The Robotic Earthshine Telescope
(2010) Ground-based and Airborne Telescopes III 7733. p.8-77332- Abstract
- Lund Observatory is presently designing and constructing a robotic telescope dedicated to studies of the Earth's albedo by measuring the ratio between the intensity of the dark and bright sides of the Moon. The telescope will operate both in broadband and narrow-band modes over the entire visible wavelength range and will transmit observational results back to the operation team over the Internet. Design challenges, in particular related to choice of CCD and stray light suppression, are described, together with the design of the optics, control system, and enclosure. Finally we present results from laboratory tests. The telescope will go into operation in the first half of 2011.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/1858338
- author
- Darudi, Ahmad LU ; Owner-Petersen, Mette LU ; Thejll, Peter ; Gleisner, Hans ; Taylor, David LU ; Ale-Ebrahem, Majid and Andersen, Torben LU
- organization
- publishing date
- 2010
- type
- Chapter in Book/Report/Conference proceeding
- publication status
- published
- subject
- host publication
- Proceedings of the SPIE
- editor
- Stepp, Larry M ; Gilmozzi, Roberto and Hall, Helen J.
- volume
- 7733
- pages
- 8 - 77332
- publisher
- SPIE
- conference name
- Ground-based and Airborne Telescopes III
- conference location
- San Diego, United States
- conference dates
- 2010-06-27 - 2010-07-02
- external identifiers
-
- wos:000285506700088
- scopus:77958143791
- ISSN
- 0277-786X
- 1996-756X
- DOI
- 10.1117/12.857126
- language
- English
- LU publication?
- yes
- id
- 7f49ed77-a75b-4780-b39c-932acb8ebfe7 (old id 1858338)
- date added to LUP
- 2016-04-01 10:50:45
- date last changed
- 2025-01-15 00:33:15
@inproceedings{7f49ed77-a75b-4780-b39c-932acb8ebfe7, abstract = {{Lund Observatory is presently designing and constructing a robotic telescope dedicated to studies of the Earth's albedo by measuring the ratio between the intensity of the dark and bright sides of the Moon. The telescope will operate both in broadband and narrow-band modes over the entire visible wavelength range and will transmit observational results back to the operation team over the Internet. Design challenges, in particular related to choice of CCD and stray light suppression, are described, together with the design of the optics, control system, and enclosure. Finally we present results from laboratory tests. The telescope will go into operation in the first half of 2011.}}, author = {{Darudi, Ahmad and Owner-Petersen, Mette and Thejll, Peter and Gleisner, Hans and Taylor, David and Ale-Ebrahem, Majid and Andersen, Torben}}, booktitle = {{Proceedings of the SPIE}}, editor = {{Stepp, Larry M and Gilmozzi, Roberto and Hall, Helen J.}}, issn = {{0277-786X}}, language = {{eng}}, pages = {{8--77332}}, publisher = {{SPIE}}, title = {{The Robotic Earthshine Telescope}}, url = {{http://dx.doi.org/10.1117/12.857126}}, doi = {{10.1117/12.857126}}, volume = {{7733}}, year = {{2010}}, }