Steve Miller
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Science in public: communication, culture, and credibility
J Gregory, S Miller
What can we learn from 25 years of PUS survey research? Liberating and expanding the agenda
MW Bauer, N Allum, S Miller
Public understanding of science 16 (1), 79-95, 2007
Public understanding of science at the crossroads
S Miller
Public understanding of science 10 (1), 115-120, 2001
Detection of H3+ on Jupiter
P Drossart, JP Maillard, J Caldwell, SJ Kim, JKG Watson, WA Majewski, ...
Nature 340 (6234), 539-541, 1989
Policy forum: Interactions with the mass media
HP Peters, D Brossard, S de Cheveigné, S Dunwoody, M Kallfass, ...
Science 321 (5886), 204-205, 2008
Spectroscopic properties of the H 3+ molecule: a new calculated line list
L Neale, S Miller, J Tennyson
The Astrophysical Journal 464, 516, 1996
Science-media interface: It's time to reconsider
HP Peters, D Brossard, S De Cheveigné, S Dunwoody, M Kallfass, ...
Science Communication 30 (2), 266-276, 2008
Deep Impact: Observations from a worldwide Earth-based campaign
KJ Meech, N Ageorges, MF A'Hearn, C Arpigny, A Ates, J Aycock, ...
science 310 (5746), 265-269, 2005
Detection of a noble gas molecular ion, 36ArH+, in the Crab Nebula
MJ Barlow, BM Swinyard, PJ Owen, J Cernicharo, HL Gomez, RJ Ivison, ...
Science 342 (6164), 1343-1345, 2013
Detection of H3 (+) from Uranus
LM Trafton, TR Geballe, S Miller, J Tennyson, GE Ballester
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 405, no. 2, p. 761-766 …, 1993
The influence of H2O line blanketing on the spectra of cool dwarf stars
F Allard, PH Hauschildt, S Miller, J Tennyson
The Astrophysical Journal 426, L39-L41, 1994
Jupiter's polar ionospheric flows: Theoretical interpretation
SWH Cowley, EJ Bunce, TS Stallard, S Miller
Geophysical research letters 30 (5), 2003
EChO: exoplanet characterisation observatory
G Tinetti, JP Beaulieu, T Henning, M Meyer, G Micela, I Ribas, D Stam, ...
Experimental Astronomy 34, 311-353, 2012
JIM: A time‐dependent, three‐dimensional model of Jupiter's thermosphere and ionosphere
N Achilleos, S Miller, J Tennyson, AD Aylward, I Mueller‐Wodarg, D Rees
Journal of Geophysical Research: Planets 103 (E9), 20089-20112, 1998
Triatom: programs for the calculation of ro-vibrational spectra of triatomic molecules
J Tennyson, S Miller, CR Le Sueur
Computer physics communications 75 (3), 339-364, 1993
The role of H+ 3 in planetary atmospheres
S Miller
Philos. Trans. R. Soc 358, 2485-2502, 2000
Identification of Features Due to H(3Plus) in the Infrared Spectrum of Supernova 1987A
S Miller, J Tennyson, S Lepp, A Dalgarno
Nature 355 (6359), 420-422, 1992
Can science communication workshops train scientists for reflexive public engagement? The ESConet experience
S Miller, D Fahy, ESC Team
Science Communication 31 (1), 116-126, 2009
Rapid energy dissipation and variability of the lo–Jupiter electrodynamic circuit
R Prangé, D Rego, D Southwood, P Zarka, S Miller, W Ip
Nature 379 (6563), 323-325, 1996
Infrared emissions of H3 (+) in the atmosphere of Jupiter in the 2.1 and 4.0 micron region
S Miller, RD Joseph, J Tennyson
The Astrophysical Journal 360, L55-L58, 1990
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