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Kappa distributions and with loss cone features have been frequently observedwith flares emissions with the signatures of Lower hybrid waves. We haveanalysed the plasma with Kappa distributions and with loss cone features forthe drift wave instabilities in perpendicular propagation for Large flare andNormal flare and Coronal condition . While analysing the growth/damping rate,we understand that the growth of propagation of EM waves increases with kappadistribution index for all the three cases. In comparing the propagation largeflare shows lesser growth in compared with the normal and the coronal plasmas.When added the loss cone features to Kappa distributions, we find that thedamping of EM wave propagation takes place. The damping rate EM waves isincreases with perpendicular temperature and loss cone index l, in all thethree cases but damping is very high for large flare and then normal incomparision with coronal condition. This shows that the lower hybrid dampingmay be the source of coronal heating.

Analysis of Lower Hybrid Drift Waves in Kappa Distributions over Solar Atmosphere