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Author : Iver H. Cairns
Publisher :
ISBN 13 :
Total Pages : 10 pages
Book Rating : 4.:/5 (212 download)
Download or read book Nonlinear Processes in Type III Solar Radio Bursts written by Iver H. Cairns and published by . This book was released on 1995 with total page 10 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Iver H. Cairns
Publisher :
ISBN 13 :
Total Pages : 10 pages
Book Rating : 4.:/5 (127 download)
Download or read book Nonlinear Process in Type III Solar Radio Bursts written by Iver H. Cairns and published by . This book was released on 1995 with total page 10 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Dean Francis Smith
Publisher :
ISBN 13 :
Total Pages : 130 pages
Book Rating : 4.F/5 ( download)
Download or read book A Model for Type III Solar Radio Bursts written by Dean Francis Smith and published by . This book was released on 1969 with total page 130 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Peter H. Yoon
Publisher : Cambridge University Press
ISBN 13 : 1316772187
Total Pages : 365 pages
Book Rating : 4.3/5 (167 download)
Download or read book Classical Kinetic Theory of Weakly Turbulent Nonlinear Plasma Processes written by Peter H. Yoon and published by Cambridge University Press. This book was released on 2019-09-12 with total page 365 pages. Available in PDF, EPUB and Kindle. Book excerpt: Kinetic theory of weakly turbulent nonlinear processes in plasma helped form the foundation of modern plasma physics. This book provides a systematic overview of the kinetic theory of weak plasma turbulence from a modern perspective. It covers the fundamentals of weak turbulence theory, including the foundational concepts and the mathematical and technical details. Some key obstacles to space plasma applications are also covered, including the origin of non-thermal charged particle population, and radio burst phenomena from the sun. Treating both collective and discrete particle effects, the book provides a valuable reference for researchers looking to familiarize themselves with plasma weak turbulence theory.
Author : Gennady P. Chernov
Publisher : Springer Science & Business Media
ISBN 13 : 364220015X
Total Pages : 298 pages
Book Rating : 4.6/5 (422 download)
Download or read book Fine Structure of Solar Radio Bursts written by Gennady P. Chernov and published by Springer Science & Business Media. This book was released on 2011-06-28 with total page 298 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.
Author : Vratislav Krupař
Publisher :
ISBN 13 :
Total Pages : 0 pages
Book Rating : 4.:/5 (115 download)
Download or read book Stereoscopic Observations of Solar Radio Emissions by the S/Waves Instrument Onboard the STEREO Spacecraft written by Vratislav Krupař and published by . This book was released on 2019 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt: This PhD thesis is primarily dedicated to a study of type III radio bursts observed by the S/Waves instrument onboard Solar TErrestrial RElations Observatory (STEREO). These emissions are produced by beams of suprathermal electrons escaping the corona along open magnetic field lines during increased solar activity. As fast electrons propagate in the interplanetary (IP) medium, Langmuir waves are generated at the local electron plasma frequency fpe by bump-on-tail instability and can be afterwards converted by a non linear process into radio emissions at fpe and/or 2 fpe : type III radio bursts. We have developed a goniopolarimetric (GP, also referred to as direction-finding) inversion using the Singular Value Decomposition (SVD) technique for electric measurements on three non-orthogonal antennas. It allows us to retrieve both wave vector directions and polarization properties of incident waves. We also investigated the influence of extended sources (as a typical feature of type III radio bursts) on measured spectral matrices. We have found an empirical relation between apparent source sizes and spectral matrices decomposed by SVD. Abovementioned techniques have been extensively tested on data obtained by the High Frequency Receiver (HFR, a part of S/Waves). We have compared flux densities and GP products of several intense radio bursts observed simultaneously by the two STEREO spacecraft and the Wind spacecraft (using the spin demodulation method for the GP inversion) during small separation distances with satisfary results. We have performed statistical analysis of a large number of type III radio bursts observed by STEREO between May 2007 and September 2011. Only intense, simple, and isolated cases have been included in our data set. We have found that the maximum flux density occurs around 1 MHz. The apparent source size is very extended (∼40°) for frequencies above 500 kHz while remaining almost constant (∼25°) between 500 kHz and 2 MHz. Calculated positions of radio sources suggest that scattering of the primary beam pattern plays an important role in the propagation of type III radio bursts in the IP medium.
Author : Dastgeer Shaikh
Publisher : AIP Conference Proceedings / A
ISBN 13 :
Total Pages : 454 pages
Book Rating : 4.:/5 (318 download)
Download or read book Turbulence and Nonlinear Processes in Astrophysical Plasmas written by Dastgeer Shaikh and published by AIP Conference Proceedings / A. This book was released on 2007-09-27 with total page 454 pages. Available in PDF, EPUB and Kindle. Book excerpt: This book contains the peer-reviewed papers presented at the Sixth Annual International Astrophysics Conference. This conference brought together a range of topics that shed light on our understanding and status of turbulence and nonlinear processes in astrophysical plasmas. Coverage in this volume includes turbulent relaxation in laboratory and space plasmas and its application to coronal flux tubes, coronal heating, and the diffusion of energetic particles.
