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J. Caplinger

Publications and source records attributed to J. Caplinger.

2 recordsLinked to original sources

Investigation of a parametric instability between ELF and VLF modes driven by antennas immersed in a cold, magnetized plasma

We have studied the behavior of a VLF, ELF and combined ELF/VLF antenna immersed in a cold, magnetized plasma using a fully kinetic, three dimensional Particle-in-Cell simulation code called Large Scale Plasma (LSP). All the antennas are modeled as magnetic dipoles ($\rho_{ant}=0$) and are assigned a time varying current density within a finite sized current loop. The VLF antenna is driven at 10 Amps with a frequency ($\omega_{VLF}$) greater than the lower hybrid frequency ($\omega_{LH}$), while the ELF antenna is driven at 3 Amps with a frequency ($\omega_{ELF}$) less than $\omega_{LH}$. The combined ELF/VLF antenna (which we call a parametric antenna) includes both antennas driven simultaneously in the same simulation domain. We show that the parametric antenna non-linearly excites electromagnetic (EM) Whistler waves to a greater extent than the VLF antenna alone. We also show that the parametric excitation of EM Whistler waves leads to greater emitted EM power (measured in Watts) compared with a VLF antenna alone.

physics.plasm-ph

Asteroseismology of sdB stars with FUSE

The hot subdwarf B (sdB) stars form an homogeneous group populating an extension of the horizontal branch (HB) in the ($T_{\rm eff}$--$\log g$) diagram towards temperatures up to 40,000 K. The recent discovery that many of them are multimode pulsators has triggered a large observational and theoretical effort. We discuss the possibility of performing space-based asteroseismology with {\em FUSE}, and we demonstrate that periodic luminosity variations are already detectable in archival TTAG data of sdB stars. In particular, we report on the {\em FUSE} observation of the pulsator PF 1219+534, which shows the presence of periodic variations at 6.9 mHz and 7.8 mHz, consistent with those reported from ground--based observations.

astro-ph