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- W3021320332 abstract "The five “magnetic” planets in the solar system (Earth and the four gas giants) emit at radio frequencies because solar-wind powered electron currents deposit energy in their magnetic polar regions. We summarize predictions of the radio emission from the known extrasolar planets and initial detection efforts. Most of the known extrasolar planets should emit in the frequency range 10–1000 MHz and, under favorable circumstances, some may have flux densities above 0.1 Jy. The current limits set by observations with the Very Large Array (VLA) and the Giant Metrewave Radio Telescope (GMRT) are consistent with but generally do not provide strong constraints on the predictions. Future radio telescopes, such as the Long Wavelength Array (LWA), the Mileura Widefield Array (MWA), Low Frequency Array (LOFAR) and the Square Kilometer Array (SKA), should be able to detect the known extrasolar planets or place austere limits on their radio emission. Planets with masses much lower than those in the current census will probably radiate below 10 MHz and will require a space-based array." @default.
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- W3021320332 date "2006-01-01" @default.
- W3021320332 modified "2023-09-27" @default.
- W3021320332 title "Radio Detection of Extrasolar Planets: Present and Future Prospects" @default.
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