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Author : Richard Frank Donnelly
Publisher : Unknown
Page : 736 pages
File Size : 54,9 Mb
Release : 1979
Category : Cosmic physics
ISBN : MINN:30000010400780
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 744 pages
File Size : 42,7 Mb
Release : 1979
Category : Geophysics
ISBN : UOM:39015017172258
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 528 pages
File Size : 55,9 Mb
Release : 1979
Category : Cosmic physics
ISBN : STANFORD:36105133453683
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 448 pages
File Size : 40,6 Mb
Release : 1979
Category : Geophysics
ISBN : UOM:39015017172324
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 528 pages
File Size : 54,8 Mb
Release : 1979
Category : Geophysics
ISBN : UOM:39015017172217
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 752 pages
File Size : 43,6 Mb
Release : 1979
Category : Ionospheric forecasting
ISBN : UIUC:30112101570262
Author : Kanya Kusano
Publisher : Springer Nature
Page : 470 pages
File Size : 55,7 Mb
Release : 2023-01-31
Category : Science
ISBN : 9789811977657
Powerful solar explosions, such as flares and coronal mass ejections, greatly disturb the electromagnetic environment around the Earth and the atmosphere. They may even impact various social systems—communications, positioning, electric power supply, aviation and activities in space. Such variations in the space environment, which can influence human activities, are called “space weather.” The space weather disaster caused by a solar explosion is a potential risk in modern society. To reduce and mitigate space weather impacts, it is essential to understand the structure and dynamics of the solar–terrestrial environment and to predict the variations. This book comprehensively describes space weather, from the basics of related sciences to the possible social impacts. It was compiled based on a national research project on solar–terrestrial environment prediction conducted in Japan recently. It consists of four parts: the linkage between space weather and society; the magnetosphere of the Earth and space weather prediction; solar storms and space weather prediction; and long-term prediction of solar cycle activity and climate impacts. Each chapter covers the basics and applications of each area, which helps readers gain a broad understanding of the subject matter throughout the book. In addition, readers are able to select and read the topics they are most interested in. It is especially valuable for undergraduate and graduate students and young researchers studying space weather and related topics, and is further helpful for experts in various industries related to space weather disasters. The translation was done with the help of artificial intelligence (machine translation by the service DeepL.com). The present version has been revised technically and linguistically by the authors in collaboration with a professional translator.
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 528 pages
File Size : 46,8 Mb
Release : 1979
Category : Cosmic physics
ISBN : MINN:30000010400798
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 736 pages
File Size : 44,6 Mb
Release : 1979
Category : Ionospheric forecasting
ISBN : UIUC:30112005438350
Author : Roger P. Briggs
Publisher : Unknown
Page : 108 pages
File Size : 55,5 Mb
Release : 1993
Category : Geophysics
ISBN : STANFORD:36105126822043
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 452 pages
File Size : 48,9 Mb
Release : 1979
Category : Ionospheric forecasting
ISBN : UIUC:30112005438376
Author : H. Wang,Ronglan L. Xu
Publisher : Elsevier
Page : 492 pages
File Size : 49,6 Mb
Release : 2002-11-20
Category : Science
ISBN : 0080441106
The COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE) was held in the National Astronomy Observatories of Chinese Academy of Sciences (NAOC) in Beijing, China in September 10-12, 2001. The meeting was focused on five areas of the solar-terrestrial magnetic activity and space environment studies, including study on solar surface magnetism; solar magnetic activity, dynamical response of the heliosphere; space weather prediction; and space environment exploration and monitoring. A hot topic of space research, CMEs, which are widely believed to be the most important phenomenon of the space environment, is discussed in many papers. Other papers show results of observational and theoretical studies toward better understanding of the complicated image of the magnetic coupling between the Sun and the Earth, although little is still known little its physical background. Space weather prediction, which is very important for a modern society expanding into out-space, is another hot topic of space research. However, a long way is still to go to predict exactly when and where a disaster will happen in the space. In that sense, there is much to do for space environment exploration and monitoring. The manuscripts submitted to this Monograph are divided into the following parts: (1) solar surface magnetism, (2) solar magnetic activity, (3) dynamical response of the heliosphere, (4) space environment exploration and monitoring; and (5) space weather prediction. Papers presented in this meeting but not submitted to this Monograph are listed by title as unpublished papers at the end of this book.
