[Code of Federal Regulations]
[Title 47, Volume 4]
[Revised as of October 1, 2003]
From the U.S. Government Printing Office via GPO Access
[CITE: 47CFR73.185]
[Page 55-57]
TITLE 47--TELECOMMUNICATION
COMMISSION (CONTINUED)
PART 73_RADIO BROADCAST SERVICES--Table of Contents
Subpart A_AM Broadcast Stations
Sec. 73.185 Computation of interfering signal.
(a) Measured values of radiation are not to be used in calculating
overlap, interference, and coverage.
(1) In the case of an antenna which is intended to be non-
directional in the horizontal plane, an ideal non-directional radiation
pattern shall be used in determining interference, overlap, and
coverage, even if the antenna is not actually non-directional.
(2) In the case of an antenna which is directional in the horizontal
plane, the radiation which shall be used in determining interference,
overlap, and coverage is that calculated pursuant to Sec. 73.150 or
Sec. 73.152, depending on whether the station has a standard or
modified standard pattern.
(3) In the case of calculation of interference or overlap to (not
from) a foreign station, the notified radiation shall be used, even if
the notified radiation differs from that in paragraphs (a) (1) or (2) of
this section.
(b) For skywave signals from stations operating on all channels,
interference shall be determined from the appropriate formulas and
Figure 6a contained in Sec. 73.190.
(c) The formulas in Sec. 73.190(d) depicted in Figure 6a of Sec.
73.190, entitled ``Angles of Departure versus Transmission Range'' are
to be used in determining the angles in the vertical pattern of the
antenna of an interfering
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station to be considered as pertinent to transmission by one reflection.
To provide for variation in the pertinent vertical angle due to
variations of ionosphere height and ionosphere scattering, the curves 2
and 3 indicate the upper and lower angles within which the radiated
field is to be considered. The maximum value of field strength occurring
between these angles shall be used to determine the multiplying factor
to apply to the 10 percent skywave field intensity value determined from
Formula 2 in Sec. 73.190. The multiplying factor is found by dividing
the maximum radiation between the pertinent angles by 100 mV/m.
(d) Example of the use of skywave curves and formulas: Assume a
proposed new Class B station from which interference may be expected is
located at a distance of 724 kilometers from a licensed Class B station.
The proposed station specifies geographic coordinates of
40[deg]00[min]00[min]N and 100[deg]00[min]00[sec]W and the station to be
protected is located at an azimuth of 45[deg] true at geographic
coordinates of 44[deg]26[min]05[sec]N and 93[deg]32[min]54[sec]W. The
critical angles of radiation as determined from Figure 6a of Sec.
73.190 for use with Class B stations are 9.6[deg] and 16.6[deg]. If the
vertical pattern of the antenna of the proposed station in the direction
of the existing station is such that, between the angles of 9.6[deg] and
16.6[deg] above the horizon the maximum radiation is 260 mV/m at one
kilometer, the value of the 50% field, as derived from Formula 1 of
Sec. 73.190, is 0.06217 mV/m at the location of the existing station.
To obtain the value of the 10% field, the 50% valuemust be adjusted by a
factor derived from Formula 2 of Sec. 73.190. The value in this case is
8.42 dB. Thus, the 10% field is 0.1616 mV/m. Using this in conjunction
with the co-channel protection ratio of 26 dB, the resultant nighttime
limit from the proposed station to the licensed station is 3.232 mV/m.
(e) In the case of an antenna which is non-directional in the
horizontal plane, the vertical distribution of the relative fields
should be computed pursuant to Sec. 73.160. In the case of an antenna
which is directional in the horizontal plane, the vertical pattern in
the great circle direction toward the point of reception in question
must first be calculated. In cases where the radiation in the vertical
plane, at the pertinent azimuth, contains a large lobe at a higher angle
than the pertinent angle for one reflection, the method of calculating
interference will not be restricted to that just described; each such
case will be considered on the basis of the best knowledge available.
(f) In performing calculations to determine permissible radiation
from stations operating presunrise or postsunset in accordance with
Sec. 73.99, calculated diurnal factors will be multiplied by the values
of skywave field strength for such stations obtained from Formula 1 or 2
of Sec. 73.190.
(1) The diurnal factor is determined using the time of day at the
mid-point of path between the site of the interfering station and the
point at which interference is being calculated. Diurnal factors are
computed using the formula
Df=a+bF+cF2+dF3 where:
Df represents the diurnal factor,
F is the frequency in MHz,
a,b,c, and d are constants obtained from the tables in paragraph (k)(2)
A diurnal factor greater than one will not be used in calculations and
interpolation is to be used between calculated values where necessary.
For reference purposes, curves for presunrise and postsunset diurnal
factors are contained in Figures 13 and 14 of Sec. 73.190.
(2) Constants used in calculating diurnal factors for the presunrise
and postsunset periods are contained in paragraphs (f)(2) (i) and (ii)
of this section respectively. The columns labeled Tmp
represent the number of hours before and after sunrise and sunset at the
path midpoint.
(i) Presunrise Constants
------------------------------------------------------------------------
Tmp a b c d
------------------------------------------------------------------------
-2.......................... 1.3084 .0083 -.0155 .0144
-1.75....................... 1.3165 -.4919 .6011 -.1884
-1.5........................ 1.0079 .0296 .1488 -.0452
-1.25....................... .7773 .3751 -.1911 .0736
-1.......................... .6230 .1547 .2654 -.1006
-.75........................ .3718 .1178 .3632 -.1172
-.5......................... .2151 .0737 .4167 -.1413
-.25........................ .2027 -.2560 .7269 -.2577
SR.......................... .1504 -.2325 .5374 -.1729
+.25........................ .1057 -.2092 .4148 -.1239
+5.......................... .0642 -.1295 .2583 -.0699
+.75........................ .0446 -.1002 .1754 -.0405
+1.......................... .0148 .0135 .0462 .0010
------------------------------------------------------------------------
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(ii) Postsunset Constants
------------------------------------------------------------------------
Tmp a b c d
------------------------------------------------------------------------
1.75........................ .9495 -.0187 .0720 -.0290
1.5......................... .7196 .3583 -.2280 .0611
1.25........................ .6756 .1518 .0279 -.0163
1.0......................... .5486 .1401 .0952 -.0288
.75......................... .3003 .4050 -.0961 .0256
.5.......................... .1186 .4281 -.0799 .0197
.25......................... .0382 .3706 -.0673 .0171
SS.......................... .0002 .3024 -.0540 .0086
-.25........................ .0278 .0458 .1473 -.0486
-.5......................... .0203 .0132 .1166 -.0340
-.75........................ .0152 -.0002 .0786 -.0185
-1.0........................ -.0043 .0452 -.0040 .0103
-1.25....................... .0010 .0135 .0103 .0047
-1.5........................ .0018 .0052 .0069 .0042
-1.75....................... -.0012 .0122 -.0076 .0076
-2.0........................ -.0024 .0141 -.0141 .0091Q
P='04'