The TRACE Inter-Network Oscillations (INO) Program I: Probing Chromospheric Topography

Details The TRACE Inter-Network Oscillations (INO) Program I: Probing Chromospheric Topography The TRACE Inter-Network Oscillations (INO) Program I: Probing Chromospheric Topography

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh13c..05m&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH13C-05

Astronomy and Astrophysics

Astrophysics

2752 Mhd Waves And Instabilities, 7500 Solar Physics, Astrophysics, And Astronomy, 7507 Chromosphere, 7522 Helioseismology, 7524 Magnetic Fields

Scientific paper

We will present results of the TRACE Inter-Network Oscillations (INO) observing program from 2003 to the present. The INO program uses near-simultaneous observations in the 1600Å and 1700Å UV continuum pass bands as an acoustic probe of chromospheric structure. In the two years of INO observations we have studied a large number of quiet chromosphere and active regions as well as regions of the chromosphere under coronal holes. In this poster we will discuss the diagnostic methods applied to analyze the INO observations and the key results found, thus far. These diagnostic methods offer us a remote means to study the complex plasma topography of the solar chromosphere.

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