Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...358..776f&link_type=abstract
Astronomy and Astrophysics, v.358, p.776-788 (2000)
Astronomy and Astrophysics
Astrophysics
12
Sun: Radio Radiation, Masers
Scientific paper
We perform a numerical study on the quasilinear relaxation of an electron cyclotron maser on the initially dominant mode. We focus thereby on a situation where the initially dominant modes are quasi-electrostatic lower hybrid (lh) waves, which have not been treated in preceding studies. To this end, we chose 0.2 <= omega_p / omega Be < 0.5 (omega_p : plasma-, omega Be: electron cyclotron frequency) and an initial losscone distribution of energetic electrons of the form f(p,mu ) ~ p-xi e-mu 2/mu_0 2 (p: momentum, mu : pitch angle cosine). Superimposed on this is a damping Maxwellian background. From our calculations, we find that multiple peaks in the lower-hybrid wave intensity can occur if the initial loss cone distribution is sufficiently broad. We also find that quasilinear relaxation with respect to lower-hybrid waves does not destroy the capability of the electron distribution to amplify transverse (XOZ) waves, which therefore become dominant at a later stage. The comparison with observations shows that the calculated shape of a single peak in the lower-hybrid energy density displays a remarkable similarity to solar radio spikes.
Arzner Kaspar
Fleishman Gregory
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