Zobrazeno 1 - 10
of 17
pro vyhledávání: '"E. H. Wishnow"'
Autor:
Gordon L. Bjoraker, John C. Pearl, Daniel Gautier, Tobias Owen, R. K. Achterberg, Nicholas A Teanby, S. B. Calcutt, V. G. Kunde, Athena Coustenis, C. Ferrari, Mark R. Showalter, Antonella Barucci, Neil Bowles, E. H. Wishnow, Patrick G. J. Irwin, B. Wallis, Linda Spilker, Regis Courtin, John R. Spencer, Scott G. Edgington, F. M. Flasar, Conor A. Nixon, M. E. Segura, Peter L. Read, Amy A. Simon-Miller, Thierry Fouchet, S. Pilorz, Bruno Bézard, Paul N. Romani, A. A. Mamoutkine, Paul J. Schinder, Emmanuel Lellouch, Robert E. Samuelson, Barney J. Conrath, Ronald Carlson, Peter J. Gierasch, Mian M. Abbas, John C. Brasunas, François Raulin, R. Prangé, Fredric W. Taylor, Glenn S. Orton, D. E. Jennings, Darrell F. Strobel, A. Marten, Peter A. R. Ade
Publikováno v:
Science
Science, American Association for the Advancement of Science (AAAS), 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
Science, 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
Science, American Association for the Advancement of Science (AAAS), 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
Science, 2005, 307, pp.1247-1251. ⟨10.1126/science.1105806⟩
International audience; Stratospheric temperatures on Saturn imply a strong decay of the equatorial winds with altitude. If the decrease in winds reported from recent Hubble Space Telescope images is not a temporal change, then the features tracked m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a233a114517cf76158eca7d61ea99131
https://doi.org/10.1126/science.1105806
https://doi.org/10.1126/science.1105806
Publikováno v:
Journal of Quantitative Spectroscopy and Radiative Transfer. 103:102-117
Author Institution: Space Sciences Laboratory, University of California, Berkeley,; CA 94720; and Department of Physics and Astronomy, University of British; Columbia, Vancouver, BC, Canada V6T 1Z1; Jet Propulsion Laboratory, Pasadena, CA 91109; Depa
Publikováno v:
Review of Scientific Instruments. 70:23-31
A far-infrared system used to measure weak absorption spectra of gases at pressures up to a few atmospheres and at temperatures as low as 20 K is described. The principal component is a multiple reflection mirror cell, cooled either with liquid nitro
Publikováno v:
The Astrophysical Journal. 492:843-848
A comparison is made between the observed submillimeter absorption spectrum of normal hydrogen gas at three different temperatures near 25 K and a fully quantum mechanical ab initio calculated spectrum. Measurements cover the wavenumber range 20-320
Publikováno v:
Journal of Molecular Spectroscopy. 170:516-533
The far-infrared spectrum of gaseous CH 3 SiH 3 has been measured with a Fourier transform spectrometer between 180 and 380 cm −1 under relatively large pressure-path length conditions. The absorption path length was 124 m and the pressure was 20 T
Publikováno v:
Physical Review Letters. 65:537-540
We report here the most precise constraint to date on the spectrum of the cosmic background radiation (CBR), obtained from measurements made with a liquid-helium-cooled spectrometer carried above the atmosphere on a rocket. The spectrum is very well
Autor:
James Booth, E. H. Wishnow, C. C. Blake, Walter Hardy, Ulrike Närger, Lorne A. Whitehead, M. E. Hayden, J.F. Carolan, D. A. Balzarini
Publikováno v:
Review of Scientific Instruments. 61:1504-1508
We have developed a low cost continuous flow labyrinth calorimetric system which attains 0.3% accuracy in absolute energy balance and has a minimum sensitivity of 20 mW. This system is ideally suited to measure the energy balance of electrolytic reac
Autor:
M. E. Segura, G. S. Orton, F. M. Flasar, Donald E. Jennings, R. W. Carlson, Bruno Bézard, A. A. Mamoutkine, John C. Brasunas, Gordon L. Bjoraker, S. Vinatier, Pgj Irwin, A. Coustenis, V. G. Kunde, R. K. Achterberg, Conor A. Nixon, John C. Pearl, Amy A. Simon-Miller, Paul N. Romani, E. H. Wishnow
Publikováno v:
Scopus-Elsevier
The Composite Infrared Spectrometer (CIRS) aboard the Cassini spacecraft has been orbiting Saturn for 2-1/2 years. CIRS is a Fourier transform spectrometer that measures atmospheric thermal structure and dynamics, and atmospheric composition, of Satu
Autor:
Emmanuel Lellouch, John C. Brasunas, R. K. Achterberg, Athena Coustenis, Scott G. Edgington, Darrell F. Strobel, Paul N. Romani, A. A. Mamoutkine, Pgj Irwin, Barney J. Conrath, Mark R. Showalter, Regis Courtin, Bruno Bézard, Tobias Owen, John C. Pearl, Ronald Carlson, Nicholas A Teanby, Amy A. Simon-Miller, Fredric W. Taylor, Robert E. Samuelson, Antonella Barucci, Sandrine Vinatier, Paul J. Schinder, C. Ferrari, Peter J. Gierasch, François Raulin, Mian M. Abbas, Gordon L. Bjoraker, E. H. Wishnow, Peter L. Read, M. E. Segura, D. E. Jennings, Linda Spilker, John R. Spencer, A. Marten, Neil Bowles, Peter A. R. Ade, R. Prangé, F. M. Flasar, Conor A. Nixon, Thierry Fouchet, S. B. Calcutt, V. G. Kunde, Daniel Gautier, Glenn S. Orton
Publikováno v:
Science
Science, American Association for the Advancement of Science (AAAS), 2005, 308, pp.975-978. ⟨10.1126/science.1111150⟩
Science, 2005, 308, pp.975-978. ⟨10.1126/science.1111150⟩
Science, American Association for the Advancement of Science (AAAS), 2005, 308, pp.975-978. ⟨10.1126/science.1111150⟩
Science, 2005, 308, pp.975-978. ⟨10.1126/science.1111150⟩
Temperatures obtained from early Cassini infrared observations of Titan show a stratopause at an altitude of 310 kilometers (and 186 kelvin at 15°S). Stratospheric temperatures are coldest in the winter northern hemisphere, with zonal winds reaching
Publikováno v:
Collision-and Interaction-Induced Spectroscopy ISBN: 9789401040822
The collision-induced absorption spectrum of normal hydrogen gas has been measured from 20–320 cm-1, at temperatures in the range 21–38 K, and pressures between 0.6 and 3 atmospheres, over an optical path of 52 and 60 meters. Under these conditio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::173f58f2ef2a4f750a826e63e4e4e885
https://doi.org/10.1007/978-94-011-0183-7_37
https://doi.org/10.1007/978-94-011-0183-7_37