10-m Optical Receiver Performance
9301-004
Performance for a
10-meter aperture receiving telescope, and an ETI transmitter around a solar-type star at
10 light years.
|
|
Mean
Power
|
Peak Power
|
Pulse
Duration |
M-ary PPM
|
Bits Per
Pulse |
Data Rate
bps |
Peak EIRP W
|
Mag
|
Peak Signal
dBW |
Photons Per
Pulse |
Post-Detection
SNR, dB |
1 Hz |
1 kHz |
1 MHz |
1 GHz |
a |
1 kW |
1 kW |
NA |
NA |
NA |
NA |
2.3 X 1018 |
+23 |
-157 |
NA |
-22 |
-8 |
-38 |
-68 |
b |
1 MW |
1 MW |
NA |
NA |
NA |
NA |
2.3 X 1021 |
+15 |
-126 |
NA |
53 |
23 |
-8 |
-38 |
c |
1 GW |
1 GW |
NA |
NA |
NA |
NA |
2.3 X 1024 |
+8 |
-96 |
NA |
83 |
53 |
23 |
-7 |
d |
1 MW |
103 TW |
1 ns |
NA |
1 |
1 |
2.3 X 1030 |
NA |
-36 |
7.4 X 105 |
IB |
IB |
IB |
56 |
e |
1 GW |
106 TW |
1 ns |
NA |
1 |
1 |
2.3 X 1033 |
NA |
-6 |
7.4 X 108 |
IB |
IB |
IB |
86 |
f |
1 GW |
2 GW |
1 ns |
2 |
1 |
500 M |
4.6 X 1024 |
NA |
-93 |
1.5 X 100 |
IB |
IB |
IB |
-1 |
g |
1 GW |
8 GW |
1 ns |
8 |
3 |
380 M |
1.8 X 1025 |
NA |
-87 |
5.9 X 100 |
IB |
IB |
IB |
5 |
h |
1 GW |
128 GW |
1 ns |
128 |
7 |
55 M |
2.9 X 1026 |
NA |
-75 |
9.5 X 101 |
IB |
IB |
IB |
17 |
i |
1 GW |
1 TW |
1 ns |
1024 |
10 |
10 M |
2.3 X 1027 |
NA |
-66 |
7.6 X 102 |
IB |
IB |
IB |
26 |
j |
1 GW |
8 TW |
1 ns |
8192 |
13 |
1.6 M |
1.9 X 1028 |
NA |
-57 |
6.1 X 103 |
IB |
IB |
IB |
35 |
k |
1 MW |
52 GW |
1 ns |
524288 |
19 |
36 k |
1.2 X 1027 |
NA |
-69 |
3.9 X 102 |
IB |
IB |
IB |
23 |
l |
1 GW |
520 TW |
1 ns |
524288 |
19 |
36 k |
1.2 X 1030 |
NA |
-39 |
3.9 X 105 |
IB |
IB |
IB |
53 |
Wavelength = 656 nm
ETI Transmitting (Uplink) Telescope Diameter = 10.0 m
Earth Receiving Station (Downlink) Telescope Diameter = 10.0 m
Atmospheric Transmission = 0.40
Telescope Efficiency = 0.70
Monochromator Efficiency = 0.50
Quantum Efficiency = 0.50
NEP For Incoherent Receiver 10-4 pW/Hz
Dark Current < 3.2 X 10-6 pA (< 20 cps or 2 X 10-8
counts/ns).
Fraunhofer Suppression = 0 dB
CW Optical Bandwidth = 100 GHz (0.14 nm), Pulse Optical Bandwidth
>> 100 GHz.
Unpolarized Detected Stellar Background -112 dBW = 6.3 X 10-12
W = 2.1 X 107 photons/s = 2.1 X 10-2 photons/ns (1.0 X 10-2
counts/ns).
Solar EIRP = 3.9 X 1026 W.
Shaded areas denote undetectable signals, i.e., negative SNRs or
insufficient bandwidth (IB).
Results assume that star and transmitter are not separately resolved.
For the digital modulation systems, the pulse SNR for Poisson counting
is the photon detection rate per pulse.
For pulsed SNRs > 20 dB, the Bit Error Rate (BER) < 10-8.
|