As for anti-air, the atmosphere changes the higher you go so it's a lot more difficult to focus it in on the target (whereas at sea level it's constant and predictable).
That's a pretty bold statement...
As for anti-air, the atmosphere changes the higher you go so it's a lot more difficult to focus it in on the target (whereas at sea level it's constant and predictable).
If you are a naval aviator, this thing should scare the shit out of you.
The radar range equation doesn't apply to lasers and the distances they can get out of this thing are phenomenal. Specifics I don't have, but from what we've covered it's got amazing potential. I know some lasers will actually use the atmosphere to help tune or focus the beam on the target. Atmospherics such as clouds and fog will affect it, however I see this being more as a small boat defense weapon (anyone notice where it was tested? hint, hint?). As for anti-air, the atmosphere changes the higher you go so it's a lot more difficult to focus it in on the target (whereas at sea level it's constant and predictable).
Hmm. Learning has occurred. So the range, if I'm doing my math right, is not linear with distance, but limited by the ratio of lens radius to wavelength. Still less than linear for a given power increase, depending on engineering constraints, but better than an inverse square law.According to some googling I did, the laser spread equation is: RT = 0.61 * D * L / RL
Where RT = beam radius at target (meters)
D = distance from laser emitter to target (meters)
L = wavelength to beam
RL = radius of laser lens or reflector
So with a wavelength of 1000 nm through a 2 meter telescope has a spot size of 12.2 cm at 100km. If the power output is 1 megawatt it could burn through about 1mm of graphite a second. It would burn through metal at a much higher rate.
Of course the published power of the laser on the Ponce is 30 kilowatts
So it is an inverse square relationship... The power output of the beam is distributed in the spot. The spot is presumably a circle, with the area = <SEE ASTB STUDY SECTION>. So.... the intensity of that spot (like radar intensity) is its power/Area... and area goes like RT^2, and RT goes like distance, so intensity goes like 1/D^2.According to some googling I did, the laser spread equation is: RT = 0.61 * D * L / RL
Where RT = beam radius at target (meters)
D = distance from laser emitter to target (meters)
L = wavelength to beam
RL = radius of laser lens or reflector
So with a wavelength of 1000 nm through a 2 meter telescope has a spot size of 12.2 cm at 100km. If the power output is 1 megawatt it could burn through about 1mm of graphite a second. It would burn through metal at a much higher rate.
Of course the published power of the laser on the Ponce is 30 kilowatts
Goddammit. Now you're making me do algebra. It's Saturday night post-bourbon. Math can wait until tomorrow post-coffee.Words words words words words
Gatling lasers? Sweet.Change lens like you change a barrel? or rotate it like most modern GAUs.