Chromospheric polarity reversals on sunspots. Are they consistent with weak line emission?

Sánchez-Almeida, J.
Bibliographical reference

Astronomy and Astrophysics, v.324, p.763-769

Advertised on:
8
1997
Number of authors
1
IAC number of authors
1
Citations
23
Refereed citations
18
Description
Photospheric and chromospheric solar magnetograms sometimes show opposite polarity. This intriguing phenomenon is associated with the emergence of magnetic flux and with nearby, but not necessarily superposed, flaring activity. Despite the fact that there may be different explanations, it is shown here that the observed reversals are consistent with weak flare-like line emission all over the reversed polarity regions. Although this emission does not show up as a flare in filtergrams, it exhibits itself as a polarity reversal of the chromospheric magnetograms. If this interpretation were correct, the reversal would not correspond to a real flip of the magnetic field direction from the photosphere to the chromosphere. It would be an artifact due to radiative transfer effects. Observations to support or discard this hypothesis are briefly pointed out.