High Resolution Analysis of the Upper Convection Zone

Details High Resolution Analysis of the Upper Convection Zone High Resolution Analysis of the Upper Convection Zone

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp31a02b&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP31A-02

Physics

7522 Helioseismology

Scientific paper

Plane-wave (ring-diagram) analysis of high-degree modes in data from the SOI/MDI instrument on SOHO have enabled us us to determine the structure and dynamics of about 0.1 solar radius below the photosphere, and study how these quantities change with time. The bulk of the work done so far has utilized full-disc data for which the analysis has the ability to resolve structures with a scale of about 180 Mm. Additional data with three times the spatial resolution over a small portion of the disc are available for shorter durations at various times. Here we report on details of various trends which not resolved by full-disc data.

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