TY - JOUR
T1 - A compact led lidar system fitted for a mars rover - Design and ground experiment
AU - Ong, Prane Mariel B.
AU - Shiina, Tatsuo
AU - Manago, Naohiro
AU - Kuze, Hiroaki
AU - Senshu, Hiroki
AU - Otobe, Naohito
AU - Hashimoto, George
AU - Kawabata, Yasuhiro
N1 - Funding Information:
This project was supported by the JSPS KAKENHI grant (JP16H03129).
Publisher Copyright:
© The Authors, published by EDP Sciences, 2018.
PY - 2018/4/13
Y1 - 2018/4/13
N2 - A compact LED lidar was constructed and fieldtested with the aim to observe the Mars' dust devils. To be able to fit it on the Mars rover, a specialized Cassegrain telescope was designed to be within a 10 cm-cube, with a field of view of 3mrad. The transmitter has 385 nm LED light source with 3 cm opening, 70mrad divergence, 0.75W (7.5nJ/10ns) pulse power, and 500 kHz repetition frequency. The configuration of the optical system is biaxial to easily configure the overlap between their optical axes.
AB - A compact LED lidar was constructed and fieldtested with the aim to observe the Mars' dust devils. To be able to fit it on the Mars rover, a specialized Cassegrain telescope was designed to be within a 10 cm-cube, with a field of view of 3mrad. The transmitter has 385 nm LED light source with 3 cm opening, 70mrad divergence, 0.75W (7.5nJ/10ns) pulse power, and 500 kHz repetition frequency. The configuration of the optical system is biaxial to easily configure the overlap between their optical axes.
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U2 - 10.1051/epjconf/201817602013
DO - 10.1051/epjconf/201817602013
M3 - Conference article
AN - SCOPUS:85045875550
SN - 2101-6275
VL - 176
JO - EPJ Web of Conferences
JF - EPJ Web of Conferences
M1 - 02013
T2 - 28th International Laser Radar Conference, ILRC 2017
Y2 - 25 June 2017 through 30 June 2017
ER -