# Analysis of EUV Solar Spectrum with Gravity Induced Resonant Emission

## TL;DR

This paper introduces Gravity Induced Resonant Emission (GIRE) as a new mechanism to analyze the EUV solar spectrum, providing insights into coronal heating by demonstrating GIRE's ability to account for observed solar emissions.

## Contribution

The study applies GIRE to compute the EUV solar spectrum, showing it can explain all solar observations related to coronal heating.

## Key findings

- GIRE effectively models the EUV solar spectrum.
- GIRE wavelength suffices to study all solar emissions.
- GIRE offers a unified explanation for solar observations.

## 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.