Longitudinal variability in Jupiter's zonal winds derived from multi-wavelength HST observations. (June 2018)

• Record Type: Journal Article
• Authors: Johnson, Perianne E.; Morales-Juberías, Raúl; Simon, Amy; Gaulme, Patrick; Wong, Michael H.; Cosentino, Richard G.
• Is Part Of: Planetary and space science. Volume 155(2018)
• Page Start: 2
• Page End: 11
• Publication Date: 2018-06
• Subjects: Jupiter -- Atmosphere -- Atmospheres -- Dynamics; Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2018.01.004
• Languages: English
• ISSNs: 0032-0633

Abstract

Abstract: Multi-wavelength Hubble Space Telescope (HST) images of Jupiter from the Outer Planets Atmospheres Legacy (OPAL) and Wide Field Coverage for Juno (WFCJ) programs in 2015, 2016, and 2017 are used to derive wind profiles as a function of latitude and longitude. Wind profiles are typically zonally averaged to reduce measurement uncertainties. However, doing this destroys any variations of the zonal-component of winds in the longitudinal direction. Here, we present the results derived from using a "sliding-window" correlation method. This method adds longitudinal specificity, and allows for the detection of spatial variations in the zonal winds. Spatial variations are identified in two jets: 1 at 17 ° N, the location of a prominent westward jet, and the other at 7 ° S, the location of the chevrons. Temporal and spatial variations at the 24°N jet and the 5-μm hot spots are also examined. Highlights: We present a method of retrieving zonal winds in Jupiter that allows for the detection of spatial variations in the profiles. Spatial variations are identified in two jets: one at 17°N and the other at 7°S. Temporal and spatial variations at the 24°N and the 5-μm hot spots are also examined.