More Than Before: Increase In Estimated Oxygen Photochemical Escape Rates From Emm Data And Updated Modeling. K. Chirakkil, Laboratory For Atmospheric And Space Physics, University Of Colorado Boulder, Boulder, Co, Usa (Krishnaprasad.Chirakkil@Lasp.Colorado.Edu); Space And Planetary Science Center, Khalifa University, Abu Dhabi, Uae, J. Deighan, Laboratory For Atmospheric And Space Physics, University Of Colorado Boulder, Boulder, Co, Usa, R. Lillis, Space Sciences Laboratory, University Of California, Berkeley, Ca, Usa, R. Elliott, M. Chaffin, S. Jain, Laboratory For Atmospheric And Space Physics, University Of Colorado Boulder, Boulder, Co, Usa, M. Gacesa, Space And Planetary Science Center, And Department Of Physics, Khalifa University, Abu Dhabi, Uae, M. Fillingim, Space Sciences Laboratory, University Of California, Berkeley, Ca, Usa, G. Holsclaw, Laboratory For Atmospheric And Space Physics, University Of Colorado Boulder, Boulder, Co, Usa, H. Almatroushi, Mohammed Bin Rashid Space Center, Dubai, Uae, D. Brain, Laboratory For Atmospheric And Space Physics, University Of Colorado Boulder, Boulder, Co, Usa, S. England, Aerospace And Ocean Engineering, Virginia Polytechnic Institute And State University, Blacksburg, Va, Usa, S. Raghuram, Laboratory For Atmospheric And Space Physics, University Of Colorado Boulder, Boulder, Co, Usa; Space And Planetary Science Center, Khalifa University, Abu Dhabi, Uae, F. Lootah, Mohammed Bin Rashid Space Center, Dubai, Uae, H. Almazmi, Uae Space Agency, Abu Dhabi, Uae. Introduction Atmospheric Escape Plays A Major Role In The Climate History And Evolution Of Mars. Quantitative Characterization Of The Current Atmospheric Loss Rate Is Thus Crucial To Understanding The Evolution Of Water And Co2 Inventories At Mars. During The Present Epoch, The Photochemical Escape Of Neutral Atoms Such As O, N, C And H Is Understood To Be A Major Non-Thermal Escape Mechanism. One Of The Critical But Less Certain Parameter In