Computer Science
Scientific paper
Jan 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.547..155s&link_type=abstract
Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO a
Computer Science
Sun: Magnetic Field, Sun: Corona, Sun: Chromosphere
Scientific paper
Magnetic field lines thread the convective layers of the Sun's interior and its atmosphere. They couple these parts of the Sun in the sense that energy is transported from the Sun's interior and surface into its atmosphere, where it is deposited, leading to a heating of the gas present there. One way of energy release is through magnetic reconnection, which leads to a change of the magnetic topology. Both these topics are briefly discussed and some recent results are reviewed, including, new measurements of the magnetic vector near the base of the corona which reveal the magnetic structure of loops and have led to the first detection of a magnetic current sheet in the solar atmosphere.
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