Direction‐finding measurements of Jovian low‐frequency radio components by Juno near Perijove 1. Issue 13 (4th July 2017)

• Record Type: Journal Article
• Authors: Imai, Masafumi; Kurth, William S.; Hospodarsky, George B.; Bolton, Scott J.; Connerney, John E. P.; Levin, Steven M.
• Is Part Of: Geophysical research letters. Volume 44:Issue 13(2017)
• Page Start: 6508
• Page End: 6516
• Publication Date: 2017-07-04
• Subjects: Jupiter -- Juno/Waves -- direction‐finding measurements -- broadband kilometric radiation -- narrowband kilometric radiation -- escaping continuum radiation; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2017GL072850
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: With the aid of the radio and plasma wave (Waves) instrument on board the Juno spacecraft, the first scientific close encounter to Jupiter (Perijove 1) of Juno led to an opportunity to perform direction‐finding measurements of the intense Jovian broadband kilometric (bKOM) radiation at 10 to 142 kHz, two escaping continuum radiation (ECR) events at 9 to 22 kHz, and two narrowband kilometric (nKOM) radiation events at 45–112 kHz. We conclude that the northern bKOM radio sources are localized on M ‐shell = 50–60 field lines where M ‐shell is similar to L ‐shell for nondipolar fields. The beam cone half‐angle varies from 40° to 55°. By intersecting the wavek vector with the Jovian centrifugal equator, two ECR sources are located inside and outside of 11–12 R J, and two nKOM sources are found between 11 and 20 R J . These source frequencies and locations can be used for plasma diagnostics in Jupiter's inner magnetosphere. Key Points: We perform direction‐finding analysis for Jupiter's low‐frequency radio emissions Northern bKOM radio sources are located along high‐latitude auroral magnetic field lines Four smooth components provide a proxy of the electron density profiles in Jovian inner magnetosphere