arXiv subjects
Publications and source records attributed to Sunitha Ambrose.
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.
The gravitational drift of ions relative to the electrons induces two type of waves in magnetized plasma; ion acoustic (IO) waves and lower hybrid (LH) waves. The IO waves induced by the gravity are damped by electromagnetic (EM) waves leads to the formation of LH waves. For higher wave vector, these LH wave results in to the resonant absorption and re-emission of EM waves, called as gravity induced resonant emission (gire). A general formula has been derived for gire frequency is convergence of all fundamental quantities.