Abstract

Some physical parameters of a neutral component of the coma of comet 103P/Hartley have been obtained by the models of Haser and Shul’man. To compensate a quick proper motion of comets in photometric observations, two techniques are investigated: image recovering with algorithms of the inverse problem solution and the method of effective diaphragms. It has been shown that the method of effective diaphragms is preferable.

Full Text
Paper version not known

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 call

Disclaimer: 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.