Zobrazeno 1 - 7
of 7
pro vyhledávání: '"H. U. Kaufl"'
Autor:
A. S. J. Khayat, M. D. Smith, Robert E. Novak, Michael J. Mumma, Paul Hartogh, H. U. Kaufl, Geronimo L. Villanueva, Alan T. Tokunaga, Th. Encrenaz
Publikováno v:
Science
Science, American Association for the Advancement of Science, 2015, 348 (6231), pp.218-221. ⟨10.1126/science.aaa3630⟩
Science, American Association for the Advancement of Science, 2015, 348 (6231), pp.218-221. ⟨10.1126/science.aaa3630⟩
Mapping Mars' water history We know the water cycle on Earth is complex. Neither is it simple on Mars. Infrared maps of water isotopes made by Villanueva et al. show the distribution of H2O and "semiheavy" water (HDO: deuterated water containing a mi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d045ddf2e6ae5d479826c030da9394b3
https://doi.org/10.1126/science.aaa3630
https://doi.org/10.1126/science.aaa3630
Autor:
Michael F. A'Hearn, Aditya Dayal, Yanga R. Fernandez, S. B. Peschke, Joseph L. Hora, Eberhard Grün, H. U. Kaufl, Michael E. Ressler, Giovanni G. Fazio, Timothy A. Livengood, William F. Hoffmann, Martha S. Hanner, Theodor Kostiuk, Carey M. Lisse, Lynne K. Deutsch
Publikováno v:
Earth, Moon, and Planets. 78:251-257
We present infrared imaging and photometry of the bright, giant comet C/1995 O1 (Hale-Bopp). The comet was observed in an extended infrared and optical observing campaign in 1996–1997. The infrared morphology of the comet was observed to change fro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d50c6b91660541d38f034c5e02433bda
https://doi.org/10.1023/a:1006261303055
https://doi.org/10.1023/a:1006261303055
Autor:
O. Marco, Emmanuel Jehin, Gian Paolo Tozzi, Heike Rauer, C. Sterken, Tanyu Bonev, Ivo Saviane, H. U. Kaufl, Fernando Selman, Hermann Böhnhardt, Jean Manfroid, Florian Kerber, Emanuela Pompei, Stefano Bagnulo, N. Ageorges, Olivier Hainaut, G. LoCurto, M. Weiler, L. Barrera, Eric Pantin
Publikováno v:
Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength ISBN: 9783540769583
The collision of Deep Impact with comet 9P/Tempel 1 generated a bright cloud of dust which dissipated during several days after the impact. The brightness variations of this cloud and the changes of its position and shape are governed by the physical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::061fad05e86cda921ae72105cfb42871
http://arxiv.org/abs/astro-ph/0703554
http://arxiv.org/abs/astro-ph/0703554
Autor:
Jean Manfroid, Miroslav Filipovic, Christiaan Sterken, Maria Teresa Capria, M. J. S. Belton, N. Ageorges, U.W. Kamath, L. M. Woodney, Randy D. Campbell, Tomohiko Sekiguchi, Diane H. Wooden, Tetsuharu Fuse, Nicholas B. Suntzeff, S.K. Pandea, Michael J. Mumma, Jacques Crovisier, Emmanuel Jehin, Itsuki Sakon, R. Fugate, H. U. Kaufl, D. Fong, L. Barrera, Anita L. Cochran, Ivo Saviane, Jeremy Bailey, K. von Braun, R. Barrena, G. Ruch, G. R. Stecklein, Sunao Hasegawa, Miquel Serra-Ricart, J. Watanabe, T. Carroll, Damien Hutsemekers, Brian M. Patten, Ronald L. Snell, R. G. Sharp, Takuya Fujiyoshi, S. Fisher, Geraint H. Jones, R. Cleis, Scott J. Wolk, Geoffrey A. Blake, Toshihiko Kadono, Susan M. Lederer, Michael F. A'Hearn, David J. Wilner, William F. Welsh, Daisuke Kinoshita, S.D. Rodgers, L. Dundon, J.-H. Wu, Marc W. Buie, Jianguo Li, Luisa Lara, Yanga R. Fernandez, Paul A. Jones, Wiphu Rujopakarn, Geronimo L. Villanueva, Michael G. Burton, Ramprasad Rao, Florian Kerber, Takaki Miyata, S. M. Larson, Stephen C. Lowry, Remi A. Cabanac, J. Debuizer, Richard J. Wainscoat, Paul R. Weissman, D. K. Sahu, Heike Rauer, Ellen S. Howell, T. Yamashita, Boncho P. Bonev, Stefano Bagnulo, G. P. Tozzi, Hideyo Kawakita, Tushar P. Prabhu, P. Colom, H. Tran, J. Aycock, Andrew J. Coates, Jack D. Drummond, Chick E Woodward, N. Biver, Harold A. Weaver, James E. Lyke, Bin Yang, Patrick