Three-dimensional magnetic field structure of a flux-emerging region in the solar atmosphere
- 11 December 2019
- journal article
- research article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 632, A112
- https://doi.org/10.1051/0004-6361/201936790
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsThis publication has 88 references indexed in Scilit:
- ANOMALOUS CIRCULAR POLARIZATION PROFILES IN THE He I 1083.0 nm MULTIPLET FROM SOLAR SPICULESThe Astrophysical Journal, 2012
- The height of chromospheric loops in an emerging flux regionAstronomy & Astrophysics, 2011
- Magnetic structures of an emerging flux region in the solar photosphere and chromosphereAstronomy & Astrophysics, 2010
- On magnetic field “reconstruction”Astronomy & Astrophysics, 2008
- Advanced Forward Modeling and Inversion of Stokes Profiles Resulting from the Joint Action of the Hanle and Zeeman EffectsThe Astrophysical Journal, 2008
- Supersonic downflows in the vicinity of a growing poreAstronomy & Astrophysics, 2006
- Determination of the Magnetic Field Vector via the Hanle and Zeeman Effects in the Heiλ10830 Multiplet: Evidence for Nearly Vertical Magnetic Fields in a Polar Crown ProminenceThe Astrophysical Journal, 2006
- Comparing magnetic field extrapolations with measurements of magnetic loopsAstronomy & Astrophysics, 2005
- Three-dimensional magnetic field topology in a region of solar coronal heatingNature, 2003
- Emerging flux tubes in the solar convection zone. 1: Asymmetry, tilt, and emergence latitudeThe Astrophysical Journal, 1995