Journal article
Saturn's quasiperiodic magnetohydrodynamic waves
Geophysical research letters, Vol.43(21), pp.11102-11111
11/16/2016
DOI: 10.1002/2016GL071069
Abstract
Quasiperiodic similar to 1 h fluctuations have been recently reported by numerous instruments on board the Cassini spacecraft. The interpretation of the sources of these fluctuations has remained elusive to date. Here we provide an explanation for the origin of these fluctuations using magnetometer observations. We find that magnetic field fluctuations at high northern latitudes are Alfvenic, with small amplitudes (similar to 0.4 nT), and are concentrated in wave packets similar to those observed in Kleindienst et al. (2009). The wave packets recur periodically at the northern magnetic oscillation period. We use a magnetospheric box model to provide an interpretation of the wave periods. Our model results suggest that the observed magnetic fluctuations are second harmonic Alfven waves standing between the northern and southern ionospheres in Saturn's outer magnetosphere.
Details
- Title: Subtitle
- Saturn's quasiperiodic magnetohydrodynamic waves
- Creators
- J. N. Yates - Imperial College LondonD. J. Southwood - Imperial College LondonM. K. Dougherty - Imperial College LondonA. H. Sulaiman - University of IowaA. Masters - Imperial College LondonS. W. H. Cowley - University of LeicesterM. G. Kivelson - University of MichiganC. H. K. Chen - Imperial College LondonG. Provan - University of LeicesterD. G. Mitchell - Johns Hopkins University Applied Physics LaboratoryG. B. Hospodarsky - University of IowaN. Achilleos - University College LondonA. M. Sorba - University College LondonA. J. Coates - University College London
- Resource Type
- Journal article
- Publication Details
- Geophysical research letters, Vol.43(21), pp.11102-11111
- DOI
- 10.1002/2016GL071069
- ISSN
- 0094-8276
- eISSN
- 1944-8007
- Publisher
- Amer Geophysical Union
- Number of pages
- 10
- Grant note
- International Space Sciences Institute (ISSI) international team on "Coordinated Numerical Modeling of the Global Jovian and Saturnian Systems" Royal Society ST/K001051/1 / STFC's Imperial College Astrophysics & Space Physics Consolidated Grant ST/K001000/1; ST/K001051/1; ST/N000722/1; ST/N003748/1; ST/N000692/1; ST/N000749/1; ST/K000977/1 / STFC; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC) Jet Propulsion Laboratory ST/N000692/1; ST/K001000/1; ST/N003748/1; ST/N000749/1; ST/K001051/1; ST/K000977/1; ST/N000722/1 / Science and Technology Facilities Council; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC) ST/N000722/1 / UK STFC; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC) STFC; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC) NAS5-97271 / NASA Office of Space Science; National Aeronautics & Space Administration (NASA) ST/M003094/1 / UK Space Agency Imperial College 1415150 / NASA; National Aeronautics & Space Administration (NASA) ST/N000749/1; ST/N50449X/1 / STFC; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC)
- Language
- English
- Date published
- 11/16/2016
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984455549302771
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