Propagating Magneto-Acoustic Waves in the Network

Details Propagating Magneto-Acoustic Waves in the Network Propagating Magneto-Acoustic Waves in the Network

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aspc..184..232b&link_type=abstract

Third Advances in Solar Physics Euroconference: Magnetic Fields and Oscillations, ASP Conference Series vol.184, p. 232-237. Eds

Physics

Waves, Chromosphere, Magnetic Field, Formation Height

Scientific paper

The analysis of spectroscopic data taken in the chromospheric network is interpreted as evidence for propagating waves. These waves are seen from the photospheric level propagating upward to the highest levels of the chromosphere at velocities around 40 km/s, suggesting a magneto-acoustic nature. We note the lack of an adequate one-dimensional model of the solar chromosphere to interpret these data.

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