2022/09/20 by Srimoyee Samaddar, Samaddar, Srimoyee, Karthik Venkataramani +3
Earth and Planetary Sciences · Physics and Astronomy · #Atmospheric Ozone and Climate #Atmospheric and Oceanic Physics (physics.ao-ph) #Cosmology and Gravitation Theories #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #Solar and Space Plasma Dynamics #Solar and Stellar Astrophysics (astro-ph.SR)
paper · pdf · doi:10.48550/arxiv.2209.10543
openalex publication_date 2022/09/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We use a new Atmospheric Chemistry and Energetics one-dimensional (ACE1D) thermospheric model to show that the energies deposited by the solar soft x-rays in the lower thermosphere at altitudes between 100 -150 km (Bailey et al. 2000), affects the temperature of the entire Earth's thermosphere even at altitudes well above 300 km. By turning off the input solar flux in the different wavelength bins of the model iteratively, we are able to demonstrate that the maximum change in exospheric temperature is due to the changes in the soft x-ray solar bins. We also show, using the thermodynamic heat equation, that the molecular diffusion via non-thermal photoelectrons, is the main source of heat transfer to the upper ionosphere/thermosphere and results in the increase of the temperature of the neutral atmosphere. Moreover, these temperature change and heating effects of the solar soft x-rays are comparable to that of the strong HeII 30.4nm emission. Lastly, we show that the uncertainties in the solar flux irradiance at these soft x-rays wavelengths result in corresponding uncertainties in modeled exospheric temperature and the uncertainties increase with increased solar activity.