Author :
Publisher :
ISBN 13 :
Total Pages : 1298 pages
Book Rating : 4.E/5 ( download)
Download or read book Nuclear Science Abstracts written by and published by . This book was released on 1974 with total page 1298 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Stanford University. Microwave Laboratory
Publisher :
ISBN 13 :
Total Pages : 11 pages
Book Rating : 4.F/5 ( download)
Download or read book Type III Solar Radio Bursts written by Stanford University. Microwave Laboratory and published by . This book was released on 1963 with total page 11 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : E.R. Priest
Publisher : Springer Science & Business Media
ISBN 13 : 9780792308799
Total Pages : 574 pages
Book Rating : 4.3/5 (87 download)
Download or read book Basic Plasma Processes on the Sun written by E.R. Priest and published by Springer Science & Business Media. This book was released on 1990-09-30 with total page 574 pages. Available in PDF, EPUB and Kindle. Book excerpt: Much of the excitement in modern Solar Physics has come from the realisation that the Sun is a plasma and that this plasma is interacting with the magnetic field in a wide variety of subtle ways. As well as being of great interest in their own right the observed plasma phenomena on the Sun are of much wider importance, since they reveal to us details of basic phenomena that are expected to be occurring throughout the universe. It was with this in mind that 173 solar physicists from 17 countries gathered together in Bangalore with an air of anticipation. We were not disappointed as we received the warmest of welcomes from our graceful and charming host,Vinod Krishan. She and her colleagues worked tirelessly to make our stay a most memorable one and to ensure that the meeting ran with calm and efficiency. In addition to being stimulated by an excellent series of talks on the up-to-the minute advances in our subject, it was a pleasure to make new friendships from so many countries and to learn, in particular, of the Solar Physics being done in India which has a great tradition and is of a high standard. Furthermore, we enjoyed hearing about Indian culture and appreciating its beauty, especially on our day's tour into the countryside to visit some Hindu and Jain temples.
Author : Michel Poquerusse
Publisher :
ISBN 13 :
Total Pages : pages
Book Rating : 4.:/5 (128 download)
Download or read book Relativistic Type III Solar Radio Bursts written by Michel Poquerusse and published by . This book was released on 1994 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Kenneth E. Eis
Publisher :
ISBN 13 :
Total Pages : 82 pages
Book Rating : 4.3/5 (91 download)
Download or read book An Observer's Manual for the Air Force Swept Frequency Interferometric Radiometer written by Kenneth E. Eis and published by . This book was released on 1978 with total page 82 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Iver H. Cairns
Publisher :
ISBN 13 :
Total Pages : 12 pages
Book Rating : 4.:/5 (212 download)
Download or read book The Stochastic Growth Theory for Type III Solar Radio Bursts written by Iver H. Cairns and published by . This book was released on 1995 with total page 12 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Michel Poquerusse
Publisher :
ISBN 13 :
Total Pages : 16 pages
Book Rating : 4.:/5 (127 download)
Download or read book Non-collisional Decay of Solar Type U Radio Bursts written by Michel Poquerusse and published by . This book was released on 1984 with total page 16 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : Sonja Vidojevic
Publisher :
ISBN 13 :
Total Pages : 0 pages
Book Rating : 4.:/5 (956 download)
Download or read book Statistics of Langmuir Waves Associated with Type III Solar Radio Bursts written by Sonja Vidojevic and published by . This book was released on 2013 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author :
Publisher :
ISBN 13 :
Total Pages : 452 pages
Book Rating : 4.6/5 (248 download)
Download or read book Instrumentation Papers written by and published by . This book was released on with total page 452 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author : John P. Castelli
Publisher :
ISBN 13 :
Total Pages : 24 pages
Book Rating : 4.3/5 (91 download)
Download or read book The Great Burst of May 23, 1967 written by John P. Castelli and published by . This book was released on 1967 with total page 24 pages. Available in PDF, EPUB and Kindle. Book excerpt: One of the largest radio bursts on record took place on May 23, 1967. Peak flux densities ranged between 23,000 flux units (10 to the minus 22nd power sq Wm/Hz) at 8800 MHz to about 370,000 units at 606 MHz. In addition to the high accuracy measurements of the peak flux densities at 606, 1415, 2695, 4995, and 8800 MHz, sweep frequency observations from 19 to 41 MHz show Type IV emission with Type II bursts occurring during the Type IV continuum. The associated flare was clearly visible in white light. In reviewing and compiling microwave radio data recorded during earlier white-light flares, it was found that all but one of eight events listed by Svestka (1966) had high microwave flux densities associated with them. In comparing radio burst intensity with optical flare importance for the series of three flares between 1809 and 2150 UT on May 23, 1967, there is only moderate agreement. The first radio burst was small; the second flare had the highest optical classification, while the third radio burst was by far the largest. The flux densities of the third radio burst may have been the highest ever recorded in the decimeter portion of the radio spectrum and among the largest four in the 8800 MHz region. It is suggested that the details of the development of the flare be followed on radio flux density plots to determine detailed correlation with particle events in space and with terrestrial effects. (Author).
