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The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters


The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters
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The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters


The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters
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Author : S. W. Kahler
language : en
Publisher:
Release Date : 1981

The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters written by S. W. Kahler and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1981 with Correlation (Statistics) categories.


In previous studies correlating E> 10 MeV proton fluxes and spectra with various associated microwave burst parameters, the resulting high correlations were assumed to reflect a common acceleration process for the protons and the microwave-emitting electrons. We suggest and test an alternative explanation for these correlations, which we term the Big Flare Syndrome (BFS), that states that, statistically, energetic flare phenomena are more intense in larger flares, regardless of the detailed physics. Peak 1-8 A X-ray fluxes, characteristic of the thermal flare, are correlated with peak proton fluxes to derive correlation coefficients characteristics of the BFS. Of all microwave parameters tested for the 1973-1979 period, only the time-integrated flux densities at 8800 and 15400 MHz may be significantly larger than expected form the BFS. We fail to confirm previous results associating peak proton spectra with peak microwave spectral characteristics, thus finding no evidence that peak microwave fluxes are indicative of proton acceleration. We extend this conclusion to peak hard X-ray correlations. The strongly nonlinear relationship deduced between flare energy and proton production also appears invalid.



The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters


The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters
DOWNLOAD
Author : S. W. Kahler
language : en
Publisher:
Release Date : 1981

The Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated Microwave Burst Parameters written by S. W. Kahler and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1981 with Correlation (Statistics) categories.


In previous studies correlating E > 10 MeV proton fluxes and spectra with various associated microwave burst parameters, the resulting high correlations were assumed to reflect a common acceleration process for the protons and the microwave-emitting electrons. We suggest and test an alternative explanation for these correlations, which we term the Big Flare Syndrome (BFS), that states that, statistically, energetic flare phenomena are more intense in larger flares, regardless of the detailed physics. Peak 1-8 A X-ray fluxes, characteristic of the thermal flare, are correlated with peak proton fluxes to derive correlation coefficients characteristics of the BFS. Of all microwave parameters tested for the 1973-1979 period, only the time-integrated flux densities at 8800 and 15400 MHz may be significantly larger than expected form the BFS. We fail to confirm previous results associating peak proton spectra with peak microwave spectral characteristics, thus finding no evidence that peak microwave fluxes are indicative of proton acceleration. We extend this conclusion to peak hard X-ray correlations. The strongly nonlinear relationship deduced between flare energy and proton production also appears invalid.



Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated


Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated
DOWNLOAD
Author : S. W. Kahler
language : en
Publisher:
Release Date : 1981

Role Of The Big Flare Syndrome In Correlations Of Solar Energetic Proton Fluxes And Associated written by S. W. Kahler and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1981 with categories.




Environmental Research Papers


Environmental Research Papers
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Author :
language : en
Publisher:
Release Date : 1981

Environmental Research Papers written by and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1981 with Environmental geology categories.




Energy Research Abstracts


Energy Research Abstracts
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Author :
language : en
Publisher:
Release Date : 1982

Energy Research Abstracts written by and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1982 with Power resources categories.




Astronomy And Astrophysics Abstracts


Astronomy And Astrophysics Abstracts
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Author : S. Böhme
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-12-14

Astronomy And Astrophysics Abstracts written by S. Böhme and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-12-14 with Science categories.


Astronomy and Astrophysics Abstracts, which has appeared in semi-annual volumes since 1969, is devoted to the recording, summarizing and indexing of astronomical publications throughout the world. It is prepared under the auspices of the International Astronomical Union (according to a resolution adopted at the 14th General Assembly in 1970). Astronomy and Astrophysics Abstracts aims to present a comprehensive documenta tion of literature in all fields of astronomy and astrophysics. Every effort will be made to ensure that the average time interval between the date of receipt of the original literature and publication of the abstracts will not exceed eight months. This time interval is near to that achieved by monthly abstracting journals, compared to which our system of accumu lating abstracts for about six months offers the advantage of greater convenience for the user. Volume 31 contains literature published in 1982 and received before July 15, 1982; some older literature which was received late and which is not recorded in earlier volumes is also included. We acknowledge with thanks contributions to this volume by Dr. J. Bouska, Prague, who surveyed journals and publications in Czech and supplied us with abstracts in English .



Solar Energetic Particles


Solar Energetic Particles
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Author : Donald V. Reames
language : en
Publisher: Springer
Release Date : 2017-03-10

Solar Energetic Particles written by Donald V. Reames and has been published by Springer this book supported file pdf, txt, epub, kindle and other format this book has been release on 2017-03-10 with Science categories.


