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  4. Observations of Galilean Moons by JIRAM on board Juno
 
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Observations of Galilean Moons by JIRAM on board Juno

Author(s)
Mura, A.
Adriani, A.
Bolton, S. J.
Plainaki, Christina  
Olivieri, Angelo  
Subjects

Planetary magnetosphe...

MAGNETOSPHERIC PHYSIC...

Atmospheres

PLANETARY SCIENCES: F...

Interiors

PLANETARY SCIENCES: F...

Jupiter

PLANETARY SCIENCES: S...

Date Issued
2017-12-01
Publisher
American Geophysical Union
Abstract
JIRAM (Jovian Infrared Auroral Mapper) is an imager/spectrometer onboard Juno, mainly devoted to the study of the atmosphere and theauroral emission of Jupiter. During the first year of the mission,thanks to the polar and highly elliptical orbit of Juno, JIRAM alsotook several images and spectra of all the Galilean moons.JIRAM combines two data channels (images and spectra) in oneinstrument. The imager channel is a single detector with two differentfilters (128 x 432 pixels each), with a total FoV of 5.9° by 3.5°.The two filters, "L" and "M" bands, are centered at 3.45 µm and 4.75µm respectively. When observing a moon, the L band mostly detect thealbedo from the surface, while the M filter is suitable for mappingthe thermal structures (especially in the case of Io). Thespectrometer ranges from 2 to 5 µm, with 9 µm spectral resolution.JIRAM uses a dedicated de-spinning mirror to compensate for spacecraftrotation ( 2 rotations per minute), thus allowing the observations ofthe moons, from a spinning spacecraft, with high integration time.JIRAM perform one acquisition, consisting of two 2D images indifferent spectral ranges/channels, and a 1D slit with full spectralresolution, every spacecraft rotation. JIRAM can also tilt its fieldof view (FoV) along the plane perpendicular to Juno spin axis, bydelaying or anticipating the acquisition, thus allowing thespectrometer slit to acquire spectral images of the moons.The angular resolution is 0.01° / pixel for both the imager and thespectrometer. This results in a spatial resolution, at the surface,that varies with the spacecraft radial distance but is of the order of100 km/pixel during most imaging activities.Here we present the first observations of Io, Europa, Ganymede andCallisto made by JIRAM during the first 8 orbits. In particular,emission from Io's sulfur and sulfur-dioxide frost is analysed andstudied, and thermal structures are mapped. The distribution ofGanymede silicate rock versus water ice features is also reported.
URI
https://hdl.handle.net/20.500.13025/5251
DOI
5aba37706c5e1b5a034b8b26
URL
http://adsabs.harvard.edu/abs/2017AGUFM.P23E..01M
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