Narrow your search

Library

KU Leuven (10)

ULiège (10)

ULB (8)

Odisee (7)

Thomas More Kempen (7)

Thomas More Mechelen (7)

UCLL (7)

VIVES (7)

LUCA School of Arts (5)

FARO (4)

More...

Resource type

book (17)


Language

English (17)


Year
From To Submit

2021 (4)

2018 (1)

2017 (3)

2015 (1)

2014 (1)

More...
Listing 1 - 10 of 17 << page
of 2
>>
Sort by

Book
Storms from the sun : coronal mass ejections light up the sky.
Author:
Year: 2002 Publisher: [Washington, D.C.] : National Aeronautics and Space Administration,

Loading...
Export citation

Choose an application

Bookmark

Abstract


Book
Storms from the sun : coronal mass ejections light up the sky.
Author:
Year: 2002 Publisher: [Washington, D.C.] : National Aeronautics and Space Administration,

Loading...
Export citation

Choose an application

Bookmark

Abstract


Book
Solar radiation alert system
Authors: --- --- ---
Year: 2005 Publisher: Washington, DC : Office of Aerospace Medicine, U.S. Dept. of Transportation, Federal Aviation Administration,

Loading...
Export citation

Choose an application

Bookmark

Abstract


Book
Solar radiation alert system
Authors: --- --- ---
Year: 2005 Publisher: Washington, DC : Office of Aerospace Medicine, U.S. Dept. of Transportation, Federal Aviation Administration,

Loading...
Export citation

Choose an application

Bookmark

Abstract


Book
Coronal Magnetometry
Authors: --- ---
Year: 2017 Publisher: Frontiers Media SA

Loading...
Export citation

Choose an application

Bookmark

Abstract

Magnetism defines the complex and dynamic solar corona. It determines the magnetic loop structure that dominates images of the corona, and stores the energy necessary to drive coronal eruptive phenomena and flare explosions. At great heights the corona transitions into the ever-outflowing solar wind, whose speed and three-dimensional morphology are controlled by the global coronal magnetic field. Coronal magnetism is thus at the heart of any understanding of the nature of the corona, and essential for predictive capability of how the Sun affects the Earth. Coronal magnetometry is a subject that requires a concerted effort to draw together the different strands of research happening around the world. Each method provides some information about the field, but none of them can be used to determine the full 3D field structure in the full volume of the corona. Thus, we need to combine them to understand the full picture. The purpose of this Frontiers Research Topic on Coronal Magnetometry is to provide a forum for comparing and coordinating these research methods, and for discussing future opportunities.


Book
Coronal Magnetometry
Authors: --- ---
Year: 2017 Publisher: Frontiers Media SA

Loading...
Export citation

Choose an application

Bookmark

Abstract

Magnetism defines the complex and dynamic solar corona. It determines the magnetic loop structure that dominates images of the corona, and stores the energy necessary to drive coronal eruptive phenomena and flare explosions. At great heights the corona transitions into the ever-outflowing solar wind, whose speed and three-dimensional morphology are controlled by the global coronal magnetic field. Coronal magnetism is thus at the heart of any understanding of the nature of the corona, and essential for predictive capability of how the Sun affects the Earth. Coronal magnetometry is a subject that requires a concerted effort to draw together the different strands of research happening around the world. Each method provides some information about the field, but none of them can be used to determine the full 3D field structure in the full volume of the corona. Thus, we need to combine them to understand the full picture. The purpose of this Frontiers Research Topic on Coronal Magnetometry is to provide a forum for comparing and coordinating these research methods, and for discussing future opportunities.

Coronal and stellar mass ejections : proceedings of the 226th Symposium of the International Astronomical Union held in Beijing, China, September 13-17, 2004
Authors: --- --- ---
ISBN: 9780521851978 0521851971 Year: 2005 Publisher: Cambridge : Cambridge University Press,

Loading...
Export citation

Choose an application

Bookmark

Abstract


Book
Coronal Magnetometry
Authors: --- ---
Year: 2017 Publisher: Frontiers Media SA

Loading...
Export citation

Choose an application

Bookmark

Abstract

Magnetism defines the complex and dynamic solar corona. It determines the magnetic loop structure that dominates images of the corona, and stores the energy necessary to drive coronal eruptive phenomena and flare explosions. At great heights the corona transitions into the ever-outflowing solar wind, whose speed and three-dimensional morphology are controlled by the global coronal magnetic field. Coronal magnetism is thus at the heart of any understanding of the nature of the corona, and essential for predictive capability of how the Sun affects the Earth. Coronal magnetometry is a subject that requires a concerted effort to draw together the different strands of research happening around the world. Each method provides some information about the field, but none of them can be used to determine the full 3D field structure in the full volume of the corona. Thus, we need to combine them to understand the full picture. The purpose of this Frontiers Research Topic on Coronal Magnetometry is to provide a forum for comparing and coordinating these research methods, and for discussing future opportunities.


Book
Coronal Mass Ejections : An Introduction
Author:
ISBN: 1441987886 9786613476043 1441987894 1283476045 Year: 2011 Publisher: New York, NY : Springer New York : Imprint: Springer,

Loading...
Export citation

Choose an application

Bookmark

Abstract

In times of growing technological sophistication and of our dependence on electronic technology, we are all affected by space weather. In its most extreme form, space weather can disrupt communications, damage and destroy spacecraft and power stations, and increase radiation exposure to astronauts and airline passengers. Major space weather events, called geomagnetic storms, are large disruptions in the Earth’s magnetic field brought about by the arrival of enormous magnetized plasma clouds from the Sun. Coronal mass ejections (CMEs) contain billions of tons of plasma and hurtle through space at speeds of several million miles per hour. Understanding coronal mass ejections and their impact on the Earth is of great interest to both the scientific and technological communities. This book provides an introduction to coronal mass ejections, including a history of their observation and scientific revelations, instruments and theory behind their detection and measurement, and the status quo of theories describing their onset and evolution through the heliosphere. We present the story behind the life of a CME, from its magnetic field origins in the solar corona and photosphere to its eventual fate deep in the heliosphere. The intention is to provide an easily accessible resource for those who are seeking to learn more about this fascinating and crucial natural phenomenon.

Coronal Mass Ejections
Authors: --- --- --- ---
ISBN: 1281139882 9786611139889 0387450882 0387450866 144192356X Year: 2006 Publisher: New York, NY : Springer New York : Imprint: Springer,

Loading...
Export citation

Choose an application

Bookmark

Abstract

It is well known that the Sun gravitationally controls the orbits of planets and minor bodies. Much less known, however, is the domain of plasma fields and charged particles in which the Sun governs a heliosphere out to a distance of about 15 billion kilometers. What forces activates the Sun to maintain this power? Coronal Mass Ejections (CMEs) and their descendants are the troops serving the Sun during high solar activity periods. This volume offers a comprehensive and integrated overview of our present knowledge and understanding of Coronal Mass Ejections (CMEs) and their descendants, Interplanetary CMEs (ICMEs). It results from a series of workshops held between 2000 and 2004. An international team of about sixty experimenters involved e.g. in the SOHO, ULYSSES, VOYAGER, PIONEER, HELIOS, WIND, IMP, and ACE missions, ground observers, and theoreticians worked jointly on interpreting the observations and developing new models for CME initiations, development, and interplanetary propagation. The book provides researchers active in space physics with an overview of the current understanding of CMEs and ICMEs, and their effects in the heliosphere. It also provides the advanced graduate student with introductory material on this active field of research.

Listing 1 - 10 of 17 << page
of 2
>>
Sort by