Planetary aurorae are powerful emissions radiated from auroral regions of magnetized planets by accelerated charged particles, in a wide range of wavelengths (from radio to X-rays). The UV range in particular is adequate to measure collisionaly excited transitions of H and H2, the dominant species in the upper atmosphere of giant planets, produced by precipitating auroral particles, and benefits a good angular resolution. Auroral UV observations therefore provide a rich source of informations on planetary atmospheres and magnetospheres. They also offer a unique diagnostic to remotely probe the solar wind activity throughout the heliosphere. from Laurent Lamy EPN-TAP Planetary aurorae are powerful emissions radiated from auroral regions of magnetized planets by accelerated charged particles, in a wide range of wavelengths (from radio to X-rays). The UV range in particular is adequate to measure collisionaly excited transitions of H and H2, the dominant species in the upper atmosphere of giant planets, produced by precipitating auroral particles, and benefits a good angular resolution. Auroral UV observations therefore provide a rich source of informations on planetary atmospheres and magnetospheres. They also offer a unique diagnostic to remotely probe the solar wind activity throughout the heliosphere. from Laurent Lamy this research have been made using APIS database by LaurentLamy Lesia-Observatoire de Paris plasma in planetary atmosphere. Query successful For advice on how to cite the resource(s) that contributed to this result, see http://voparis-tap-planeto.obspm.fr:80/tableinfo/apis.epn_core plasma in planetary atmosphere. Granule unique identifier, provides direct access Group identifier, identical for similar data products Identical for data products related to the same original data Organization of the data product (from enumerated list) Name of target (IAU standard) type of target from enumerated list Acquisition start time (in JD) Acquisition stop time (in JD) Min time sampling step Max time sampling step Min integration time Max integration time Min spectral range (frequency) Max spectral range (frequency) min spectral sampling step (as frequency) max pectral sampling step (as frequency) Min spectral resolution (as frequency) Max spectral resolution (as frequency) Min (westernmost) longitude on planetary surface Max (easternmost) longitude on planetary surface Min latitude on planetary surface Max latitude on planetary surface Min of third coordinate (altitude) Max of third coordinate (altitude) Min resolution on longitude Max resolution on longitude Min resolution on latitude Max resolution on latitude Min resolution in third coordinate Max resolution in third coordinate Defines the nature of coordinates (from enumerated list) Min incidence angle (solar zenith angle) Max incidence angle (solar zenith angle) Min emergence angle Max emergence angle Min phase angle Max phase angle Standard name of the observatory or spacecraft Standard name of instrument UCD(s) defining the nature of measurements URL of the data files. file format type. Estimate file size in kB. Level of calibration (CODMAC level) publiher of the ressource Extra: bibliograpic reference Title of the ressourcee region of interest from a predifine list Secondary name (can be standard name of region of interest) Right ascention Declination Start of public period Creation date of entry Date of last modification of entry STC-S region URL of a thumbnail image Link to a web page providing more details on the granule Observing mode Detector name Optical element name Filter name Position angle of image y axis Measurement unit Proposal identifier Proposal principal investigator Proposal title spatial resolution per pixel or platescale Name of the observational campaign Apparent radius of the target North pole position angle with respect to celestial north pole Primary observed hemisphere Secondary observed hemisphere