MAVIS adaptive optics module optical design

Author(s):  
Davide Greggio ◽  
Demetrio Magrin ◽  
Christian Schwab ◽  
Simone Di Filippo ◽  
Valentina Viotto ◽  
...  
2019 ◽  
Vol 56 (2) ◽  
pp. 022202
Author(s):  
江慧绿 Jiang Huilü ◽  
李超宏 Li Chaohong ◽  
廖娜 Liao Na ◽  
厉以宇 Li Yiyu ◽  
陈浩 Chen Hao

2006 ◽  
Author(s):  
Ming Liang ◽  
J. H. Elias ◽  
A. T. Tokunaga ◽  
M. R. Chun ◽  
M. J. Richter ◽  
...  

2010 ◽  
Vol 2010 ◽  
pp. 1-15
Author(s):  
Richard Willingale ◽  
Charlotte Feldman ◽  
Alan Michette ◽  
Tim Button ◽  
Camelia Dunare ◽  
...  

The UK Smart X-Ray Optics (SXO) programme is developing active/adaptive optics for terrestrial applications. One of the technologies proposed is microstructured optical arrays (MOAs), which focus X-rays using grazing incidence reflection through consecutive aligned arrays of microscopic channels. Although such arrays are similar in concept to polycapillary and microchannel plate optics, they can be bent and adjusted using piezoelectric actuators providing control over the focusing and inherent aberrations. Custom configurations can be designed, using ray tracing and finite element analysis, for applications from sub-keV to several-keV X-rays, and the channels of appropriate aspect ratios can be made using deep silicon etching. An exemplar application will be in the microprobing of biological cells and tissue samples using Ti Kα radiation (4.5 keV) in studies related to radiation-induced cancers. This paper discusses the optical design, modelling, and manufacture of such optics.


2008 ◽  
Author(s):  
Weiwei Wang ◽  
Melanie C. W. Campbell ◽  
Marsha L. Kisilak ◽  
Shelley R. Boyd

2013 ◽  
Vol 8 (S300) ◽  
pp. 355-361
Author(s):  
S. S. Hasan

AbstractThe primary objective of the 2-m National Large Solar Telescope (NLST) is to study the solar atmosphere with high spatial and spectral resolution. With an innovative optical design, NLST is an on-axis Gregorian telescope with a low number of optical elements and a high throughput. In addition, it is equipped with a high order adaptive optics system to produce close to diffraction limited performance.NLST will address a large number of scientific questions with a focus on high resolution observations. With NLST, high spatial resolution observations of prominences will be possible in multiple spectral lines. Studies of magnetic fields, filament eruptions as a whole, and the dynamics of filaments on fine scales using high resolution observations will be some of the major areas of focus.


2014 ◽  
Author(s):  
Xianyu Zhang ◽  
Nicolas Gorceix ◽  
Dirk Schmidt ◽  
Philip R. Goode ◽  
Wenda Cao ◽  
...  

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