Jovian hectometric radiation - Beaming, source extension, and solar wind control

Details Jovian hectometric radiation - Beaming, source extension, and solar wind control Jovian hectometric radiation - Beaming, source extension, and solar wind control

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...226..297l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 226, no. 1, Dec. 1989, p. 297-310.

Astronomy and Astrophysics

Astrophysics

26

Jupiter (Planet), Planetary Radiation, Radio Emission, Solar Wind, Emission Spectra, Light Beams, Magnetic Dipoles, Polarization (Waves), Voyager 1 Spacecraft, Voyager 2 Spacecraft

Scientific paper

The Voyager 1 and Voyager 2 hectometric-wavelength (HOM) radio emission data for Jupiter, recorded in 1979, were used to determine beaming at three selected frequencies: f = 1326 kHz, 942 kHz, and 558 kHz. Evidence is presented for strong HOM beaming with the beam axis situated to the north of the magnetic dipole equator (1.6). The total beam width is between 10 and 20 deg, depending on the normalized detection threshold.

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