DocumentCode
1042839
Title
Preliminary results of 400-MC radar investigations of auroral echoes at college, Alaska
Author
Leadabrand, R.L. ; Dolphin, L. ; Peterson, A.M.
Author_Institution
Stanford University, Stanford, CA, USA
Volume
7
Issue
2
fYear
1959
fDate
4/1/1959 12:00:00 AM
Firstpage
127
Lastpage
136
Abstract
Results of radar investigations of auroral ionization at a frequency of 398 mc are described. The radar detected auroral echoes at College, Alaska (near Fairbanks), even when the line of sight from the transmitter does not intersect the earth\´s magnetic field lines at perfect perpendicular incidence. The auroral echoes were observed with off-perpendicular intersection angles as great as
. The requirement for near-perpendicular intersection of the radar beam with the earth\´s magnetic field is therefore met. The auroral echoes at 398 mc were seen frequently. Occasionally they were very strong; those of highest amplitude were as much as 27 db above the receiver noise level. The echoes were detected over a relatively large echoing region corresponding to bearings within
of geomagnetic north, and elevation angles of
. Two types of auroral echoes were observed-discrete and diffuse. The discrete echoes corresponded roughly to reflections from visual auroral forms seen at night. The diffuse echoes corresponded to reflections from a large echoing region that apparently existed most often during daylight hours. Estimates of the wavelength,
, dependence of auroral echo power, although quite crude, are deduced as
for the radar site at College, Alaska, and
for sites where perpendicular reflection can be obtained.
. The requirement for near-perpendicular intersection of the radar beam with the earth\´s magnetic field is therefore met. The auroral echoes at 398 mc were seen frequently. Occasionally they were very strong; those of highest amplitude were as much as 27 db above the receiver noise level. The echoes were detected over a relatively large echoing region corresponding to bearings within
of geomagnetic north, and elevation angles of
. Two types of auroral echoes were observed-discrete and diffuse. The discrete echoes corresponded roughly to reflections from visual auroral forms seen at night. The diffuse echoes corresponded to reflections from a large echoing region that apparently existed most often during daylight hours. Estimates of the wavelength,
, dependence of auroral echo power, although quite crude, are deduced as
for the radar site at College, Alaska, and
for sites where perpendicular reflection can be obtained.Keywords
Aurora; Electromagnetic scattering by plasma media; UHF radio propagation; Earth; Educational institutions; Frequency; Geomagnetism; Ionization; Magnetic fields; Noise level; Optical reflection; Radar detection; Transmitters;
fLanguage
English
Journal_Title
Antennas and Propagation, IRE Transactions on
Publisher
ieee
ISSN
0096-1973
Type
jour
DOI
10.1109/TAP.1959.1144664
Filename
1144664
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