Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aj....137.3398y&link_type=abstract
The Astronomical Journal, Volume 137, Issue 2, pp. 3398-3403 (2009).
Astronomy and Astrophysics
Astronomy
Methods: Numerical, Occultations
Scientific paper
Calculation of a stellar occultation lightcurve from an assumed refractivity profile involves the integral of the refractivity or its derivatives along the line of sight through an atmosphere. For the general case, normal numerical integration can be time consuming for least-squares fitting with a modest number of free parameters, or for calculation at a fine grid for comparison with local refocusing ("spikes") in a lightcurve. A new method, based on the Fourier decomposition of the refractivity profile, can rapidly calculate the line-of-sight integrals needed for occultations. The method is formulated for small planets, to be applicable to Pluto and Triton. The Fourier decomposition method may have applicability to a wider range of atmospheric studies.
No associations
LandOfFree
Rapid Computation of Occultation Lightcurves Using Fourier Decomposition 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 Rapid Computation of Occultation Lightcurves Using Fourier Decomposition, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapid Computation of Occultation Lightcurves Using Fourier Decomposition will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-836218