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Physics of Space: Growth Points and Problems
Proceedings of the Second "Rencontres de l'observatoire", Observatoire de Paris, Meudon, France
Measurement Techniques in Space Plasmas
Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 103. Space plasma measurements are conducted in a hostile, remote environment. The art and science of measurements gathered in space depend therefore on unique instrument designs and fabrication methods to an extent perhaps unprecedented in experimental physics. In-situ measurement of space plasmas constitutes an expensive, unforgiving, and highly visible form of scientific endeavor.
The 3-D Heliosphere at Solar Maximum
Our knowledge of the heliosphere in three dimensions near solar minimum has advanced significantly in the last 10 years, largely as a result of the on-going ESAINASA Ulysses mission. Similar advances in our understanding of the global heliosphere near solar maximum are to be expected with the return of Ulysses to high solar latitudes in 2000/200 I. With this in mind, the 34th ESLAB Symposium, held at ESTEC in Noordwijk, The Netherlands, on 3-6 October, 2000, was devoted to 'The 3-D Heliosphere at Solar Maximum'. This was the third ESLAB Sympo sium focusing on the three-dimensional heliosphere (previous symposia being in 1985 and 1994), and the timing was particularly appropriate, marking as ...
Handbook of Space Resources
Earth has limited material and energy resources, while these resources are virtually unlimited in space. It is only a matter of time, before planetary resources are mined and used in-situ to sustain human and robotic exploration or returned to Earth for commercial gain. This book covers a number of aspects related to space resources. In particular, subjects related to mission concepts, exploration approaches, mining and extraction technologies, commercial potential, and regulatory aspects of space resources are covered in detail. This book is therefore a good resource for readers who seek background and deeper understanding of space resources related activities.
Meteorology
None
Solar Wind Nine: Proceedings of the Ninth International Solar Wind Conference
Marked by four themes: origin of the solar wind, internal state of the solar wind, large scale structure and dynamics, and the outer heliosphere.
Solar Wind Ten
The Tenth Solar Wind conference describes the latest results in the physics of the outer solar atmosphere, the solar wind, and the interplanetary medium which together comprise the heliosphere. The conference brought together researchers studying the sun and its influence on the earth’s space environment both from an experimental and theoretical point of view. The effect of the solar magnetic field in shaping and accelerating the solar wind throughout the solar cycle, via coronal heating and coronal mass ejections was described in unprecedented clarity and breadth, thanks to both satellite experiments and numerical modelling. The conference proceedings is of interest to researchers in space science and the geomagnetic effects of solar activity, plasma physicists and astrophysicists as well as other scientists interested in the life of our mother star.
Future Perspectives of Space Plasma and Particle Instrumentation and International Collaborations
Future perspectives on space-borne/ground-based state-of-the-art scientific instruments, exploration space missions, and advanced modeling/simulation methods, are intensively discussed from multilateral viewpoints regarding solar-terrestrial physics, space plasma, upper atmospheric observations for the Earth and planets. In addition to innovative technologies, international collaborations have been getting more essential and crucial factors in the space observations/missions. The novel concept, strategy, and promotion in these international collaborations are also main subjects of this conference.
Radio Astronomy at Long Wavelengths
The first reports back from what has until now been an unexplored region of the radiomagnetic spectrum, from 30 kHz and a wavelength of ten kilometers to about 30 MHz and a wavelength of ten meters, three orders of frequency magnitude just below the standard radion astronomy region. The 36 tutorials and reviews from an October conference in Paris, France consider the generation of radio waves, propagation and scattering, long wavelength radio emission from the solar system and from galactic and extragalactic sources, and radio telescopes for long wavelength observations and sounding. They include a few color plates, but are not indexed. Annotation copyrighted by Book News, Inc., Portland, OR.
