Skip to main content
. Author manuscript; available in PMC: 2016 Sep 14.
Published in final edited form as: Astrophys J. 2014 Nov 4;796(1):41. doi: 10.1088/0004-637X/796/1/41

Fig. 19.

Fig. 19

Top Panel: β measured by Cuderman (1972) for K + O2 and K + N2. The solid lines through the experimental points are fits of the expression from Jones (1997). The dash line is the estimate β for K + air collisions, which includes the correction for multiple high energy collisions. Bottom Panel: Variation of β for all the meteoric atoms colliding with air, as a function of particle velocity.