Bibcode
Sánchez-Almeida, J.
Referencia bibliográfica
Astronomy and Astrophysics, v.324, p.763-769
Fecha de publicación:
8
1997
Revista
Número de citas
22
Número de citas referidas
17
Descripción
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.