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.
@article{arxiv.1705.09956,
title = {Analysis of EUV Solar Spectrum with Gravity Induced Resonant Emission},
author = {Antony Soosaleon and Sunitha Ambrose},
journal= {arXiv preprint arXiv:1705.09956},
year = {2017}
}