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An analysis of gamma ray burst time historiesGamma ray burst time histories, ranging in durations from milliseconds to thousands of seconds, are as varied as the number of bursts. They show a wide array of structures from those that are very smooth to those that contain a seemingly uncountable number of spikes riding on top of other spikes. These profiles have tantalized researchers for years - they obviously hold important information on the nature of GRB's, but to date no one has been successful in analyzing them. For the past year the author has been working on algorithms to analyze these data. Two approaches have been followed in this investigation. The first is an attempt to quantify the amount of structure, or spikiness, in a profile. The second involves applying the latest theorems on chaos and fractals with the aim of extracting useful information from what seems to be a random collection of shot noise.
Document ID
19940020717
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lestrade, John Patrick
(Alabama Univ. Huntsville, AL, United States)
Karr, Gerald R.
(Alabama Univ. Huntsville, AL, United States)
Date Acquired
September 6, 2013
Publication Date
February 1, 1994
Subject Category
Space Radiation
Report/Patent Number
UAH-5-30166
NAS 1.26:195191
NASA-CR-195191
Report Number: UAH-5-30166
Report Number: NAS 1.26:195191
Report Number: NASA-CR-195191
Meeting Information
Meeting: Summer Faculty Fellowship Research Continuation Program
Location: Huntsville, AL
Country: United States
Start Date: February 1, 1994
End Date: February 28, 1994
Sponsors: Alabama Univ.
Accession Number
94N25199
Funding Number(s)
CONTRACT_GRANT: NAG8-212
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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