Author : Stephen J. Mangis
Publisher : Unknown
Page : 76 pages
File Size : 46,9 Mb
Release : 1975
Category : Geomagnetism
ISBN : MINN:30000010416612
This report is an introduction to solar-terrestrial phenomena for those with no special background in astrophysics or solar astronomy. Discussions of physics have been kept to a minimum, with emphasis on phenomonology instead. An individual completely unfamiliar with solar events should, after reading this volume, be able to read and understand the SESC Report and Forecast of Solar Geophysical Activity and be able to apply its contents to his particular area of concern. This volume is also intended as a quick reference work for Skylab ATM Principal Investigator Teams to assist them in using the ATM data book. For that reason, a list of abbreviations used in forecasts and observatory reports is included. Subjects discussed are solar structure and processes, solar activity, and solar-terrestrial relations. There is a brief description of the Space Environment Services Center's activities.
Author : Giuliana Cini Castagnoli,Antonello Provenzale
Publisher : IOS Press
Page : 528 pages
File Size : 49,5 Mb
Release : 1997
Category : Juvenile Nonfiction
ISBN : 9051993587
The global climate of the Earth has significantly varied over the last millennia. On a regional scale, the climate has varied and does presently vary on many different time scales, leading to a continuously changing pattern of temperatures, humidity, precipitation, with important effects on the whole terrestrial biosphere. Physicist are interested in understanding the mechanism at work by gathering data and properly analysing them, by building theoretical models and, if possible, making predictions on the future evolution of the system. Along these lines, an important question is to understand the role of the solar forcing, in order to unravel the internal mechanisms of variability of the Earth's climate from the variable forcing of the Sun. On the other hand, one can learn about the past solar variability by reading into the terrestrial archives that provide us with proxy data on the history of both the Sun and the climate. Thus, realizing that the Sun and the Earth form a closely coupled system, where the variable properties of the former may affect in many subtle ways the behaviour of the latter, is an important step toward the understanding of both.This book is explicitly devoted to these issues. First, it is important to obtain reliable data from terrestrial archives, and to properly date the records that have been measured. The first part of the book is devoted to these crucial aspects, dealing with various types of proxy data and with the difficult issue of the dating of the records. Once obtained, the data has to be interpreted. This process nowadays relies upon a plethora of data analysis methods that explicitly take into account the nonlinear nature of the system and try to elucidate the dynamics and the main processes active in the measured system. The second part of the book is devoted to the issue of data analysis and prediction. Finally, once the data has been interpreted and analyzed, theoretical models have to be built describing the dynamics of the system considered. Due to the extreme complexity of the Sun/Earth system (as well as of its components, the Sun itself and the Earth's climate), drastic simplifications in the modelling efforts have to be accepted and one has to bear in mind that the models probably are nothing more than a pale image of the real dynamics. The third part of the book is devoted to the theoretical and numerical modelling of the solar and climatic variability, and of their complex interactions. This volume gives an up-to-date view of the present state of this field.
Author : National Research Council,Division on Engineering and Physical Sciences,Space Studies Board,Solar and Space Physics Survey Committee
Publisher : National Academies Press
Page : 196 pages
File Size : 45,7 Mb
Release : 2003-07-01
Category : Science
ISBN : 9780309169196
The sun is the source of energy for life on earth and is the strongest modulator of the human physical environment. In fact, the Sun's influence extends throughout the solar system, both through photons, which provide heat, light, and ionization, and through the continuous outflow of a magnetized, supersonic ionized gas known as the solar wind. While the accomplishments of the past decade have answered important questions about the physics of the Sun, the interplanetary medium, and the space environments of Earth and other solar system bodies, they have also highlighted other questions, some of which are long-standing and fundamental. The Sun to the Earthâ€"and Beyond organizes these questions in terms of five challenges that are expected to be the focus of scientific investigations in solar and space physics during the coming decade and beyond.
