International Conference on Space Optics — ICSO 2016 2017
DOI: 10.1117/12.2296200
|View full text |Cite
|
Sign up to set email alerts
|

Use of adaptive optics in ground stations for high data rate satellite-to-ground links

Abstract: Abstract-Over the past years we have successfully applied adaptive optics (AO) in some optical ground stations (OGS) to improve the signal-to-noise ratio of satellite to ground laser communications. In the paper we present the realized setups including optics and components, the reconstruction scheme especially latest performance measurements of the AO system implemented at the 26cm TAOGS optical terminal which is presently at the Observatorio del Teide, Tenerife. Furthermore, we present the concept for the up… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1

Citation Types

0
3
0

Year Published

2018
2018
2022
2022

Publication Types

Select...
2
2

Relationship

0
4

Authors

Journals

citations
Cited by 4 publications
(3 citation statements)
references
References 3 publications
0
3
0
Order By: Relevance
“…The downlink experiences lower losses and the OGS can be equipped with a large diameter receiver (or use the Coudé focus of the main telescope) as well as cooled highsensitivity detectors, together allowing for the use of a relatively low power laser source and small transmitter telescope on the space segment. Finally, we note the encouraging result reported in [58] that the large difference in quantum channel and beacon laser wavelength does not preclude using the beacon laser at 1550 nm to correct the turbulence-induced beam wander at the quantum channel wavelength of 808 nm (employing, e.g., a fast steering mirror on the OGS or its adaptive optics system [59]).…”
Section: /34mentioning
confidence: 71%
“…The downlink experiences lower losses and the OGS can be equipped with a large diameter receiver (or use the Coudé focus of the main telescope) as well as cooled highsensitivity detectors, together allowing for the use of a relatively low power laser source and small transmitter telescope on the space segment. Finally, we note the encouraging result reported in [58] that the large difference in quantum channel and beacon laser wavelength does not preclude using the beacon laser at 1550 nm to correct the turbulence-induced beam wander at the quantum channel wavelength of 808 nm (employing, e.g., a fast steering mirror on the OGS or its adaptive optics system [59]).…”
Section: /34mentioning
confidence: 71%
“…The downlink experiences lower losses and the OGS can be equipped with a large diameter receiver (or use the Coudé focus of the main telescope) as well as cooled high-sensitivity detectors, together allowing for the use of a relatively low power laser source and small transmitter telescope on the space segment. Finally, we note the encouraging result reported in [61] that the large difference in quantum channel and beacon laser wavelength does not preclude using the beacon laser at 1550 nm to correct the turbulence-induced beam wander at the quantum channel wavelength of 808 nm (employing, e.g., a fast steering mirror on the OGS or its adaptive optics system [62]).…”
Section: Beacon Lasersmentioning
confidence: 71%
“…Also, the high achievable data rates and other methods for increasing the sensitivity (like optical pre-amplification or coherent modulation) are desirable. Here, optical space communications follow terrestrial systems [14], but these often require a higher implementation effort, such as with adaptive optics for the single mode fiber coupling of an atmospherically distorted optical field [15]. Bulk AP-detectors do not require such sophisticated techniques and allow focal illumination with an atmospherically distorted light field.…”
Section: Introductionmentioning
confidence: 99%