Author: Wallace Hall Campbell
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages : 24
Book Description
The purpose of this paper is to introduce the reader to the active sun as a source of disturbance that affect the magnetic field measured at the earth's surface. Included under this topic are the general sun's properties, solar surface activity centers and characteristics of the solar field and ejecta flowing into interplanetary space.
Introduction to Solar Terrestrial Activity for Geomagnetic Studies
Introduction to Solar Terrestrial Activity for Geomagnetic Studies
Author: Wallace Hall Campbell
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages :
Book Description
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages :
Book Description
Introduction to Solar-terrestrial Phenomena and the Space Environment Services Center
Author: Stephen J. Mangis
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages : 76
Book Description
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages : 76
Book Description
Introduction to Solar Terrestrial Activity for Geomagnetic Studies: The earth's main field
Author: Wallace Hall Campbell
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages :
Book Description
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages :
Book Description
Introduction to Solar Terrestrial Activity for Geomagnetic Studies
Author: Wallace Hall Campbell
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages : 24
Book Description
Publisher:
ISBN:
Category : Geomagnetism
Languages : en
Pages : 24
Book Description
Introduction to Solar Terrestrial Activity for Geomagnetic Studies
Author: Wallace Hall Campbell
Publisher:
ISBN:
Category : Solar activity
Languages : en
Pages : 14
Book Description
Publisher:
ISBN:
Category : Solar activity
Languages : en
Pages : 14
Book Description
Solar-Terrestrial Magnetic Activity and Space Environment
Author: H. Wang
Publisher: Elsevier
ISBN: 0080541437
Category : Technology & Engineering
Languages : en
Pages : 475
Book Description
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.
Publisher: Elsevier
ISBN: 0080541437
Category : Technology & Engineering
Languages : en
Pages : 475
Book Description
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.
Introduction to Solar Terrestrial Relations
Author: J. Ortner
Publisher:
ISBN:
Category : Atmosphere, Upper
Languages : en
Pages : 534
Book Description
Publisher:
ISBN:
Category : Atmosphere, Upper
Languages : en
Pages : 534
Book Description
Solar Terrestrial Programs
Author: David Peter Stern
Publisher:
ISBN:
Category : Solar activity
Languages : en
Pages : 114
Book Description
Publisher:
ISBN:
Category : Solar activity
Languages : en
Pages : 114
Book Description
Handbook of the Solar-Terrestrial Environment
Author: Yohsuke Kamide
Publisher: Springer Science & Business Media
ISBN: 3540463143
Category : Science
Languages : en
Pages : 539
Book Description
As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ?? ing energy into space, as much as ?. ? ?? erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di?cult. ?rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth’s the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than ? keV to more than ? GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci?cally the close coupling of di?erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment.
Publisher: Springer Science & Business Media
ISBN: 3540463143
Category : Science
Languages : en
Pages : 539
Book Description
As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ?? ing energy into space, as much as ?. ? ?? erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di?cult. ?rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth’s the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than ? keV to more than ? GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci?cally the close coupling of di?erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment.