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A seismic attribute is a measurable property of seismic data, such as amplitude, dip, frequency, phase, and polarity that facilitates seismic data comprehension and interpretation.
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Thus, utilising well-defined functionalised nanorods, wrinkle-templates with tuneable amplitudes and dip-coating yield a plethora of interesting particle chain morphologies, namely triple, double, and single lines.
The solid curve denotes amplitude for a dip slip event of strike 0 (degree), dip 20 (degrees), rake 90 (degrees), and a depth of 20 km measured at 300 km of epicentral distance and an azimuth from 0 to 180 (degrees).
Three parameters such as dip, amplitude, and wavelength were chosen to analyze how the dipping and sinusoidal structure could affect the frontal speed of CO2 plume.
Secondly, the objective magnetic fluctuation has the three observational characteristics, i.e., the geomagnetic conjugacy, no altitude dependence, which implies that they do not have atmospheric density dependence, and the smaller amplitude on the dip equator.
As shown in the left panels a and b, the residual Sq amplitude near the dip equator showed no significant correlation with the magnetic field intensity but the Sq amplitude tended to decrease with an increase of the magnetic field inclination.
The long-term variation in the residual Sq amplitude near the dip equator can be interpreted as the movement of the equatorial electrojet due to secular variation of the magnetic field inclination [e.g., Cnossen and Richmond [2013]; De Haro Barbas et al. [2013].
The amplitude of that "dip" must cross the threshold (dashed portion of curve) to trigger the polarisation, as otherwise it decays back to the uniform activation level.
As the flare occurred when the equatorial electrojet current had developed significantly, SFE (ΔH) showed increasing positive amplitudes towards the dip equator while SFE (Y) increased uniformly with increasing latitudes of the station.
The amplitude minimum on the dip equator is also seen in Figure 6.Figure 7 shows that as the dip angle becomes smaller, the averaged period of the spectral peak becomes longer.
From these results, it can be mentioned that the residual Sq amplitude observed near the dip equator depends strongly on the magnetic field inclination.
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