SPECIAL SOFTWARE FOR PLANETARY IMAGE PROCESSING AND RESEARCH

The special modules of photogrammetric processing of remote sensing data that provide the opportunity to effectively organize and optimize the planetary studies were developed. As basic application the commercial software package PHOTOMOD™ is used. Special modules were created to perform various typ...

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Bibliographic Details
Published in:International archives of the photogrammetry, remote sensing and spatial information sciences. remote sensing and spatial information sciences., 2016-01, Vol.XLI-B4, p.529-536
Main Authors: Zubarev, A. E., Nadezhdina, I. E., Kozlova, N. A., Brusnikin, E.S., Karachevtseva, I. P.
Format: Article
Language:English
Subjects:
Cameras
Celestial bodies
Computer software
Data
Data analysis
Data processing
Earth
Earth surface
Enceladus
Galilean satellites
Illumination
Image processing
Jupiter satellites
Mars
Mars satellites
Mercury
Modules
Moon
Navigation
Parameters
Phobos
Photogrammetry
Planetary rovers
Remote sensing
Satellites
Saturn satellites
Software
Spaceborne remote sensing
Submarine pipelines
Thematic mapping
Three dimensional models
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Summary:The special modules of photogrammetric processing of remote sensing data that provide the opportunity to effectively organize and optimize the planetary studies were developed. As basic application the commercial software package PHOTOMOD™ is used. Special modules were created to perform various types of data processing: calculation of preliminary navigation parameters, calculation of shape parameters of celestial body, global view image orthorectification, estimation of Sun illumination and Earth visibilities from planetary surface. For photogrammetric processing the different types of data have been used, including images of the Moon, Mars, Mercury, Phobos, Galilean satellites and Enceladus obtained by frame or push-broom cameras. We used modern planetary data and images that were taken over the years, shooting from orbit flight path with various illumination and resolution as well as obtained by planetary rovers from surface. Planetary data image processing is a complex task, and as usual it can take from few months to years. We present our efficient pipeline procedure that provides the possibilities to obtain different data products and supports a long way from planetary images to celestial body maps. The obtained data – new three-dimensional control point networks, elevation models, orthomosaics – provided accurate maps production: a new Phobos atlas (Karachevtseva et al., 2015) and various thematic maps that derived from studies of planetary surface (Karachevtseva et al., 2016a).
ISSN:2194-9034
1682-1750
2194-9034
DOI:10.5194/isprs-archives-XLI-B4-529-2016