Not exact matches
LIGO
detects gravitational waves
by splitting a powerful infrared
laser beam in two, then sending the
beams at right angles through tunnels to mirrors 2.5 miles away.
The global maps were created from data obtained
by an instrument called the Mars Orbiter
Laser Altimeter (MOLA), which bounces an infrared laser beam off the surface and calculates the distance from the spacecraft by measuring the time it takes to detect the reflected p
Laser Altimeter (MOLA), which bounces an infrared
laser beam off the surface and calculates the distance from the spacecraft by measuring the time it takes to detect the reflected p
laser beam off the surface and calculates the distance from the spacecraft
by measuring the time it takes to
detect the reflected pulse.
By carefully measuring the deflected light scientists can
detect tiny differences in intensity across the spectrum which inform them about the chirality of the grating the
laser beam interacts with.
The signal the researchers are trying to
detect is very small so it must be amplified
by spatially overlapping a reference
laser beam that doesn't contain the signal of interest, which is a process called heterodyne amplification.
They had achieved an even larger
laser amplification,
by a factor of 10,000, when using weak measurements to
detect a shift in a
beam of polarized light moving between air and glass.
As the particles pass through a
laser beam, the absorbed energy heats the particles and in turn the surrounding air, which sets off a pressure wave that can be
detected by a microphone.