Published July 1, 2011 | Version v1
Journal article

DISTRIBUTION FUNCTIONS OF SIZES AND FLUXES DETERMINED FROM SUPRA-ARCADE DOWNFLOWS

  • 1. Department of Physics, P.O. Box 173840, Montana State University, Bozeman, MT 59717-3840 (United States)
  • 2. NASA/Goddard Space Flight Center, Oak Ridge Associated Universities, 8800 Greenbelt RD, Code 671, Greenbelt, MD 20771 (United States)

Description

The frequency distributions of sizes and fluxes of supra-arcade downflows (SADs) provide information about the process of their creation. For example, a fractal creation process may be expected to yield a power-law distribution of sizes and/or fluxes. We examine 120 cross-sectional areas and magnetic flux estimates found by Savage and McKenzie for SADs, and find that (1) the areas are consistent with a log-normal distribution and (2) the fluxes are consistent with both a log-normal and an exponential distribution. Neither set of measurements is compatible with a power-law distribution nor a normal distribution. As a demonstration of the applicability of these findings to improved understanding of reconnection, we consider a simple SAD growth scenario with minimal assumptions, capable of producing a log-normal distribution.

Availability note (English)

Available from http://dx.doi.org/10.1088/2041-8205/735/1/L6

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal Letters
Journal Volume
735
Journal Issue
1
Journal Page Range
[5 p.]
ISSN
2041-8205

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43040402
Subject category
S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
DISTRIBUTION; DISTRIBUTION FUNCTIONS; MAGNETIC FLUX; MAGNETIC RECONNECTION; SIZE; SOLAR FLARES
Descriptors DEC
FUNCTIONS; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES