This page contains a Flash digital edition of a book.

outputs, and a wide spectral range (350nm- 1,000nm).

650nm; a 500µm active area; and adjustable temperature, quantum efficiency, and deadtime. They are C-mount, SM1, and Thorlabs cage compatible, provided with universal network adapter (110/220V), have NIM and LLTTL


Late last year, a team of researchers from the Massachusetts Institute of Technology’s (MIT) Lincoln Laboratory working with NASA demonstrated a laser-based communication uplink between the moon and Earth. At CLEO 2014, the team will present new details and the first comprehensive overview of the on-orbit performance of the uplink, which beat the previous record transmission speed by a factor of 4,800. Earlier reports have stated what the team accomplished, but have not provided the details of the implementation.

‘This will be the first time

that we present both the implementation overview and how well it actually worked,’ said Mark Stevens of MIT Lincoln Laboratory. ‘The on-orbit performance was excellent and close to what we’d predicted, giving us confidence that we have a good understanding of the underlying physics.’ The team made history last year when their Lunar Laser Communication Demonstration (LLCD) transmitted data over the 384,633km between the moon and Earth at a download rate of 622 megabits per second, faster

than any radio frequency (RF) system. They also transmitted data from the Earth to the moon at 19.44 megabits per second, a factor of 4,800 times faster than the best RF uplink ever used.

‘Communicating at high data rates from Earth to the moon with laser beams is challenging because of the 400,000km distance spreading out the light beam,’ Stevens said. ‘It’s doubly difficult going through the atmosphere, because turbulence can bend light, causing rapid fading or dropouts of the signal at the receiver.’

A ground terminal at White Sands, New Mexico, uses four separate telescopes to send the uplink signal to the moon. Each telescope is about six inches in diameter and fed by a laser transmitter that sends information coded as pulses of infrared light. The total transmitter power is the sum of the four separate transmitters, which results in 40W of power. The reason for the four telescopes is that each one transmits light through a different column of air that experiences different bending effects from the

‘ This will be the first time that we present both the implementation overview and how well it actually worked’

atmosphere, Stevens said. This increases the chance that at least one of the laser beams will interact with the receiver, which is mounted on a satellite orbiting the moon. This receiver uses a slightly narrower telescope to collect the light, which is

then focused into an optical fibre. From there, the signal in the fibre is amplified about 30,000 times. A photodetector converts the pulses of light into electrical pulses that are in turn converted into data bit patterns that carry the transmitted message. Of the 40W signals sent

by the transmitter, less than a billionth of a watt is received at the satellite – but that’s still about 10 times the signal necessary to achieve error-free communication, Stevens said.

The CLEO presentation, which will take place on 9 June at 4pm, will also describe how the large margins in received signal level can allow the system to operate through partly transparent thin clouds in the Earth’s atmosphere, which the team views as a big bonus.

While the LLCD design is directly relevant for near-Earth missions, the team predicts that it’s also extendable to deep-space missions to Mars and the outer planets.

Picoquant will present the new supercontinuum laser Solea. The tunable picosecond laser source provides users with capabilities such as full wavelength tunability and free triggering. This makes it an ideal excitation source for ultrasensitive applications like single-molecule detection and Förster Resonant Energy Transfer (FRET). The laser can be operated at a number of internal repetition rates or even be externally triggered at any repetition rate between 1 and 40MHz. The user can select any single wavelength between 480 and 700nm.

A further highlight on display will be the recently developed 560nm picosecond pulsed

diode laser head. The new laser is ideal for exciting fluorescent proteins like mCherry or DsRed, and fluorescent dyes such as CY3 or Atto565. With pulse durations as short as 80ps, the pulsed laser head perfectly matches the time resolution of mainstream detectors and is ideally suited for all time-resolved fluorescence applications.


@electrooptics |

Andrew Sproule/

Page 1  |  Page 2  |  Page 3  |  Page 4  |  Page 5  |  Page 6  |  Page 7  |  Page 8  |  Page 9  |  Page 10  |  Page 11  |  Page 12  |  Page 13  |  Page 14  |  Page 15  |  Page 16  |  Page 17  |  Page 18  |  Page 19  |  Page 20  |  Page 21  |  Page 22  |  Page 23  |  Page 24  |  Page 25  |  Page 26  |  Page 27  |  Page 28  |  Page 29  |  Page 30  |  Page 31  |  Page 32  |  Page 33  |  Page 34  |  Page 35  |  Page 36  |  Page 37  |  Page 38  |  Page 39  |  Page 40  |  Page 41  |  Page 42  |  Page 43  |  Page 44  |  Page 45