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This volume presents a complete and thorough examination of advances in the instrumentation, evaluation, and implementation of UV technology for reliable and efficient data acquisition and analysis. It provides real-world applications in expanding fields such as chemical physics, plasma science, photolithography, laser spectroscopy, astronomy and a
? J. Andersen Niels Bohr Institute for Astronomy Physics and Geophysics Astronomical Observatory Copenhagen [email protected] The development of astronomy worldwide begins at the roots: Already from childhood, humans of all nations and civilizations seem to share an innate fascination with the sky. Yet, people in different regions of the world have vastly different possibilities for pursuing this interest. In wealthy, industrialised societies the way is open to a school or higher education in science, possibly leading to a career in astronomy or basic or applied space science for the benefit of the country as well as the individual. In other regions, neither the financial nor the trained human resources are sufficient to offer that avenue to the future of the young generation, or those intellectual resources to the development of their country. This book addresses ways and means by which these obstacles can be, if not fully overcome, then at least significantly reduced.
Takes a comparative-studies approach to the study of the solar system, with 25 contributions organized into six sections: overviews; interactions between planetary and small body atmospheres with the surrounding plasma medium; chemistry, energetics, and dynamics; models of aeronomic systems; observational applications; and atmospheres of other worlds. Suitable as an overview for graduate students and new professionals in aeronomy, as well as providing synthesis for veterans in the field, with excellent references to guide further research. Mostly b&w illustrations, with a few color plates. Annotation copyrighted by Book News, Inc., Portland, OR.
Traces the historical development of both spectral and imaging methods, placing them in a unified framework relevant to observations of the troposphere, stratosphere, mesosphere, and thermosphere.
Since the successful refurbishment mission, the Hubble Space Telescope has made dramatic and exciting progress in unravelling the nature of sources at high redshift. The upcoming installation of the next generation of instruments will give further impetus to the field, particularly in the infrared spectral region.The proceedings of this landmark meeting review the results of the first three years of post-repair data, including the deepest astronomical images ever obtained: the Hubble Deep Field. This was the first presentation of these exciting results at a major international conference. The interface between HST and ground-based facilities and planned programmes with forthcoming HST instruments are also extensively discussed.