Physics
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..124..219g&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 124, no. 2, 1989, p. 219-226. Research supported by CAICYT.
Physics
7
Solar Activity, Solar Magnetic Field, Chromosphere, Decay, Magnetic Field Reconnection, Magnetic Signatures, Solar Corona, Solar Observatories, Velocity Distribution
Scientific paper
A case of cancellation of magnetic fields is observed during the decay of a small active region. Three different sources of information were simultaneously used: high resolution magnetograms, chromospheric Ca II filtergrams and transverse velocity fields. A magnetic structure is apparently dragged to the network by the supergranular velocity field while it splits into two. There, they meet another structure with opposite magnetic polarity. After a period of coexistence, the magnetic pairs vanish, leaving no trace of either magnetic or chromospheric structures.
Aballe M. A.
Collados Manuel
Garcia de La Rosa J. I.
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