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Fiske and Fisk family
Being the record of the descendants of Symond Fiske, lord of the manor of Stadhaugh, Suffolk County, England, from the time of Henry IV to date, including all the American members of the family
Relativistic Astrophysics and Cosmology
This book constitutes the proceedings of the 13th Course of the International School of Cosmic Ray Astrophysics. It focuses on major areas of astrophysics, their relation to cosmic ray physics, and our current understanding of the energetic processes in the Galaxy and the Universe that govern the acceleration and form the features of the cosmic rays that we detect at Earth. The proceedings have been selected for coverage in: . OCo Index to Scientific & Technical Proceedings (ISTP CDROM version / ISI Proceedings). OCo CC Proceedings OCo Engineering & Physical Sciences."
The 3-D Heliosphere at Solar Maximum
The global structure of the heliosphere changes dramatically with the solar circle. Our knowledge of the heliosphere in three dimensions under solar-minimum conditions has advanced significantly in the last 10 years, largely as a result of the on-going ESA/NASA Ulysses mission. Similar advances in our understanding of the heliosphere at solar maximum are to be expected with the return of Ulysses to the Sun's polar regions in 2000/2001. The papers in this volume address a wide range of topics related to the solar-maximum heliosphere, and include many of the latest findings from Ulysses and other space-based missions. Ground-based studies and theoretical modeling are also well represented. Specific questions include: what are the dominant processes that determine the global structure of the inner heliosphere under conditions of high solar activity, and what are the key differences between the high-latitude heliosphere at solar maximum and solar minimum? The book is intended for those carrying out active research in the fields of solar and heliospheric physics.
From the Outer Heliosphere to the Local Bubble
Knowledge about the outer heliosphere and the interstellar medium, which were long treated as two separate fields, has improved dramatically over the past 25 years as a consequence of recent developments: The discovery of interstellar pickup ions and neutral helium inside the heliosphere, the determination of the interstellar hydrogen distribution in the heliosphere obtained using backscattered solar Lyman-alpha radiation, the prediction and subsequent detection of the hydrogen wall just outside of the heliopause, the development of detailed global models for the interaction of solar wind plasma with the interstellar medium, and most recently, direct in-situ plasma and field measurements ins...
Bulletin
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Corotating Interaction Regions
This volume gives a comprehensive and integrated overview of current knowledge and understanding of corotating interaction regions (CIRs) in the solar wind. It is the result of a workshop at ISSI, where space scientists involved in the Ulysses, Pioneer, Voyager, IMP-8, Wind, and SOHO missions exchanged their data and interpretations with theorists in the fields of solar and heliospheric physics. The book provides a broad synthesis of current understanding of CIRs, which form at the interface between the fast solar wind originating in the northern and southern coronal holes and the slow solar wind that originates near and within coronal streamers surrounding the heliomagnetic equator. CIRs ar...
The American Missionary
Vols. 13-62 include abridged annual reports and proceedings of the annual meetings of the American Missionary Association, 1869-1908; v. 38-62 include abridged annual reports of the Society's Executive committee, 1883/84-1907/1908.
