Abstract
In the model of spherical atmosphere in some planets the intensity of tertiary scattering becomes very predominant, then we must further execute the calculation to a great height of order.The author has devised a new method of evaluation of the phase function of higher order's scattering which is different from the method in the case of tertiary. This can be easily converted to the computer program.
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 callMore From: Journal of the Meteorological Society of Japan. Ser. II
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.
