Webinar 5: Special Multidisciplinary Webinar
Talk 1 Probing Solar System: PPT and Video
Talk 2 Antarctica - The Journey South: PPT and Video
Talk 3 Probing... interior and outer .... our Sun: PPT and Video
Talk 4 Asteroseismology of Delta Scuti Stars: PPT
This webinar consisted of four talks on a variety of topics. The summary of these are as below:
Talk 2 Antarctica - The Journey South: PPT and Video
Talk 3 Probing... interior and outer .... our Sun: PPT and Video
Talk 4 Asteroseismology of Delta Scuti Stars: PPT
This webinar consisted of four talks on a variety of topics. The summary of these are as below:
1. Probing Solar System by Professor U. C. Joshi on 4th September 2018: Study of minor bodies in solar system (comets and asteroids) is very important to understand the formation of solar system. These possess pristine material to investigate physical conditions that existed at the time of the formation of solar system. The talk covered a brief introduction to the solar system with more emphasis on comets and asteroids.
2. Antarctica - The
Journey South by Mr. Rakesh P. Rao on 5th September 2018: The Antarctic continent spans around 14 million square kilometers in area, of
which 98 % is covered with snow and ice. In last 3 decades, India has built 3
research stations; Dakshina Gangotri, Maitri and Bharati. The presentation highlighted
Antarctica and Southern Ocean. This emphasized the Indian Antarctica
research program.
3. Probing the hidden interior and outer atmosphere of our Sun by
Professor Ashok Ambastha on 6th September 2018: Sun is our nearest star and the only stars where it is possible
to study the outer surface in fine details. However, its interior is hidden
under the dense surface. Similarly, the outer atmosphere of the Sun, where a
host of activities occur, is not directly visible. We discussed various
techniques for probing these aspects of our Sun.
4. Asteroseismology
of Delta Scuti Stars by Mr. Janaka Adassuriya on 7th September 2018: Asteroseismology allows an unprecedented way to determine the
internal structure of stars by studying their oscillations. These oscillations
are radial or non-radial. The UBVRI photometry and high-resolution spectroscopy
can be used to detect the pulsation frequencies of the stellar oscillations and
hence determine the stellar properties.