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Equatorial Coronal Holes And Their Relation To The High Speed Solar Wind Streams


Equatorial Coronal Holes And Their Relation To The High Speed Solar Wind Streams
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Equatorial Coronal Holes And Their Relation To The High Speed Solar Wind Streams


Equatorial Coronal Holes And Their Relation To The High Speed Solar Wind Streams
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Author : Lidong Xia
language : en
Publisher:
Release Date : 2003

Equatorial Coronal Holes And Their Relation To The High Speed Solar Wind Streams written by Lidong Xia and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2003 with categories.




Coronal Holes And High Speed Wind Streams


Coronal Holes And High Speed Wind Streams
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Author : Jack B. Zirker
language : en
Publisher:
Release Date : 1977

Coronal Holes And High Speed Wind Streams written by Jack B. Zirker and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1977 with Science categories.




Coronal Holes And Solar Wind Acceleration


Coronal Holes And Solar Wind Acceleration
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Author : John L. Kohl
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-11-09

Coronal Holes And Solar Wind Acceleration written by John L. Kohl and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-11-09 with Science categories.


The SOHO-7 Workshop was held from 28 September through 1 October 1998 at the Asticou Inn in Northeast Harbor, Maine. The primary topic of this Workshop was the impact of SOHO observations on our understanding of the nature and evolution of coronal holes and the acceleration and composition of the solar wind. The presentations and discussions occasionally went beyond this topic to include the impact of the reported research on other solar structures and the heliosphere. SOHO (the Solar and Heliospheric Observatory), a project of international cooperation between ESA and NASA, was launched in December 1995 and began its science operations during the first few months of 1996. To many solar and space physicists, it was a great advantage that SOHO began itscomprehensive look at the Sun during the 1996 solar minimum. The qualitatively simple two-phase corona, with polar coronal holes expanding into the high-speed solar wind, and a steady equatorial streamer belt related somehow to the stochastic slow-speed solar wind, allowed various SOHO diagnostics to be initiated with a reasonably well understoodcircumsolar geometry. The analysis of subsequentSOHO measurements made during the rising phase of solar cycle 23 will continue to benefit from what has been learned from the first two years of data.



Correlation Of High Latitude Coronal Holes With Solar Wind Streams High Above Or Below The Ecliptic


Correlation Of High Latitude Coronal Holes With Solar Wind Streams High Above Or Below The Ecliptic
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Author : Kile B. Baker
language : en
Publisher:
Release Date : 1980

Correlation Of High Latitude Coronal Holes With Solar Wind Streams High Above Or Below The Ecliptic written by Kile B. Baker and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1980 with categories.


This report has correlated the positions of high latitude coronal holes as determined from the Helium 10830 A spectroheliograms, with the velocities of solar wind streams high above or below the ecliptic, which could have originated from the same positions as the coronal holes. The solar wind speeds were determined from interplanetary scintillation (IPS) measurements made at the University of California at San Diego and at the Toyokawa Observatory in Japan. The correlation covered the two and a half year period, January 1, 1977 to June 30, 1979, during which there were no large equatorial coronal holes present, since we were approaching solar maximum. We have found that these high latitude coronal holes are often, but not always, correlated to high speed solar wind streams. The lack of a clearer correlation can be attributed to uncertainties in the solar wind velocities obtained from IPS measurements, to uncertainties in the exact boundaries of the coronal holes, and to the deflection or attenuation of relatively weak solar wind streams in interplanetary space.



Coronal Holes And High Speed Wind Streams


Coronal Holes And High Speed Wind Streams
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Author : Jack B. Zirker
language : en
Publisher:
Release Date : 1977

Coronal Holes And High Speed Wind Streams written by Jack B. Zirker and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1977 with Solar wind categories.




Physics Of The Inner Heliosphere Ii


Physics Of The Inner Heliosphere Ii
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Author : Rainer Schwenn
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-06-29

Physics Of The Inner Heliosphere Ii written by Rainer Schwenn and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-06-29 with Science categories.


Physics of the Inner Heliosphere gives for the first time a comprehensive and complete summary of our knowledge of the inner solar system. Using data collected over more than 11 years by the HELIOS twin solar probes, one of the most successful ventures in unmanned space exploration, the authors have compiled six extensive reviews of the physical processes of the inner heliosphere and their relation to the solar atmosphere. Researchers and advanced students in space and plasma physics, astronomy, and solar physics will be surprised to see just how closely the heliosphere is tied to, and how sensitively it depends on, the sun. Volume 2 deals with particles, waves, and turbulence, with chapters on: - magnetic clouds - interplanetary clouds - the solar wind plasma and MHD turbulence - waves and instabilities - energetic particles in the inner solar system



Machine Learning Techniques For Space Weather


Machine Learning Techniques For Space Weather
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Author : Enrico Camporeale
language : en
Publisher: Elsevier
Release Date : 2018-05-31

Machine Learning Techniques For Space Weather written by Enrico Camporeale and has been published by Elsevier this book supported file pdf, txt, epub, kindle and other format this book has been release on 2018-05-31 with Science categories.


Machine Learning Techniques for Space Weather provides a thorough and accessible presentation of machine learning techniques that can be employed by space weather professionals. Additionally, it presents an overview of real-world applications in space science to the machine learning community, offering a bridge between the fields. As this volume demonstrates, real advances in space weather can be gained using nontraditional approaches that take into account nonlinear and complex dynamics, including information theory, nonlinear auto-regression models, neural networks and clustering algorithms. Offering practical techniques for translating the huge amount of information hidden in data into useful knowledge that allows for better prediction, this book is a unique and important resource for space physicists, space weather professionals and computer scientists in related fields. Collects many representative non-traditional approaches to space weather into a single volume Covers, in an accessible way, the mathematical background that is not often explained in detail for space scientists Includes free software in the form of simple MATLAB® scripts that allow for replication of results in the book, also familiarizing readers with algorithms



Corotating Interaction Regions


Corotating Interaction Regions
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Author : A. Balogh
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-06-29

Corotating Interaction Regions written by A. Balogh and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-06-29 with Science categories.


A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. Until recently, however, CIRs could only be observed close to the ecliptic plane, and their three-dimensional structure was therefore not obvious to observers and theoreticians alike. Ulysses was the first spacecraft allowing direct exploration of the third dimen sion of the heliosphere. Since 1992, when it has entered a polar orbit that takes it 0 up to 80 latitude, the spacecraft's performance has been flawless and the mission has provided excellent data from a superbly matched set of instruments. Perhaps the most exciting observation during Ulysses' first passage towards the south pole of the Sun was a strong and long lasting CIR whose energetic particle effects were observed up to unexpectedly high latitudes. These observations, documented in a number of publications, stimulated considerable new theoretical work.



Solar Wind Three


Solar Wind Three
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Author : Christopher T. Russell
language : en
Publisher:
Release Date : 1974

Solar Wind Three written by Christopher T. Russell and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1974 with Solar wind categories.




Physics Of The Solar Corona


Physics Of The Solar Corona
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Author : Constantin J. Macris
language : en
Publisher:
Release Date : 1971

Physics Of The Solar Corona written by Constantin J. Macris and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1971 with Sun categories.