermal equilibrium of plasma particle distr...
Abstract. A linear analysis is performed to investigate he kinetic ross-field streaming instability ...
Dipolarization of geomagnetic fields had been found to occur at tailside during geomagnetic activiti...
International audienceThe intensification of the nightside whistler-mode chorus emissions is observe...
The Earth's magnetosheath (MSH) is governed by numerous physical processes which shape the particle ...
Abstract. Geomagnetotail is the main reservoir where the energy from the solar wind is accumulated a...
International audienceThe whistler-mode waves and electron temperature anisotropy play a key role pr...
We provide evidence of the simultaneous occurrence of large-amplitude, quasi-parallel whistler mode ...
38-41Using an anisotropic and loss cone velocity distribution for the electrons, the dependence of w...
International audienceWe provide evidence of the simultaneous occurrence of large-amplitude, quasi-p...
248-253The nature of the convective instability has been investigated for whistler wave propagation ...
Using the HOTRAY code, we demonstrate that lightning-generated whistlers which enter the magnetosphe...
Whistler mode chorus emissions are excited as plasma sheet electrons are injected into the inner mag...
There are two main theories for the origin of diffuse auroral electron precipitation: precipitation ...
Whistler emissions close to the magnetopause on the magnetospheric side are investigated using the f...
In the absence of efficient collisions, deviations from thermal equilibrium of plasma particle distr...
Abstract. A linear analysis is performed to investigate he kinetic ross-field streaming instability ...
Dipolarization of geomagnetic fields had been found to occur at tailside during geomagnetic activiti...
International audienceThe intensification of the nightside whistler-mode chorus emissions is observe...
The Earth's magnetosheath (MSH) is governed by numerous physical processes which shape the particle ...
Abstract. Geomagnetotail is the main reservoir where the energy from the solar wind is accumulated a...
International audienceThe whistler-mode waves and electron temperature anisotropy play a key role pr...