GONG 1992: Seismic investigation of the sun and stars; Proceedings of the Conference, Boulder, CO, Aug. 11-14, 1992

Details GONG 1992: Seismic investigation of the sun and stars; Proceedings of the Conference, Boulder, CO, Aug. 11-14, 1992 GONG 1992: Seismic investigation of the sun and stars; Proceedings of the Conference, Boulder, CO, Aug. 11-14, 1992

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...42.....b&link_type=abstract

Conference Proceedings,

Computer Science

Sound

14

Conferences, Helioseismology, Stellar Physics, Acoustic Excitation, Thermal Boundary Layer, Boundary Layer Stability, Gravity Waves, Solar Interior, Solar Rotation, Wave Interaction, Sound Waves, Convective Flow, Charge Coupled Devices, Solar Oscillations, Data Processing, Data Reduction, Fiber Optics, Massively Parallel Processors, Echelle Gratings, Avalanche Diodes, Photodiodes

Scientific paper

Various papers on the seismic investigation of the sun and stars are presented. Individual topics addressed include: excitation of solar p-modes, cause of cycle-related global solar changes, ionization effects on solar granulation dynamics, turbulent compressible convection with rotation, convective overshooting in stars, local helioseismology of subsurface structure, observations of high-frequency solar oscillations, high-frequency P-mode spectrum, high-frequency solar velocity noise, isothermal waves in solar atmosphere, detection of convective overshoot, 2D helioseismic inversions, seismic limits on the sun's internal toroidal field, faster formulations of the OLA method, torsional oscillations and internal rotation. Also discussed are: solar g-mode signatures in p-mode signals, theory of Delta Scuti stars, the Whole Earth Telescope, phase function for solar-like stars, asteroseismic HR diagram, seismic analysis of stellar P-mode spectra, asteroseismic calibration of stellar clusters, observations of Delta Scuti stars from Arhus, seismology of Procyon, seismological modeling of PG1159-035, GONG Project update, ring diagram analysis of Mt. Wilson data, gap filling the GONG data set, helioseismic prospects in the MIR, multicolor CCD photometer, new echelle spectrograph for asteroseismology.

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