Constant-Scale Natural Boundary Mapping to Reveal Global and Cosmic Processes (eBook)

Pamela E. Clark, PhD grew up in New England. Inspired by President John Kennedy, she decided as a child to explore outer space. She thought, “If they can put a man on the moon, they can put a woman (me) on Mars!” She obtained her BA from St. Joseph College. There, she had many opportunities to participate in laboratory research with Sr. Chlorophyll (Dr. Claire Markham) and Sr. Moon Rock (Dr. Mary Ellen Murphy) as well as to coordinate an NSF interdisciplinary undergraduate field research project. While obtaining her PhD in planetary geochemistry from the University of Maryland, she worked at NASA/GSFC outside of Washington DC and the Astrogeology Branch of the USGS in Flagstaff, Arizona, simulating, analyzing, correlating, and interpreting lunar X-ray spectra. She was a member of the group, led by Isidore Adler and Jack Trombka, that pioneered the use of orbital x-ray and gamma-ray spectrometers to determine the composition of planetary surfaces. She participated in the Flagstaff Lunar Data Consortium, the first attempt to create a common format database for all the remote sensing data from a planetary body. After completing her PhD, she joined the technical staff at NASA/JPL, worked with the Goldstone Solar System Radar group, and expanded her remote sensing background to include radar, thermal and near infrared studies of planetary surfaces with particular emphasis on the study of Mercury’s surface. Dr. Clark organized a briefing team to promote a mission to Mercury, and for a while edited the Mercury Messenger newsletter. Springer published the first editions of her book “Dynamic Planet: Mercury in the Context of its Environment” and “Remote Sensing Tools for Exploration”. She eventually returned to Goddard to work with the XGRS team on the NEAR mission to asteroid Eros. Dr. Clark is the science lead in a group initiated by Steve Curtis to develop new paradigms for the design of space missions and vehicles. She is currently involved in developing and evaluating surface science scenarios, tools, technologies, and architectures, and for space missions to extreme environments, with particular emphasis on the Moon and Mars. Dr. Clark has done several stints in academia, including Murray State University in Kentucky, Albright College in Reading, Pennsylvania, and Catholic University of America in Washington DC. She has developed courses in analytical and environmental chemistry, geochemistry, physical geology, mineralogy, optics, planetary astronomy, remote sensing, and physics. Her goals include exploring under every rock to increase the sense of wonder about the solar system.      In Massachusetts under the informal tutelage of Robert Frost, Chuck Clark received an unusual childhood education in architecture. Frost, facing a trip to South America and frustrated by conventional maps’ “stretchy edges,” charged Clark to “Make me a map a heron can use  . . . to get to Brazil!” At first, Clark succeeded only in tearing his father’s road maps, but, undaunted, at ten he began drafting, and by sixteen was a cartographic technician with the US Army Corps of Engineers in Jacksonville, Florida. Crestfallen to learn from his supervisor, Cleve Powell, that “nobody draws world maps anymore. That’s all done numerically,” he set aside his boyhood task and soon enrolled at Georgia Tech, where he showed promise in perspective drafting, freehand sketching, and partial differential equations. After graduation, he migrated to Mbandaka, Zaire, to help Millard Fuller and others found Habitat for Humanity. Later, relying on Frost’s principles—learn to steer water, and to make the part speak for the whole—Clark designed and built museum exhibits that garnered national praise for their “narrative architecture,” and inspired Fred Rogers to add a stoplight to the set of his television show, Mr. Roger’s Neighborhood. At forty-four, Clark was challenged to illustrate certain global symmetries and asymmetries in Earth’s land-water distribution that colleague jim hagan had compared to Egypt’s Great Pyramid. (Clark’s response is within, at Figure 1.3a.) He next made a map showing watersheds, which he discussed with Athelstan Spilhaus, maker of “world maps with natural boundaries.” Clark realized his odd approach was not only distinct from 450 years of tradition, it also used ideas of another childhood mentor, Marston Morse, and, moreover, like his museum exhibits, cloaked form with content. Talks with NOAA’s Dave McAdoo and NASA’s Paul Lowman led to maps of asteroids and acquaintance with the planetary science community. Conference abstracts and posters over the last decade, and especially the concept-extending insights of coauthor P. E. Clark, have explored the possibilities of global maps with constant-scale natural boundaries. (Clark and Clark share New England roots, and, although they have not done the genealogy, may be distant relatives.) When not mapping, Chuck Clark may be found in Atlanta, GA, designing and building pole-type structures, enjoying rambunctious grandchildren, and completing a memoir of his encounters with Frost and Morse.

Chapter One: Constant-Scale Natural Boundary Mapping in Context.- Chapter Two: CSNB Mapping Technique.- Chapter Three: Interpretation of CSNB Maps.- Chapter Four: Mapping the Earth.- Chapter Five: CSNB Mapping Applied to Other Regular Bodies.- Chapter Six: CSNB Mapping Applied to Irregular Bodies.- Chapter Seven: Mapping the Sky.- Chapter Eight: The Future of CSNB Mapping.