Application of spatial-coherence spectroscopy for determining the angular diameters of stars: feasibility experiment.

Details Application of spatial-coherence spectroscopy for determining the angular diameters of stars: feasibility experiment. Application of spatial-coherence spectroscopy for determining the angular diameters of stars: feasibility experiment.

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ijpap..36..665k&link_type=abstract

Indian J. Pure Appl. Phys., Vol. 36, No. 11, p. 665 - 674

Astronomy and Astrophysics

Astronomy

2

Spectroscopy: Stellar Diameters

Scientific paper

An experiment is performed in which a new method is used to determine the coherence properties of the wave fields, produced by a broadband source, from the spectral changes produced on interference in the Young's double slit experiment. The knowledge of spectral degree of coherence obtained experimentally combined with the space-frequency equivalence theorem is used to determine the angular diameter of the star which is the source of the field. This is the first experiment showing the application of spatial-coherence spectroscopy in astronomy.

Affiliated with

Also associated with

No associations

Rating

Application of spatial-coherence spectroscopy for determining the angular diameters of stars: feasibility experiment. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Application of spatial-coherence spectroscopy for determining the angular diameters of stars: feasibility experiment., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Application of spatial-coherence spectroscopy for determining the angular diameters of stars: feasibility experiment. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-801322