This concise primer introduces the non-specialist reader to the physics of solar energetic particles (SEP) and systematically reviews the evidence for the two main mechanisms which lead to the so-called impulsive and gradual SEP events. More specifically, the timing of the onsets, the longitude distributions, the high-energy spectral shapes, the correlations with other solar phenomena (e.g. coronal mass ejections), as well as the all-important elemental and isotopic abundances of SEPs are investigated. Impulsive SEP events are related to magnetic reconnection in solar flares and jets. The concept of shock acceleration by scattering on self-amplified Alfvén waves is introduced, as is the evidence of reacceleration of impulsive-SEP material in the seed population accessed by the shocks in gradual events. The text then develops processes of transport of ions out to an observer. Finally, a new technique to determine the source plasma temperature in both impulsive and gradual events is demonstrated. Last but not least the role of SEP events as a radiation hazard in space is mentioned and a short discussion of the nature of the main particle telescope designs that have contributed to most of the SEP measurements is given.



Peak Flux Density Spectra Of Large Solar Radio Bursts And Proton Emission From Flares


Peak Flux Density Spectra Of Large Solar Radio Bursts And Proton Emission From Flares
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Author : Edward W. Cliver
language : en
Publisher:
Release Date : 1985

Peak Flux Density Spectra Of Large Solar Radio Bursts And Proton Emission From Flares written by Edward W. Cliver and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1985 with Proton flares categories.


We have reexamined the relationship between U-shaped peak-flux-density microwave spectra and solar proton events for approx 200 large (Sp(> or = 2GHz) > or = 800 solar flux uits (sfu) microwave burst (1965 - 1979). The radio spectra fell into two basic classes: (a) U-shaped with two maxima ( > or = 800 sfu) in the range from 200 MHz to > or = 10 GHz (59 percent of all events), and (b) cutoff spectra with a maximum > or = 800 sfu at f > or = 2 GHz and Sp (200 MHz) 100 sfu (18 percent). Nine percent of the events had intermediate spectra with a maximum or = 800 sfu at f > or = 2 GHz and 100 sfu or = Sp (200 MHz) 800 sfu. We were unable to classify 15 percent of the events because of incomplete data. The associations of the three classes of spectra with Type II (and/or Type IV) meter wavelenght bursts and 10 MeV proton events of any size ( or = 0.01 pr per sq cm per sec per sr) are as follows: U-shaped Type II/IV (90 percent of large microwave bursts with U-shaped spectra are associated with Type II/IV events), protons (77 percent); intermediate Type II/IV (78 percent), protons (73 percent); and cutoff Type II/IV (22 percent), protons (33 percent). These statistics affirm various lines of evidence linking coronal shock waves and interplanetary proton events. They also suggest that the meter wavelength branch of the U-shaped spectrum may be attributable to second phase (vs flash phase) accelerated electrons.



Scientific And Technical Aerospace Reports


Scientific And Technical Aerospace Reports
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Author :
language : en
Publisher:
Release Date : 1985

Scientific And Technical Aerospace Reports written by and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1985 with Aeronautics categories.




Solar Particle Radiation Storms Forecasting And Analysis


Solar Particle Radiation Storms Forecasting And Analysis
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Author : Olga E. Malandraki
language : en
Publisher: Springer
Release Date : 2018-02-01

Solar Particle Radiation Storms Forecasting And Analysis written by Olga E. Malandraki and has been published by Springer this book supported file pdf, txt, epub, kindle and other format this book has been release on 2018-02-01 with Science categories.


Solar energetic particles (SEPs) emitted from the Sun are a major space weather hazard motivating the development of predictive capabilities. This book presents the results and findings of the HESPERIA (High Energy Solar Particle Events forecasting and Analysis) project of the EU HORIZON 2020 programme. It discusses the forecasting operational tools developed within the project, and presents progress to SEP research contributed by HESPERIA both from the observational as well as the SEP modelling perspective. Using multi-frequency observational data and simulations HESPERIA investigated the chain of processes from particle acceleration in the corona, particle transport in the magnetically complex corona and interplanetary space, to the detection near 1 AU. The book also elaborates on the unique software that has been constructed for inverting observations of relativistic SEPs to physical parameters that can be compared with space-borne measurements at lower energies. Introductory and pedagogical material included in the book make it accessible to students at graduate level and will be useful as background material for Space Physics and Space Weather courses with emphasis on Solar Energetic Particle Event Forecasting and Analysis. This book is published with open access under a CC BY license.