User Tools

Site Tools


science_cases

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
science_cases [2022/09/12 09:30] adminscience_cases [2022/09/29 13:49] (current) admin
Line 8: Line 8:
 |INAF  |[[:science_cases:inaf_science_case|Mineral identification via reflectance spectra]] (planetary surfaces/compositions/interiors) \\  [possible applications foreseen in GMAP]  | |INAF  |[[:science_cases:inaf_science_case|Mineral identification via reflectance spectra]] (planetary surfaces/compositions/interiors) \\  [possible applications foreseen in GMAP]  |
 |DLR  |[[:science_cases:dlr_science_case|Classification of surface composition on the surface of Mercury]] (planetary surfaces/compositions/interiors) \\  [resulting data products can be used for GMAP]  | |DLR  |[[:science_cases:dlr_science_case|Classification of surface composition on the surface of Mercury]] (planetary surfaces/compositions/interiors) \\  [resulting data products can be used for GMAP]  |
-|AOP  |[[:science_cases:aop_science_case|Abundance of asteroids in Earth-like orbits from STEREO images]] (small bodies, asteroids & comets)  |+|AOP  |Classification of meteors based on their lightcurves (small bodies, asteroids & comets)  |
 |GMAP  |[[:science_cases:gmap_science_cases|Automatic recognition and analysis of planetary surface features]] (planetary surfaces/compositions/interiors)  | |GMAP  |[[:science_cases:gmap_science_cases|Automatic recognition and analysis of planetary surface features]] (planetary surfaces/compositions/interiors)  |
 |IWF-OEAW  |[[:science_cases:iwf_science_case|Detection and classification of CMEs in in-situ solar wind data]] (magnetospheres, plasma environments and space weather)  | |IWF-OEAW  |[[:science_cases:iwf_science_case|Detection and classification of CMEs in in-situ solar wind data]] (magnetospheres, plasma environments and space weather)  |
science_cases.txt · Last modified: 2022/09/29 13:49 by admin