[Laser] heliograph vs. laser indeed!
F1AVYopto at aol.com
F1AVYopto at aol.com
Fri Jun 15 17:22:22 EDT 2007
I did rough calculations with your initial conditions.
These calculations are simplified to get only orders of range.
A 1 m² mirror gives to 200 Km a (400pi / 360) x 0,5 = 1,7 Km in diameter
spot with a 0,5° beam divergence.
In vacuum, the spot power density will be 1000 / 850².pi = 0,00044 W/m² for
1 KW reflected power.
With a 5 mW laser the same laser density will be in a 0,005 / 0,00044 = 11
m² spot (3,8 m in diameter !)
The laser beam angle must be 2pi / (400pi / 0,0038) = 2.10-5 radians = 20
micro radians !
A 20 micro radians beam is only possible with a very big telescope as
collimator.
On the moon the spot will be smaller than 7 Km !
A so small spot needs a more than 1 m aperture telescope !
For the heliograph or the laser, in a very clear atmosphere, the loss should
be 0,2 dB / Km.
The laser wavelength must very well chosen for this minimal loss...
At 200 Km the loss will be 40 dB.
The real power density becomes 44.10^-9 W/m².
For conclusion, for the same optical brightness, the heliograph is very
better than the laser for simplicity …
In the same principle I did another calculation.
I imagine a simple 1 m² LEDs matrix (for example LUXEONs) on the moon with
10 W total optical power.
Each of the modulated LEDs is fitted with a lens that gives an angular
dispersion to just cover the earth diameter (about 2°).
The power density on the earth will be near 8.10^-8 W/Km².
In a square meter 8.10^-8 / 10^6 = 8.10^-14 W.
The atmospheric losses are rather small for a nearly vertical aiming.
In a 30 cm telescope with a femto watt capability photo receiver, a FFTDSP
extracting, this signal can be detected.
Of course because the light background, the detection will be only possible
during the moon phases that give darkness to the beacon location.
73 Yves F1AVY
More information about the Laser
mailing list