Solar Astronomy studies the Sun as a physical system and energy source. It investigates solar structure, radiation, and magnetic activity. Physics governs nuclear fusion processes powering the Sun. Solar astronomy explains sunspots, flares, and solar winds. Observations across the electromagnetic spectrum reveal dynamic solar behavior. Solar activity influences space weather and Earth’s climate. This field combines plasma physics, nuclear physics, and radiative transfer. Solar astronomy is essential for understanding stellar processes and heliophysics. It provides insight into fundamental astrophysical phenomena.
Title : Photoaligned azodye nanolayers: New trends for liquid crystal devices
Vladimir Chigrinov, Hong Kong University of Science and Technology, Hong Kong
Title : Where is modern physics heading? Why constants of nature matter
Alexander Unzicker, Pestalozzi Gymnasium Munchen, Germany
Title : Global photochemical model CHARM-DE of the earth’s atmosphere for altitudes 0-130 km
Alexei Krivolutsky, Central Aerological Observatory (CAO), Russian Federation
Title : Nonlinear plasma wave excitation in cylindrical semiconductor waveguides
Amir Sohail, COMSATS University Islamabad, Pakistan
Title : Characterization of quaternary alloy
Yarub Al Douri, European Academy of Sciences, Belgium
Title : Using physics to eliminate implant infection in over 25000 patients to date
Thomas J Webster, Brown University, United States