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Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1302..158w&link_type=abstract
PICKUP IONS THROUGHOUT THE HELIOSPHERE AND BEYOND: Proceedings of the 9th Annual International Astrophysics Conference. AIP Con
Other
Interplanetary Magnetic Fields, Spacecraft, Solar Wind, Sensors, Gravitational Radiation, Magnetic Fields, And Other Observations, Spacecraft/Atmosphere Interactions, Particle Emission, Solar Wind, Photoconductors And Bolometers
Scientific paper
Two of the most recent outer heliospheric kHz emissions detected by the University of Iowa plasma wave detector on Voyager 1 started at about 2004.64 and 2006.39, respectively. Large interplanetary shocks reached V1 and V2, which are near the heliospheric termination shock, at almost the same time that the two kHz radio emissions turned-on. So, in fact, the arrivals of these large shocks near the heliospheric termination shock were coincident with the onset of these kHz emissions. These two large shocks were unusual in that they were the two strongest shocks in solar cycle 23 seen in the outer heliosphere at V2. They had developed maximum dynamic pressures ~4-6 times the average solar wind dynamic pressure for periods >26 days by the time they reached V2.
Intriligator Devrie S.
Webber William R.
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