Analysis of EUV Solar Spectrum with Gravity Induced Resonant Emission
arXiv:1705.09956
Abstract
Gravity Induced Resonant Emission (GIRE) is a new phenomenon recently reported; we have analyzed the solar emissions on the basis of GIRE. We have computed the EUV solar spectrum using GIRE wave length as a part of studying coronal heating problem. We find all the solar observations converge in GIRE and the GIRE wave length is sufficient to study all the solar emissions.
16 pages; 4 figures; two tables