Seitzer, Alan Fitzsimmons, Richard Dekany, Michael S. P. Kelley, Zhong-Yi Lin, Shigehisa Takakuwa, M. Sumner, Mark Gurwell, Rita Schulz, Harold J. Reitsema, Karen J. Meech, Bidushi Bhattacharya, Choogon Lee, Gerald Moriarty-Schieven, Samuel Gulkis, O. Marco, D. Harrington, Matthew M. Knight, David E. Harker, Roberto Vázquez, Olivier Hainaut, R. Swaters, M. Schirmer, Z.J. Jiang, X. Zhao, Fernando Selman, Humberto Campins, Tom Stallard, Maria Womack, Daisuke Iono, Noemi Pinilla-Alonso, Pierre Martin, E. Thompson, William M. Jackson, Alan T. Tokunaga, Bryan E. Penprase, Al Conrad, Amy J. Lovell, Mitsuhiko Honda, Rosemary Barber, A. C. Zook, David K. Lynch, A. Delsanti, Hermann Boehnhardt, B. E. A. Mueller, Wing-Huen Ip, G. LoCurto, Xin Zhou, Faith Vilas, Kevin J. Walsh, Peter H. Schultz, Y.-B. Yang, Chunhua Qi, R. Furusho, A. Zauderer, Erika L. Gibb, J. Pittichova, M. Weiler, Steven B. Charnley, Dominique Bockelée-Morvan, Gary J. Melnick, R. Vasundhara, Shigeyuki Sako, Anny Chantal Levasseur-Regourd, David J. Osip, Naruhisa Takato, Claude Arpigny, Iain Coulson, Mitchell Troy, R. Ruane, M. Kidger, Alison B. Peck, Javier Licandro, N. Moskovitz, Carl Hergenrother, Eric Pantin, David A. Neufeld, Colin Snodgrass, N. Dello Russo, Harold M. Butner, Takafumi Ootsubo, P.B. Etzel, Seiji Sugita, J. E. Thomas-Osip, Karen Magee-Sauer, Klaus-Werner Hodapp, W. Weaver, J. de León, James M. Bauer, Olivier Groussin, G. Maheswar, Tony L. Farnham, P. Rodriguez, A. Ates, F. Bensch, G. Petitas, Paul Hirst, Michael A. DiSanti, Rachel Paterno-Mahler, F. Chaffee, Patrick M. Vora, J. van Cleve, J.-M. Zucconi, Tanyu Bonev, Steve Miller, J. Ma, Martin Harwit, Z.-Y. Wu, J. A. Stüwe, Carey M. Lisse, Toshihiro Kasuga, S. Muneer, John Sarkissian, Chadwick A. Trujillo, Emanuela Pompei, Nalin H. Samarasinha, Paul D. Feldman, Qiang Li, Edith Hadamcik, Haruhiko Fujiwara, S. Yokogawa
Publikováno v:
Science
Science, American Association for the Advancement of Science, 2005, 310 (5746), pp.265-269. 〈10.1126/science.1118978〉
Science, American Association for the Advancement of Science, 2005, 310 (5746), pp.265-269. ⟨10.1126/science.1118978⟩
Science, 2005, 310 (5746), pp.265-269. ⟨10.1126/science.1118978⟩
Science, American Association for the Advancement of Science, 2005, 310 (5746), pp.265-269. 〈10.1126/science.1118978〉
Science, American Association for the Advancement of Science, 2005, 310 (5746), pp.265-269. ⟨10.1126/science.1118978⟩
Science, 2005, 310 (5746), pp.265-269. ⟨10.1126/science.1118978⟩
著者人数: 209名
Accepted: 2005-09-01
資料番号: SA1004082000
Accepted: 2005-09-01
資料番号: SA1004082000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2fe3932cefc708eec650d8c9bd5142a3
https://hal.archives-ouvertes.fr/hal-00448665
https://hal.archives-ouvertes.fr/hal-00448665
Publikováno v:
Infrared Physics. 25:505-512
The Venusian atmosphere has been investigated using a 10 μm heterodyne spectrometer (spectral resolution λ/Δλ = 3 × 10 6 ) during upper conjunction and during elongation in 1983. In both cases a variety of spectra from the subsolar region were t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::283c2ca4e1f9f6aa34f757bdc7032869
https://doi.org/10.1016/0020-0891(85)90128-9
https://doi.org/10.1016/0020-0891(85)90128-9
Publikováno v:
Instrumentation and Research Programmes for Small Telescopes ISBN: 9789027723253
Heterodyne spectroscopy combines high instrumental transmission with virtually unlimited spectral resolution. For 250K bodies like Mars and Venus resolution is limited to 107 (=30 m/s) because of photon statistics whereas for solar measurements the c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bfee3aeb4d190b77f9d2f6e4ed16f897
https://doi.org/10.1007/978-94-010-9433-7_84
https://doi.org/10.1007/978-94-010-9433-7_84
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