skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Characteristics of Low-latitude Coronal Holes near the Maximum of Solar Cycle 24

Journal Article · · Astrophysical Journal
; ; ;  [1];  [2];  [3];  [4]
  1. University of Graz, Institute of Physics, IGAM-Kanzelhöhe Observatory, Graz (Austria)
  2. National Space Institute, DTU Space (Denmark)
  3. Hvar Observatory, Faculty of Geodesy, Zagreb (Croatia)
  4. Universität Kiel, Institut für Experimentelle und Angewandte Physik, Kiel (Germany)

We investigate the statistics of 288 low-latitude coronal holes extracted from SDO /AIA-193 filtergrams over the time range of 2011 January 01–2013 December 31. We analyze the distribution of characteristic coronal hole properties, such as the areas, mean AIA-193 intensities, and mean magnetic field densities, the local distribution of the SDO /AIA-193 intensity and the magnetic field within the coronal holes, and the distribution of magnetic flux tubes in coronal holes. We find that the mean magnetic field density of all coronal holes under study is 3.0 ± 1.6 G, and the percentaged unbalanced magnetic flux is 49 ± 16%. The mean magnetic field density, the mean unsigned magnetic field density, and the percentaged unbalanced magnetic flux of coronal holes depend strongly pairwise on each other, with correlation coefficients cc > 0.92. Furthermore, we find that the unbalanced magnetic flux of the coronal holes is predominantly concentrated in magnetic flux tubes: 38% (81%) of the unbalanced magnetic flux of coronal holes arises from only 1% (10%) of the coronal hole area, clustered in magnetic flux tubes with field strengths >50 G (10 G). The average magnetic field density and the unbalanced magnetic flux derived from the magnetic flux tubes correlate with the mean magnetic field density and the unbalanced magnetic flux of the overall coronal hole (cc>0.93). These findings give evidence that the overall magnetic characteristics of coronal holes are governed by the characteristics of the magnetic flux tubes.

OSTI ID:
22663893
Journal Information:
Astrophysical Journal, Vol. 835, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

Measurements of EUV coronal holes and open magnetic flux
Journal Article · Mon Mar 10 00:00:00 EDT 2014 · Astrophysical Journal · OSTI ID:22663893

OFF-LIMB SOLAR CORONAL WAVEFRONTS FROM SDO/AIA EXTREME-ULTRAVIOLET OBSERVATIONS-IMPLICATIONS FOR PARTICLE PRODUCTION
Journal Article · Wed Jun 01 00:00:00 EDT 2011 · Astrophysical Journal Letters · OSTI ID:22663893

SIGMOID-TO-FLUX-ROPE TRANSITION LEADING TO A LOOP-LIKE CORONAL MASS EJECTION
Journal Article · Fri Dec 10 00:00:00 EST 2010 · Astrophysical Journal Letters · OSTI ID:22663893