Spectral signature of uncombed penumbral magnetic fields. Reply

Martínez Pillet, V.
Bibliographical reference

Astronomy and Astrophysics, v.369, p.644-645 (2001)

Advertised on:
4
2001
Number of authors
1
IAC number of authors
1
Citations
16
Refereed citations
15
Description
A combination of two penumbral models similar to those used by Martínez Pillet (2000) is presented. One matches the observed rms fluctuations perfectly while the other reproduces the observed Net Circular Polarization. No factor three mismatch exists in this case. The rationale of using two different, but strongly coupled, models is explained.