The power spectrum of the seeing during solar observations
Costantino Sigismondi, Andrea Raponi, Xiaofan Wang, Giulia De Rosi,, Michele Bianda, Renzo Ramelli
TL;DR
This study measures the power spectrum of atmospheric seeing during solar observations across multiple locations to evaluate the reliability of the meridian transits method for solar diameter monitoring.
Contribution
It provides empirical measurements of the seeing power spectrum in the 0.001-1 Hz range at different sites, assessing the method's criticality.
Findings
Power spectrum measured in the 0.001-1 Hz range.
Assessment of meridian transits method reliability.
Empirical data from multiple observation sites.
Abstract
Measurements of the power spectrum of the atmospheric seeing in the line of sight of the Sun, in the range 0.001-1 Hz, have been performed in Santa Maria degli Angeli Lucernaria Dome, at IRSOL and in Huairou Station. This study is aimed to understand the criticity of the meridian transits method for solar diameter monitoring.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomical Observations and Instrumentation · Solar and Space Plasma Dynamics · History and Developments in Astronomy