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The amount of solar radiation reaching the surface depends on latitude, time of year, time of day, and orientation of the land surface with respect to the Sun.
The GPS information sent back includes longitude, latitude, time stamp, signal quality, etc.
A range of situations is presented, including variations in orbital position, latitude, time of day, dust loading and ozone presence.
A key driving variable is surface radiation (Rs) which is influenced by both meso-scale factors (latitude, time of year, cloudiness) and the topographic variables of slope, aspect and horizon shading.
Figure 8 presents radar magnetic latitude time plots of backscatter echo power and LOS velocity parameters between 09 00 and 10 00 UT by beams 6 and 11, respectively.
The best fit for both the longitude and latitude time series, and, respectively, were combined with the time variable (t) to show the trend of the horizontal displacement of each GPS buoy (red line in Fig. 3, top).
Similar(40)
The overall shape in latitude-time space was similar during the expansive/early recovery phase lasting from 5 33 UT to nearly 6 30 UT.
Figure 26 shows a comparison between four commonly used models on a latitude-time grid for a quiet day, revealing some notable differences.
To investigate the seasonal behaviour of the TDT in more detail, two latitude-time cross sections around 90 km and 110 km are shown in Figure 5.
Figure 5 Latitude-time plot of the normalised amplitude of the 8-h oscillation at approximately 90/110 km (left/right panel).
Fig. 2. The magnetic index Dst and Latitude-Time-TEC plots of IRI, MAGIC, ground-based GPS observation during the average of 15 21 and 22 26 July 2009.
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