Author: Itahiza Francisco Domínguez Cerdeña
Publisher:
ISBN: 9783936586312
Category :
Languages : en
Pages : 111
Book Description
Quiet Sun Magnetic Fields
Author: Itahiza Francisco Domínguez Cerdeña
Publisher:
ISBN: 9783936586312
Category :
Languages : en
Pages : 111
Book Description
Publisher:
ISBN: 9783936586312
Category :
Languages : en
Pages : 111
Book Description
Dynamics of Quiet Sun Magnetic Fields
Author: C. Denker
Publisher:
ISBN:
Category : Solar magnetic fields
Languages : en
Pages :
Book Description
Publisher:
ISBN:
Category : Solar magnetic fields
Languages : en
Pages :
Book Description
Properties of the Quiet Sun Magnetic Fields as Reveald Through the Spectrovideomagnetograph
Author: Harold Zirin
Publisher:
ISBN:
Category : Solar magnetic fields
Languages : en
Pages :
Book Description
Publisher:
ISBN:
Category : Solar magnetic fields
Languages : en
Pages :
Book Description
The Quiet Sun
Author: Edward G. Gibson
Publisher:
ISBN:
Category : Solar activity
Languages : en
Pages : 362
Book Description
An up-to-date textbook of solar physics is presented. The solar structure and processes, and the interior are described along with the photosphere, the chromosphere, and the corona. The strongest Fraunhofer lines, visible coronal lines, and coronal UV, XUV, and X-ray lines are listed.
Publisher:
ISBN:
Category : Solar activity
Languages : en
Pages : 362
Book Description
An up-to-date textbook of solar physics is presented. The solar structure and processes, and the interior are described along with the photosphere, the chromosphere, and the corona. The strongest Fraunhofer lines, visible coronal lines, and coronal UV, XUV, and X-ray lines are listed.
The Appearance and Disappearance of Magnetic Flux on the Quiet Sun
Author: Harold Zirin
Publisher:
ISBN:
Category :
Languages : en
Pages : 19
Book Description
This project yielded the following significant new discoveries and findings about solar magnetic fields: The majority of magnetic flux on the sun is observed to disappear when magnetic fields of one polarity migrate into or develop in juxtaposition with fields of opposite polarity. The cancellation of magnetic fields can be interpreted as: (a) submergence (b) reconnection or (c) dissipation (annihilation) of magnetic fields. Large-scale filaments are observed to form in the chromosphere immediately above the boundaries between areas of network magnetic field of opposite polarity where network cancellation occurs. Small-scale filaments develop in association with small-scale cancelling magnetic fields at the rate of hundreds per day. Magnetic fields associated with large-scale solar convection cells, known as intranetwork magnetic fields, can be detected everywhere on the visible disk of the sun by using the videomagnetograph to integrate successive, 1/15 sec. magnetic field images for intervals of 1 to 10 minutes. The intranetwork field appear to be a few seconds of arc in diameter, and have field strengths of the order of a few Gauss to tens of Gauss. The intranetwork fields appear to originate at the centers of supergranules and flow to the boundaries of the cells in approximately radial patterns.
Publisher:
ISBN:
Category :
Languages : en
Pages : 19
Book Description
This project yielded the following significant new discoveries and findings about solar magnetic fields: The majority of magnetic flux on the sun is observed to disappear when magnetic fields of one polarity migrate into or develop in juxtaposition with fields of opposite polarity. The cancellation of magnetic fields can be interpreted as: (a) submergence (b) reconnection or (c) dissipation (annihilation) of magnetic fields. Large-scale filaments are observed to form in the chromosphere immediately above the boundaries between areas of network magnetic field of opposite polarity where network cancellation occurs. Small-scale filaments develop in association with small-scale cancelling magnetic fields at the rate of hundreds per day. Magnetic fields associated with large-scale solar convection cells, known as intranetwork magnetic fields, can be detected everywhere on the visible disk of the sun by using the videomagnetograph to integrate successive, 1/15 sec. magnetic field images for intervals of 1 to 10 minutes. The intranetwork field appear to be a few seconds of arc in diameter, and have field strengths of the order of a few Gauss to tens of Gauss. The intranetwork fields appear to originate at the centers of supergranules and flow to the boundaries of the cells in approximately radial patterns.
Magnetic Fields and Supergranule Velocity Fields on the Quiet Sun
Author: Haimin Wang
Publisher:
ISBN:
Category : Solar granulation
Languages : en
Pages : 217
Book Description
Publisher:
ISBN:
Category : Solar granulation
Languages : en
Pages : 217
Book Description
Stochastic Analysis of the Quiet Sun Magnetic Field Evolution
Author: Andriy Gorobets
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
Solar Magnetic Fields Study
Author: Robert C. Smithson
Publisher:
ISBN:
Category :
Languages : en
Pages : 19
Book Description
High resolution observations of quiet sun magnetic fields have been made at Sacramento Peak Observatory using the Lockheed Universal Filter. The existence of 'salt and pepper' fields described by other observers has been called into question. (Author).
Publisher:
ISBN:
Category :
Languages : en
Pages : 19
Book Description
High resolution observations of quiet sun magnetic fields have been made at Sacramento Peak Observatory using the Lockheed Universal Filter. The existence of 'salt and pepper' fields described by other observers has been called into question. (Author).
Diffraction-limited Spectropolarimetry of Quiet-Sun Magnetic Fields
Author: David Orozco Suárez
Publisher:
ISBN: 9788469156940
Category :
Languages : en
Pages : 222
Book Description
Publisher:
ISBN: 9788469156940
Category :
Languages : en
Pages : 222
Book Description
The Quiet Sun
Author: Edward G. Gibson
Publisher:
ISBN:
Category : Government publications
Languages : en
Pages : 356
Book Description
Publisher:
ISBN:
Category : Government publications
Languages : en
Pages : 356
Book Description