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Author : M. A. Shea,D. F. Smart,Susan M. P. McKenna-Lawlor
Publisher : Unknown
Page : 448 pages
File Size : 49,8 Mb
Release : 1984
Category : Comets
ISBN : UOM:39015017172332
Author : Anonim
Publisher : Unknown
Page : 594 pages
File Size : 45,7 Mb
Release : 1988
Category : Aeronautics
ISBN : MINN:31951000607768A
Lists citations with abstracts for aerospace related reports obtained from world wide sources and announces documents that have recently been entered into the NASA Scientific and Technical Information Database.
Author : Anonim
Publisher : Unknown
Page : 1076 pages
File Size : 53,6 Mb
Release : 1989
Category : Power resources
ISBN : MSU:31293010868960
Author : Anonim
Publisher : Unknown
Page : 944 pages
File Size : 49,6 Mb
Release : 1995-11
Category : Government publications
ISBN : UIUC:30112005683476
Author : Anonim
Publisher : Unknown
Page : 942 pages
File Size : 49,6 Mb
Release : 1995
Category : Government publications
ISBN : OSU:32435058894080
Author : Vladimir Evgenʹevich Stepanov,V. N. Obridko
Publisher : VSP
Page : 470 pages
File Size : 50,8 Mb
Release : 1987-12
Category : Science
ISBN : 9067640654
These proceedings contain the review and contributed papers given at the SMY--SMA Workshop held in Irkutsk (USSR), 17--24 June 1985. The main themes of the Workshop were plasma physics and magnetohydrodynamics with applications to processes occurring in solar flares. The papers published in this volume are organized around the following topics: -- the reconnection of coronal magnetic fields as a source of flare energy -- the acceleration of particles to high energies -- the dynamics of interplanetary clouds and shocks
Author : M. Kitamura,E. Budding
Publisher : Springer Science & Business Media
Page : 500 pages
File Size : 50,6 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400944961
M. KITAMURA Tokyo Astronomical Observatory, Japan and E. BUDDING Carter Observatory, Wellington, New Zealand The Third Asian-Pacific Regional Meeting of the International Astronomical Union was held from 30 September to 5 October, 1984, at the Kyoto International Conference Hall, Kyoto, Japan, under the auspices of the Union and the Astronomical Society of Japan with Kyoto University as host. Three hundred and twenty-seven astronomers from twenty-two countries participated at the meeting and more than two hundred papers were presented. The aim of the meeting was not only to promote scientific developments and cooperation, but also to offer a chance for all participants to become acquainted with major astronomical projects of the Asian-Pacific Region. Therefore, two new sessions of 'A View of Asian-Pacific Astronomy' and 'Astronomical Education in the Asian Pacific Region', which had not been undertaken in the previous two Regional Meetings, were arranged as a first trial, besides the other ordinary scientific sessions. The Scientific Organizing Committee consisted of D.C. Morton (chairman), R.N. Manchester, S.M. Gong, K.J. Feng, C.S. Shen, J.C. Bhattacharyya, G. Swa B. Hidayat, H.M.K. AI-Nairniy, H.S. Yun, J.B. Hearnshaw, S.C. Wolff, I. Ka rup, waguchi, M. Kitamura, M. Morimoto, M. Oda, andJ. P. Swings (IAU, ex officio); and the Local Organizing Committee of T. Kogure (chairman), T.lshizawa, M. Saite, R. Hirata, S.lnagaki, E. Hiei, M. Kitamura, B. Takase, N. Kaifu, H. Maehara, Y. Osaki, and A. Yamasaki.
Author : Robert G. Stone,Bruce T. Tsurutani
Publisher : American Geophysical Union
Page : 306 pages
File Size : 55,7 Mb
Release : 1985
Category : Science
ISBN : 9780875900612
Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 35. Violent expansions of the solar corona cause transient shock waves which propagate outward from the sun at hundreds to thousands of kilometers per second; simple solar wind velocity gradients at the surface of the sun lead to high-speed streams overtaking slower streams, forming corotating shocks; and steady state supermagnetosonic solar wind flow past objects such as the planets lead to standing bow shocks. However, the solar wind plasma is so hot and tenuous that charged particle Coulomb collisions produce negligible thermalization or dissipation on scale sizes less than 0.1 AU. The irreversible plasma heating by these shocks is accomplished by wave-particle interactions driven by plasma instabilities. Hence these shocks are described as "collisionless."
