Science in public: communication, culture, and credibility J Gregory, S Miller | 1711 | 1998 |
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 | 1226 | 2007 |
Public understanding of science at the crossroads S Miller Public understanding of science 10 (1), 115-120, 2001 | 923 | 2001 |
Detection of H3+ on Jupiter P Drossart, JP Maillard, J Caldwell, SJ Kim, JKG Watson, WA Majewski, ... Nature 340 (6234), 539-541, 1989 | 455 | 1989 |
Policy forum: Interactions with the mass media HP Peters, D Brossard, S de Cheveigne, S Dunwoody, M Kallfass, ... Science 321 (5886), 204-205, 2008 | 331 | 2008 |
Spectroscopic properties of the H 3+ molecule: a new calculated line list L Neale, S Miller, J Tennyson Astrophysical Journal v. 464, p. 516 464, 516, 1996 | 253 | 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 | 204 | 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 | 200 | 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 | 186 | 2013 |
Jupiter's polar ionospheric flows: Theoretical interpretation SWH Cowley, EJ Bunce, TS Stallard, S Miller Geophysical research letters 30 (5), 2003 | 164 | 2003 |
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 | 164 | 1993 |
The influence of H2O line blanketing on the spectra of cool dwarf stars F Allard, PH Hauschildt, S Miller, J Tennyson Astrophysical Journal, Part 2-Letters (ISSN 0004-637X), vol. 426, no. 1, p …, 1994 | 152 | 1994 |
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 | 148 | 1998 |
EChO: exoplanet characterisation observatory G Tinetti, JP Beaulieu, T Henning, M Meyer, G Micela, I Ribas, D Stam, ... Experimental Astronomy 34, 311-353, 2012 | 145 | 2012 |
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 | 142 | 1996 |
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 | 134 | 1993 |
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 | 133* | 2009 |
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 | 132 | 1990 |
The role of H+ 3 in planetary atmospheres S Miller Philos. Trans. R. Soc 358, 2485-2502, 2000 | 129 | 2000 |
Jupiter's Thermosphere and Ionosphere R Yelle, S Miller Jupiter: The Planet, Satellites and Magnetosphere, 185-218, 2004 | 128 | 2004 |