Status of GNSS ionospheric Study in Korea Jong-Kyun Chung Korea Astronomy & Space Science Institute ISTF/1 – SP/2.
Solar Rotation Lab 3. Differential Rotation The sun lacks a fixed rotation rate Since it is composed of a gaseous plasma, the rate of rotation is fastest.
Solar irradiance variability on hourly to decadal scale from SCIAMACHY and its impact on middle atmospheric ozone and ozone-climate interaction M. Weber,
University of Colorado 1 ; Delft University of Technology 2 ; University of Alaska 3 ; Centre National d’Etudes Spatiales 4 ; National Center for Atmospheric.
A New Bound on the Radar Cross-section of the Sun Bill Coles, UCSD Mike Sulzer and John Harmon, NAIC Jorge Chau and Ron Woodman, JRO We have not observed.
The Response of an Ionosphere to changes in the solar F 10.7 flux: Comparison of Venus, Earth and Mars Paul Withers and Michael Mendillo Boston University.
The Sun Goals: -Summarize the overall properties of the Sun. -Explain how energy travels from the solar core, through the interior, and out into space.
A New Bound on the Radar Cross-section of the Sun Bill Coles, UCSD
