Flux distribution of solar intranetwork magnetic fields
Abstract
Big Bear deep magnetograms of June 4, 1992 provide unprecedented observations for direct measurements of solar intranetwork (IN) magnetic fields. More than 2500 individual IN elements and 500 network elements are identified and their magnetic flux measured in a quiet region of 300 × 235 arc sec. The analysis reveals the following results: IN element flux ranges from 1016 Mx (detection limit) to 2 × 1018 Mx, with a peak flux distribution of 6 × 1016 Mx.
- Publication:
-
Solar Physics
- Pub Date:
- September 1995
- DOI:
- 10.1007/BF00732808
- Bibcode:
- 1995SoPh..160..277W
- Keywords:
-
- Magnetic Field;
- Spatial Distribution;
- Detection Limit;
- Direct Measurement;
- Magnetic Flux