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UVS and JIRAM field of view and field of regard polar projections

UVS and JIRAM field of view and field of regard polar projections. For questions or comments, please contact Bertrand Bonfond at b.bonfond@boulder.swri.edu. UVS swath (mirror position: +10degrees). Juno horizon. Juno visibility limit for features at 1000 km altitude. “Mean” aurora

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UVS and JIRAM field of view and field of regard polar projections

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  1. UVS and JIRAM field of view and field of regard polar projections For questions or comments, please contact Bertrand Bonfond at b.bonfond@boulder.swri.edu

  2. UVS swath (mirror position: +10degrees) Juno horizon Juno visibility limit for features at 1000 km altitude “Mean” aurora from Hubble Space Telescope FUV images JIRAM swath JIRAM field of view Extremity of the UVS field of regard UVS field of view (mirror position: +10degrees) Terminator

  3. Juno footprint according to the VIP4 magnetic field model (Connerney et al, 1998) Juno footprint according to the VIPAL magnetic field model (Hess et al, 2011) Pointwhere the surface magnetic field and the Juno direction are co-aligned Sub-Juno position

  4. Callisto longitude Callisto footprint Europa footprint Ganymede footprint Europa longitude Io footprint spots and tail Ganymede longitude Io longitude

  5. Main Oval (MO) in red: The Juno VIPAL footprint is <5000km from the MO (i.e. Juno is close to MF lines connected to the MO) Extremities of the UVS field of regard IFP tail in blue: A portion of the IFP tail is <2000km from the Juno horizon (useful for vertical extension measurements) GFP in blue: The GFP is <5000km from the Juno horizon (useful for vertical extension measurements) Main Oval (MO) in blue: A portion of the MO is <5000km from the Juno horizon (useful for vertical extension measurements)

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