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These observations are analyzed statistically in Fig. 4a, showing a summary of the analysis of the CPD variation at the GBs of all investigated samples.
The statistics of the repeated observations are analyzed to derive an empirical calibration of the reliability of the spectroscopic identifications in the CFRS in order to determine how often additional observations could lead to the identification of an initially unidentified object and to provide an estimate of the internal velocity accuracy.
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A total of 152 hours of behavioral observations were analyzed using a combination of behavior and scan sampling to obtain information on individual time budgets.
180 events from more than three years of observations were analyzed, focusing on 13 meteorological variables, including the number of raindrops, their diameter, and velocity.
AUREOL-3 satellite observations were analyzed to study their properties in the framework of the ionosphere-magnetosphere coupling model proposed by Tverskoy (1982).
So, the data of half a year of observations were analyzed to establish the behavior of Total Electron Content (TEC) in a region of Northern crest of the equatorial anomaly in quiet helio-geophysical conditions as a background for detecting the impact of effects from below.
Second, due to data availability, only 1841 observations were analyzed.
The data including interviews, journals, and observations were analyzed through reading, coding, and revising the codes.
The qualitative data gathered through in-depth interview and field observations were analyzed thematically.
Although some might work better with different settings, all the GPS observations were analyzed with the same filter setups hereafter.
These observations were analyzed, and the results were compared with those obtained from observations over the East China Sea in the Air Mass Transformation Experiment in 1974 (AMTEX '74).
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