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 : Using physics to eliminate implant infection in over 25000 patients to date
Thomas J Webster, Brown University, United States
Title : How the Rad Lab helped avert nuclear war
Thomas F Ramos, Lawrence Livermore National Laboratory, United States
Title : Anisotropic stiffness matrix of bed joint mesh-reinforced masonry: A numerical homogenization approach
Omar Mohammed Daud Shakarneh, Novosibirsk State University of Architecture and Civil Engineering, Russian Federation
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 : Enhanced ferromagnetism in carbon dots polyaniline nanocomposite
Paulo Cesar De Morais, University of Brasilia, Brazil