Issue |
A&A
Volume 526, February 2011
|
|
---|---|---|
Article Number | A56 | |
Number of page(s) | 5 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/201014844 | |
Published online | 21 December 2010 |
Research Note
Detecting photons with orbital angular momentum in extended astronomical objects: application to solar observations
1
Laboratorio de Instrumentación Espacial (LINES)Instituto Nacional de
Técnica Aeroespacial (INTA),
Ctra. Ajalvir km 4, Torrejón de
Ardoz,
28850
Madrid,
Spain
e-mail: uribepnr@gmail.com; alvareza@inta.es
2
THEMIS, CNRS UPS 853, C/ vía Láctea s\n, La Laguna, 38205
Tenerife,
Spain
e-mail: arturo@themis.iac.es; bgelly@themis.iac.es; claude.lemen@gmail.com
3
Instituto de Astrofisica de Canarias, C/ vía Láctea s\n, La Laguna, 38205
Tenerife,
Spain
e-mail: aasensio@iac.es; rms.iac@gmail.com
4
Departamento de Astrofisica, Univ. de La Laguna, La Laguna, 38205
Tenerife,
Spain
Received: 22 April 2010
Accepted: 17 October 2010
Context. The orbital angular momentum (OAM) of the photon is a property of light from astronomical objects that has not yet been measured. We propose a method of measuring the OAM spectrum of light from an extended natural source, the Sun. Relating the OAM spectrum of different solar areas to its structures could lead to a novel remote sensing technique.
Aims. We present a method for measuring the OAM spectrum of solar photons.
Methods. The THEMIS⋆ telescope is being used with a novel phase-diversity technique. A spatial light modulator is placed on one pupil image, and an ad-hoc optical setup allows the measurement of two simultaneous phase-diverse images in the same CCD, with equal optical paths.
Results. Preliminary results show that very good seeing is mandatory for this kind of observation. The method works in the laboratory, and good seeing conditions in the 2010 campaign are being awaited.
Key words: instrumentation: miscellaneous / techniques: miscellaneous
© ESO, 2010
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