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It is generally attributed to the Doppler effect, a change in wavelength that results when a given source of waves (e.g., light or radio waves) and an observer are in rapid motion with respect to each other.
Such a magma flow at the crater could reduce the pressure inside the conduit, probably generating a magma flow wave at/around the pressure source (e.g., activating the source of waves (Z)).
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Results suggest that CODAR HF Radar wave data are a reliable source of wave information even in the case of extreme events, providing an avenue to improve and complete the offer of services deriving from the CALYPSO system.
The intensity of weather systems as well as the location of potential sources of waves towards the points of HF Doppler shift observation influence significantly the occurrence of infrasonic waves in the ionosphere.
It was the largest source of infrasound waves — low-frequency waves of pressure — ever recorded by a system set up globally to monitor compliance with the Nuclear Test Ban Treaty.
There are two sources of wave directionality, i.e. firstly, the variable direction of uni-directional seas, and secondly, wave spreading around a given mean direction.
Many of the above suggestions as to the sources of wave components can in principle be tested theoretically through numerical experiments in a general circulation model wherein various combinations of primary waves are excited within the model.
Two main sources of wave damping have been recognized in the performed tests: (i) due to the wave interaction with the mangrove models, particularly with the root system, (ii) due to wave breaking generated for favorable water depth/incident wave conditions.
The relationship between significant wave height and period, the variability of significant wave period, the spectral peak enhancement factor, and the directional spreading parameter of large deepwater waves around the Korean Peninsula have been investigated using various sources of wave measurement and hindcasting data.
The peak at a period near 150 min, corresponding to horizontal scales approximately 100 km, is due to orographic waves located over the Antarctic Peninsula, a strong source of such waves (Hertzog et al. 2008).
In another version, the spacing of the antennas can be changed in an attempt to make the waves interfere; the distance between them for interference depends on the wavelength and on the diameter of the source of the waves.
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