L. Moore

activity

20172020

_{3}^{+}

in planetary atmospheres: effects of vertical gradients on observed quantities

33 citations · 74 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2020★ 23 cited

ExoMol line lists -- XL. Ro-vibrational molecular line list for the hydronium ion (H $_{3}$ O $^{+}$ )

S. N. Yurchenko, Jonathan Tennyson, Steve Miller +3

A new line list for hydronium (H $_{3}$ $^{16}$ O $^{+}$ ) is computed. The line list is based on a new ab initio dipole moment surface (CCSD(T)/aug-cc-pVQZ) and a new empirical potential e…

astro-ph.EP2019★ 33 cited

Modelling H $_{3}^{+}$ in planetary atmospheres: effects of vertical gradients on observed quantities

L. Moore, H. Melin, J. O'Donoghue +5

Since its discovery in the aurorae of Jupiter ~30 years ago, the H $_{3}^{+}$ ion has served as an invaluable probe of giant planet upper atmospheres. However, the vast majority of…

astro-ph.EP2017★ 18 cited

The quest for H $_{3}^{+}$ at Neptune: deep burn observations with NASA IRTF iSHELL

H. Melin, L. N. Fletcher, T. S. Stallard +4

Emission from the molecular ion H $_{3}^{+}$ is a powerful diagnostic of the upper atmosphere of Jupiter, Saturn, and Uranus, but it remains undetected at Neptune. In search of this emi…

ExoMol line lists -- XL. Ro-vibrational molecular line list for the hydronium ion (H3​O+)

Modelling H3+​ in planetary atmospheres: effects of vertical gradients on observed quantities

The quest for H3+​ at Neptune: deep burn observations with NASA IRTF iSHELL

ExoMol line lists -- XL. Ro-vibrational molecular line list for the hydronium ion (H $_{3}$ O $^{+}$ )

Modelling H $_{3}^{+}$ in planetary atmospheres: effects of vertical gradients on observed quantities

The quest for H $_{3}^{+}$ at Neptune: deep burn observations with NASA IRTF iSHELL