Author : Murray Dryer
Publisher : Unknown
Page : 52 pages
File Size : 45,8 Mb
Release : 1982
Category : Magnetic storms
ISBN : UOM:39015095143445
A time-dependent, nonplanar, two-dimensional (2-D) magnetohydrodynamic computer simulation model is used to simulate a series of solar flare-generated shock waves and their subsequent disturbances in interplanetary space between the sun and the earth's magnetosphere. The canonical or anzatz series of shock waves include initial velocities near the sun over the range 500 to 3000 km/sec. The ambient solar wind, through which the shocks propagate, is taken to be a steady-state flow that is independent of heliolongitude; its radial dependency consists of a representative set of plasma and magnetic field parameters which will be presented. Particular attention is directed to the MHD model's ability to address fundamental operational questions regarding the long-range forecasting of geomagnetic disturbances. These questions are: (1) will a disturbance (such as the present canonical series of solar flare shock waves) produce a magnetospheric and ionospheric disturbance, and, if so; (2) when wil it start; (3) how severe will it be; and (4) how long will it last? The model's output is used to compute various solar wind indices of current interest for this purpose. It is concluded that future work should be focused on a cohesive updating of, for example, daily measured solar parameters as input for the model whose output should be compared with spacecraft data for specific events.
Author : Mukul Ranjan Kundu,Bruce Woodgate
Publisher : Unknown
Page : 450 pages
File Size : 51,6 Mb
Release : 1987
Category : Solar flares
ISBN : UOM:39015015941050
Author : Einar Tandberg-Hanssen,A. Gordon Emslie
Publisher : Cambridge University Press
Page : 290 pages
File Size : 47,5 Mb
Release : 1988-11-17
Category : Science
ISBN : 9780521308045
The authors explore solar flares by applying physics and theoretical investigations.
Author : COSPAR. Plenary Meeting
Publisher : Unknown
Page : 372 pages
File Size : 49,9 Mb
Release : 1987
Category : Solar flares
ISBN : STANFORD:36105030447556
Author : Environmental Research Laboratories (U.S.)
Publisher : Unknown
Page : 212 pages
File Size : 48,9 Mb
Release : 1987
Category : Environmental policy
ISBN : UIUC:30112075633179
Author : Arnold O. Benz
Publisher : Springer Science & Business Media
Page : 253 pages
File Size : 44,6 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400947108
Continuum radio emission and fine structure (in particular millisecond spikes) have recently raised interest as diagnostic tools for the interpretation of energy release and particle acceleration in flares. In the circles of the European solar radio astronomers, loosely organized in CESRA, the idea of a workshop came up intended for active observers of the impulsive phase of flares in radio and associated emissions. The scientific organizing committee included A.D. Benz (chairman), A. Magun, M. Pick, G. Trottet, and P. Zlobec. The workshop was held on May 27-31, 1985 in the castle of Duino near Trieste, Italy. The meeting intended to find a common terminology, to compare radio observations with measurements in other emissions and to confront observations with theoretical concepts. We have achieved a representative summary on the current status of the field and a clear perspective for the next cycle. This volume contains the reviews and a selection of contributions and extended abstracts of papers presented at the workshop. I wish to thank the local organizers, in particular A. Abrami, M. Comari, F. Depolli, L. Fornasari, M. Messerotti (chairman), M. Nonino, and P. Zlobec. Financial support was graciously provided by the Italian Research Council (CNR). Most of all, however, I would like to express my thankfulness to our host, His Highness Prince Raimondo della Torre e Tasso, for his invaluable hospitality. We are deeply sorry to hear of his passing in the meantime. To his memory these proceedings are dedicated.
Author : George V. Coyne,Karl Schmitz-Moormann,Christoph Wassermann
Publisher : Labor et Fides
Page : 340 pages
File Size : 41,6 Mb
Release : 1994
Category : Knowledge, Theory of (Religion)
ISBN : 2830907426