Spectropolarimetry of a sunspot at disk centre

@inproceedings{Cuberes2005SpectropolarimetryOA,
  title={Spectropolarimetry of a sunspot at disk centre},
  author={M. S{\'a}nchez Cuberes and Katharina Puschmann and E. Wiehr},
  year={2005}
}
The magnetic, thermal and velocity structure of a sunspot at the solar disk centre (θ = 2◦) is investigated by inverting the full Stokes profiles of three infrared lines. A single magnetic component atmosphere is assumed with height gradients of the physical quantities. Since the line-of-sight (LOS) is perpendicular to the solar surface, differential optical or projection effects do not interfere, as often is the case for the usual observations at oblique LOS. We find a symmetric configuration… CONTINUE READING

Citations

Publications citing this paper.

Magnetic Structure of Sunspots

Living reviews in solar physics • 2011
View 6 Excerpts
Highly Influenced

References

Publications referenced by this paper.

Spectropolarimetry of a sunspot at disk centre

M. Sánchez Cuberes
Sol. Phys., • 1992

Similar Papers

Loading similar papers…