Guide To Magellan Image Interpretation

Guide to Magellan Image Interpretation

Guide to Magellan Image Interpretation

An overview of Magellan Mission requirements, radar system characteristics, and methods of data collection is followed by a description of the image data, mosaic formats, areal coverage, resolution, and pixel DN-to-dB conversion. The availability and sources of image data are outlined. Applications of the altimeter data to estimate relief, Fresnel reflectivity, and surface slope, and the radiometer data to derive microwave emissivity are summarized and illustrated in conjunction with corresponding SAR image data. Same-side and opposite-side stereo images provide examples of parallax differences from which to measure relief with a lateral resolution many times greater than that of the altimeter. Basic radar interactions with geologic surfaces are discussed with respect to radar-imaging geometry, surface roughness, backscatter modeling, and dielectric constant. Techniques are described for interpreting the geomorphology and surface properties of surficial features, impact craters, tectonically deformed terrain, and volcanic landforms. The morphologic characteristics that distinguish impact craters from volcanic craters are defined. Criteria for discriminating extensional and compressional origins of tectonic features are discussed. Volcanic edifices, constructs, and lava channels are readily identified from their radar outlines in images. Geologic map units are identified on the basis of surface texture, image brightness, pattern, and morphology. Superposition, cross-cutting relations, and areal distribution of the units serve to elucidate the geologic history. Ford, John P. and Plaut, Jeffrey J. and Weitz, Catherine M. and Farr, Tom G. and Senske, David A. and Stofan, Ellen R. and Michaels, Gregory and Parker, Timothy J. and Fulton, D. (Editor) Jet Propulsion Laboratory GEOMORPHOLOGY; IMAGE ANALYSIS; MAGELLAN PROJECT (NASA); PLANETARY CRATERS; PLANETARY GEOLOGY; PLANETARY SURFACES; RADAR IMAGERY; SURFACE PROPERTIES; SURFACE ROUGHNESS; TECTONICS; LAVA; MICROWAVE EMISS...

Spacecraft that Explored the Inner Planets Venus and Mercury

A series of increasingly capable spacecraft were sent to explore the inner planets Venus and Mercury. The history of that planetary exploration is traced in this book along with the evolution of sophisticated spacecraft that unveiled long-sought secrets of the planets. The spacecraft were ingenious and reflected the best efforts of talented people working with the available technology of the day. Additionally, this book showcases engineering involved in those capable machines. A consecutive series of 34 planetary spacecraft, which span the time period 1961 to 2021, are described. This includes the unsuccessful missions of several early spacecraft that paved the way for a better understanding of Venus’ hostile environments. This book will describe many successful spacecraft sent to Venus by the Soviet Union and many successful spacecraft sent to Venus and to Mercury by the United States. The recent exploration of Venus by the European Space Agency’s Venus Express and the Japanese spacecraft Akatsuki can also be found in this book. The author draws on over 50 years of experience on aircraft and spacecraft systems to tell the story of these planetary spacecraft. The spacecraft experience includes being the technical lead for the landing radars on the Surveyor and Apollo lunar landers as well as providing analyses for the rendezvous radar for the Space Shuttle. Practical engineering experience is augmented by Master’s degrees in electrical engineering, physics, and business administration.