Computer Science – Sound
Scientific paper
Dec 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3....3v&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, Nov.-Dec. 1987, p. 3-9. In Russian.
Computer Science
Sound
3
Infrasonic Frequencies, Mars Atmosphere, Solar Atmosphere, Solar Planetary Interactions, Annual Variations, Atmospheric Pressure, Temperature Gradients, Thermoelasticity, Troposphere
Scientific paper
It is shown that conditions for the excitation of terminator infrasound are realized in the Martian atmosphere. Direct measurements of daily temperature variations indicate the appearance of dynamic pressure-variation anomalies with a quasi-period of about 3 min and a characteristic 'wavelength' of about 40 km in the planetographic latitude range of 10-30 deg (as a function of season). During the morning hours of the Martian summer in the southern hemisphere, the excess pressure in the waves can amount to several fractions of a percent and can result in the modulation observed for certain cloud structures.
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