Author: Gennady P. Chernov
Publisher: Springer Science & Business Media
ISBN: 364220015X
Category : Science
Languages : en
Pages : 298
Book Description
The study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a reliable means for both diagnosing the corona and verifying the results of laboratory plasma experiments on wave-wave and wave-particle interactions. This monograph provides a comprehensive review of the fine structure of solar radio bursts. Based on the diversity of experimental data resulting from the progress made in observational techniques, the validity of various theoretical models is reexamined. The book serves as an up-to-date reference work for all researchers in this field.
Fine Structure of Solar Radio Bursts
Author: Gennady P. Chernov
Publisher: Springer Science & Business Media
ISBN: 364220015X
Category : Science
Languages : en
Pages : 298
Book Description
The study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a reliable means for both diagnosing the corona and verifying the results of laboratory plasma experiments on wave-wave and wave-particle interactions. This monograph provides a comprehensive review of the fine structure of solar radio bursts. Based on the diversity of experimental data resulting from the progress made in observational techniques, the validity of various theoretical models is reexamined. The book serves as an up-to-date reference work for all researchers in this field.
Publisher: Springer Science & Business Media
ISBN: 364220015X
Category : Science
Languages : en
Pages : 298
Book Description
The study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a reliable means for both diagnosing the corona and verifying the results of laboratory plasma experiments on wave-wave and wave-particle interactions. This monograph provides a comprehensive review of the fine structure of solar radio bursts. Based on the diversity of experimental data resulting from the progress made in observational techniques, the validity of various theoretical models is reexamined. The book serves as an up-to-date reference work for all researchers in this field.
Interpretation of a special fine structure in type IV solar radio bursts
Author:
Publisher:
ISBN:
Category :
Languages : de
Pages :
Book Description
Publisher:
ISBN:
Category :
Languages : de
Pages :
Book Description
Fine Structure in Metre-Wave Solar Radio Bursts
Author: D. McConnell
Publisher:
ISBN:
Category :
Languages : en
Pages : 6
Book Description
Observations with high time resolution (
Publisher:
ISBN:
Category :
Languages : en
Pages : 6
Book Description
Observations with high time resolution (
The Fibre Fine Structure During Solar Type IV Radio Bursts
Author: Thomas E. X. Bernold
Publisher:
ISBN:
Category :
Languages : en
Pages : 39
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 39
Book Description
The Fibre Fine Structure Duing Solar Type IV Radio Bursts
Author: Thomas E. X. Bernold
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
Fine Structure on the Sun at 2.8 Cm
Author: C. John Grebenkemper
Publisher:
ISBN:
Category :
Languages : en
Pages : 67
Book Description
More than 400 hours of observations of the 2.8 cm solar radio emission were obtained with the Stanford interferometer. The observations were divided into two categories: the emission of the quiet sun and the emission from active regions. The observations of the quiet sun reveal emission from fine structure in addition to the thermal emission component. This fine structure is time varying. One-dimensional power spectra of the variations show that the power decreases as F to the -2 power, and there is no significant peak in the power spectra near the observed optical five-minute oscillations. Four radio bursts were observed during observations of solar active regions. One of these bursts was classified as a simple burst, and the other three were post-burst events. Two of the post-burst events were measured for their circular polarization. The instantaneous one-dimensional resolution of the interferometer shows that the simple burst could have been in the same location as an H-alpha sub-flare which occurred at the same time. The observations of the post-burst events show that they were primarily an enhancement of the pre-existing S-component emission. The percentage of circularly polarized radiation remained essentially unchanged throughout each of the events. A model is proposed for explaining the post-burst observations. (Author).
Publisher:
ISBN:
Category :
Languages : en
Pages : 67
Book Description
More than 400 hours of observations of the 2.8 cm solar radio emission were obtained with the Stanford interferometer. The observations were divided into two categories: the emission of the quiet sun and the emission from active regions. The observations of the quiet sun reveal emission from fine structure in addition to the thermal emission component. This fine structure is time varying. One-dimensional power spectra of the variations show that the power decreases as F to the -2 power, and there is no significant peak in the power spectra near the observed optical five-minute oscillations. Four radio bursts were observed during observations of solar active regions. One of these bursts was classified as a simple burst, and the other three were post-burst events. Two of the post-burst events were measured for their circular polarization. The instantaneous one-dimensional resolution of the interferometer shows that the simple burst could have been in the same location as an H-alpha sub-flare which occurred at the same time. The observations of the post-burst events show that they were primarily an enhancement of the pre-existing S-component emission. The percentage of circularly polarized radiation remained essentially unchanged throughout each of the events. A model is proposed for explaining the post-burst observations. (Author).
Fine Structures of Solar Radio Bursts
Author: Nicolina Chrysaphi
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages :
Book Description
Solar Noise Storms
Author: E. O. Elgaroy
Publisher: Elsevier
ISBN: 1483187985
Category : Science
Languages : en
Pages : 379
Book Description
Solar Noise Storms examines the properties and features of solar noise storm phenomenon. The book also presents some theories that can be used to gain a better understanding of the phenomenon. The coverage of the text includes topics that cover the features and behavior of noise storms, such as the observable features of noise storms; the relationship between noise storms and the observable features on the sun; and ordered behavior of storm bursts in the time-frequency plane. The book also covers the spectrum, polarization, and directivity of noise storms. The text will be of great use to astrophysicists, astronomers, and other scientists concerned with the properties and behaviors of celestial bodies.
Publisher: Elsevier
ISBN: 1483187985
Category : Science
Languages : en
Pages : 379
Book Description
Solar Noise Storms examines the properties and features of solar noise storm phenomenon. The book also presents some theories that can be used to gain a better understanding of the phenomenon. The coverage of the text includes topics that cover the features and behavior of noise storms, such as the observable features of noise storms; the relationship between noise storms and the observable features on the sun; and ordered behavior of storm bursts in the time-frequency plane. The book also covers the spectrum, polarization, and directivity of noise storms. The text will be of great use to astrophysicists, astronomers, and other scientists concerned with the properties and behaviors of celestial bodies.
The Structure of Solar Radio Bursts on a Wavelenght of 10 Cm
Author: Yu. F. Yurovskii
Publisher:
ISBN:
Category :
Languages : en
Pages : 25
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 25
Book Description
The Structure of Solar Radio Bursts on a Wavelength of 10 Cm
Author: Yu. F. Yurovskii
Publisher:
ISBN:
Category :
Languages : en
Pages : 25
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 25
Book Description