DISTRIBUTION FUNCTIONS OF SIZES AND FLUXES DETERMINED FROM SUPRA-ARCADE DOWNFLOWS
Creators
- 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/L6Additional 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