During the summer of 1973 the rain reflectivity environment in three-dimensional space was routinely recorded on digital tape at Wallops Island, Va. A mode of operation consisted of sampling periodically60degazimuth intervals over regions in which the rain activities were most intense and widespread. A series of plan-position indicator (PPI) sweeps over these intervals were implemented at a sequence of elevation angles starting from0.5degup io an angle above which the reflectivity values were below a designated threshold level. Approximately 500 such raster scans were acquired in which each scan was obtained in less than 4 min and covered a range interval of 10 to 140 km. Using the above data base, reflectivity profiles along representative earth-satellite paths were determined from which attenuation and space diversity statistics were calculated at the frequencies of 13 and 18 GHz. Specifically, the formk = aZ^{b}was used to deduce the total path attenuation, wherekis the attenuation coefficient (dB/km), andZis the reflectivity factor (mm6/m3). The constantsaandbwere calculated using the raindrop distribution for thunderstorm activity as proposed by Joss. Probabilities that the attenuations exceed given fade depths, diversity gain as a function of fade depths, and diversity gain as a function of site separation distances are characterized and compared at the various frequencies. For the space diversity mode, a site spacing of 15 km is shown to give rise to a near optimum condition for the diversity gain. Furthermore, the diversity gain has been demonstrated to be minimally influenced by the transmitter frequency.
Published in:
Antennas and Propagation, IEEE Transactions on
(Volume:23
,
Issue:
2
)
Date of Publication:
Mar 1975
- Page(s):
-
221
-
227
- ISSN :
-
0018-926X
- Digital Object Identifier :
-
10.1109/TAP.1975.1141038
- Product Type:
-
Journals & Magazines
- Date of Current Version :
-
06 January 2003
- Issue Date :
-
Mar 1975
- Sponsored by :
-
IEEE Antennas and Propagation Society