Why Solar Magnetic Flux Concentrations Are Bright in Molecular Bands
Open Access
- 17 October 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 597 (2), L173-L176
- https://doi.org/10.1086/379869
Abstract
No abstract availableThis publication has 21 references indexed in Scilit:
- Reconstruction of solar irradiance variations in cycle 23: Is solar surface magnetism the cause?Astronomy & Astrophysics, 2003
- Quiet-Sun Magnetic Fields at High Spatial ResolutionThe Astrophysical Journal, 2002
- High‐Resolution Observations of Small‐Scale Emerging Flux in the PhotosphereThe Astrophysical Journal, 2002
- On the Relation of G‐Band Bright Points to the Photospheric Magnetic FieldThe Astrophysical Journal, 2001
- The Formation of G-band Bright Points I: Standard LTE ModellingSymposium - International Astronomical Union, 2001
- Measurements of Solar Magnetic Element Motion from High‐Resolution FiltergramsThe Astrophysical Journal, 1998
- On the Dynamics of Small-Scale Solar Magnetic ElementsThe Astrophysical Journal, 1996
- New Observations of Subarcsecond Photospheric Bright PointsThe Astrophysical Journal, 1995
- Resolution of magnetic flux tubes on the SunNature, 1992
- Some developments in the theory of magnetic flux concentrations in the solar atmosphereAdvances in Space Research, 1991