H3+ cooling in planetary atmospheres.
Miller S, Stallard T, Melin H, Tennyson J.
Miller S, et al. Among authors: tennyson j.
Faraday Discuss. 2010;147:283-91; discussion 379-403. doi: 10.1039/c004152c.
Faraday Discuss. 2010.
PMID: 21302551
In the course of our analysis of this effect, we found that cooling functions that make use of the partition function, Q(T) based on the calculated H3+ energy levels of Neale and Tennyson (Astrophys. J., 1995, 454, L169) may underestimate just how much energy this i …
In the course of our analysis of this effect, we found that cooling functions that make use of the partition function, Q(T) based on the cal …