1995
DOI: 10.1117/12.208202
|View full text |Cite
|
Sign up to set email alerts
|

<title>PAMELA: phase I testing and verification on a 0.5-m diameter telescope with a 36-segment adaptive primary mirror</title>

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2006
2006
2006
2006

Publication Types

Select...
1

Relationship

0
1

Authors

Journals

citations
Cited by 1 publication
(1 citation statement)
references
References 0 publications
0
1
0
Order By: Relevance
“…A different method, demonstrated in the Phased Array Mirror Extendible Large Aperture (PAMELA), sought to decentralize the global control strategy (Rather et al 1989;Ames et al 1995;Rakoczy et al 2000). In the PAMELA test bed (a 36 hexagonal segment, 0.5 m diameter primary mirror), a ShackHartmann wave-front sensor was employed to sense tip and tilt motions of each segment.…”
Section: Introductionmentioning
confidence: 99%
“…A different method, demonstrated in the Phased Array Mirror Extendible Large Aperture (PAMELA), sought to decentralize the global control strategy (Rather et al 1989;Ames et al 1995;Rakoczy et al 2000). In the PAMELA test bed (a 36 hexagonal segment, 0.5 m diameter primary mirror), a ShackHartmann wave-front sensor was employed to sense tip and tilt motions of each segment.…”
Section: Introductionmentioning
confidence: 99%