Abstract
In this paper we address the problem of the calibration for the Doppler signal obtained from resonant scattering spectrometers and magneto optical filters that are being used to measure solar oscillations. After discussing current methods of calibration, we suggest and study a new method based on the Stark effect. Our analysis and preliminary test confirm the capability and the advantages of the method.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
