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FALSE-ALARM PROBABILITY IN RELATION TO OVERSAMPLED POWER SPECTRA, WITH APPLICATION TO SUPER-KAMIOKANDE SOLAR NEUTRINO DATA
The term "false-alarm probability" denotes the probability that at least one out of M independent power values in a prescribed search band of a power spectrum computed from a white-noise time seriesExpand
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THE KINEMATICS OF GROWING WAVES
This paper is concerned with the problem of distinguishing between amplifying and evanescent waves. These have, in the past, been distinguished by considerations of energy transfer or of the initialExpand
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CORONAL X-RAY BRIGHTNESS AND PHOTOSPHERIC MAGNETIC FIELD: A STUDY IN CORRELATIONS
We have examined correlations between coronal X-ray emission from the Yohkoh Soft X-Ray Telescope (SXT) and photospheric magnetic field measurements from the Michelson Doppler Imager (MDI) on SOHO.Expand
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Maximum energy of semi-infinite magnetic-field configurations
In solar physics and many other areas of astrophysics, one is interested in the properties of magnetic-field configurations that extend out from a given surface that may be termed the "sourceExpand
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Combined and Comparative Analysis of Power Spectra
In solar physics, especially in exploratory stages of research, it is often necessary to compare the power spectra of two or more time series. One may, for instance, wish to estimate what the powerExpand
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Power spectrum analysis of LMSU (Lomonosov Moscow State University) nuclear decay-rate data: Further indication of r-mode oscillations in an inner solar tachocline
Abstract This article presents a power-spectrum analysis of 2350 measurements of the 90 Sr - 90 Y decay process acquired over the interval August 4 2002 to February 6 2009 at the Lomonosov MoscowExpand
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Non-linear effects in electron plasmas
In this investigation of non-linear effects in electron plasmas, the complications of finite boundaries, external fields, non-zero temperature, multi-stream flow and collisions are ignored.Expand
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Asymptotic analysis of force-free magnetic fields of cylindrical symmetry
It is known from computer calculations that if a force-free magnetic-field configuration is stressed progressively by footpoint displacements, the configuration expands and approaches the openExpand
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Coronal Heating: Energy Release Associated with Chromospheric Magnetic Reconnection
We examine a one-dimensional circularly symmetric supergranulation reconnection model with typical quiet-Sun values. In this model, the assumed source rate of elements determines heating, because allExpand
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