M. N. Chowdhury   T. S. Stallard   K. H. Baines   G. Provan   H. Melin   G. J. Hunt   L. Moore   J. O’Donoghue   E. M. Thomas   R. Wang   S. Miller   S. V. Badman   
J. O’Donoghue   L. Moore   T. Bhakyapaibul   H. Melin   T. Stallard   J. E.P. Connerney   C. Tao   
Nature 596(7870) 54-57 2021年8月 [査読有り]
Jupiter’s upper atmosphere is considerably hotter than expected from the amount of sunlight that it receives1–3. Processes that couple the magnetosphere to the atmosphere give rise to intense auroral emissions and enormous deposition of energy in ...
L. Moore   J. I. Moses   H. Melin   T. S. Stallard   J. O’Donoghue   
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 378(2187) 20200100-20200100 2020年12月 [査読有り]
H
<sub arrange="stack">3
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has been detected at all of the solar system giant planets aside from Neptune. Current observational upper limits imply that there is far less H
<sub arrange="stack">3
<sup arr...
S N Yurchenko   Jonathan Tennyson   Steve Miller   V V Melnikov   J O’Donoghue   L Moore   
Monthly Notices of the Royal Astronomical Society 497(2) 2340-2351 2020年9月 [査読有り]
<title>ABSTRACT</title>
A new line list for hydronium (H316O+) 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 energy surface (PES). The empirical PES of H3O+ was ob...