Milan Gošić

Dr. Gošić is a solar physicist who has been working on the spatio-temporal evolution of the solar magnetic fields using multi-instrument, multiwavelength observations. His field of expertise is space (IRIS, Hinode, and SDO) and ground (SST) solar observations, data processing, and data analysis, which includes techniques such as magnetic feature tracking, magnetic field extrapolations, and inversions of the radiative transfer equation. His work is focused on understanding the origin, structure, and dynamics of the solar magnetic field, and its role in the heating of the solar atmosphere. In his work, Dr. Gošić also employs MHD models to better understand and interpret solar observations. 

Since 2016, Dr. Gošić has been supporting everyday science operations of the IRIS satellite. He has been training solar physicists to perform observations using IRIS and arranging coordinations between IRIS and space and ground-based telescopes such as Hinode, Parker Solar Probe, Solar Orbiter, and SST, to name a few.

Dr. Gošić holds a Ph.D., with cum laude honors, in Solar Physics from the University of Granada, Spain.

• laSexta, the sixth nationwide broadcast television station in Spain published an article about the results reported in Gošić et al. (2014). http://www.lasexta.com/tecnologia-tecnoxplora/sinc/hallan-el-origen-de-la-red-magnetica-que-cubre-la-superficie-del-sol_2015021957fcbb5a0cf2fd8cc6b11092.html
• Gošić et al. (2018) has been selected as a highlight in the AAS Nova. https://aasnova.org/2018/04/23/heating-the-chromosphere-in-the-quiet-sun/
• Recipient of the Thomas Metcalf Travel Award, 6 July 2018

orcid.org

Dr. Gošić's current work focuses on the origin, properties, and spatio-temporal evolution of small-scale magnetic fields, as well as their impact on the energetics and dynamics of the solar atmosphere in various regions, including the quiet Sun, coronal holes, and the solar polar regions.