Author(s)

L. K. Pande^1,2

¹Theory Group, School of Environmental Sciences, Jawaharlal Nehru University, New Delhi, India.
²C1/1206, Vasant Kunj, New Delhi, India.

We analyze the line data from solar flares to present evidence for the emission spectrum of the recently discussed electron-proton pairs at high temperatures. We also point out that since the pairing phenomenon provides an additional source for these lines—the conventional source being the highly ionized high-Z atoms already existing in the solar atmosphere, we have a plausible explanation of the FIP effect.

Electron-Proton Pairing at High Temperatures, Emission Spectra from Solar Flares, FIP Effect

Pande, L. (2016) Electron-Proton Pairing at High Temperatures, Solar Flares, and the FIP Effect. Journal of Modern Physics, 7, 25-35. doi: 10.4236/jmp.2016.71003.