GLL UVS Instrument

GLL EUV Instrument

The Galileo ultraviolet spectrometer experiment consists of two instruments: the Ultraviolet Spectrometer (UVS), mounted on the pointed orbiter scan platform, and the Extreme Ultraviolet Spectrometer (EUV), mounted on the spinning part of the orbiter with the field of view perpendicular to the spin axis.

Primary objectives of the investigation are to understand physical processes occurring in: (1) the upper atmosphere of Jupiter; (2) the Io plasma torus; (3) the volatile gases escaping from Galilean satellites. (see Space Science Reviews 60:503-530, 1992)

Capitalized items represent additional directories.

CALIBRATION
CMD_FORMATS
GLL_probe_loc.pdf
HDR_FORMATS
SCIENCE_SUMMARIES
SEQUENCE_ARCHIVE
SPICE_KERNELS
UVS_w_Hord_McNutt.pdf
cmd_archive.lis
euv_edr_dataset.lis
euv_inst_lyle.template_1
experimenters_handbook.doc
filenames.html
ganymede_hydrogen.pdf
gggs_torus_anim.mpg
gll_phone.lis
grating_scan_cases.lis
grating_scan_wrong.stat
jup_radius_used.doc
load_boundaries.lis_3
milestones.html
people.html
press.html
publications.lis_101
safing_history.lis_6
time_clocks.doc_4
user_handbook_p1.doc_38
user_handbook_p2.doc_2
uvs_edr_dataset.lis
uvs_inst.template_2
uvs_inst_history.doc