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of 2 158
pro vyhledávání: '"Cuzzi, J."'
Autor:
Brooks, Shawn M., Becker, Tracy M., Baillié, K., Becker, H. N., Bradley, E. T., Colwell, J. E., Cuzzi, J. N., de Pater, I., Eckert, S., Moutamid, M. El, Edgington, S. G., Estrada, P. R., Evans, M. W., Flandes, A., French, R. G., García, Á., Gordon, M. K., Hedman, M. M., Hsu, H. -W., Jerousek, R. G., Marouf, E. A., Meinke, B. K., Nicholson, P. D., Pilorz, S. H., Showalter, M. R., Spilker, L. J., Throop, H. B., Tiscareno, M. S.
We now know that the outer solar system is host to at least six diverse planetary ring systems, each of which is a scientifically compelling target with the potential to inform us about the evolution, history and even the internal structure of the bo
Externí odkaz:
http://arxiv.org/abs/2008.12418
Autor:
Filacchione, G., Capaccioni, F., Clark, R. N., Nicholson, P. D., Cruikshank, D. P., Cuzzi, J. N., Lunine, J. I., Brown, R. H., Cerroni, P., Tosi, F., Ciarniello, M., Buratti, B. J., Hedman, M. M., Flamini, E.
Over the last eight years, the Visual and Infrared Mapping Spectrometer (VIMS) aboard the Cassini orbiter has returned hyperspectral images in the 0.35-5.1 micron range of the icy satellites and rings of Saturn. These very different objects show sign
Externí odkaz:
http://arxiv.org/abs/1301.6611
Autor:
Hedman, M. M., Nicholson, P. D., Cuzzi, J. N., Clark, R. N., Filacchione, G., Capaccioni, F., Ciarniello, M.
Publikováno v:
Icarus 223 (2013), pp. 105-130
Saturn's main rings exhibit variations in both their opacity and spectral properties on a broad range of spatial scales, and the correlations between these parameters can provide insights into the processes that shape the composition and dynamics of
Externí odkaz:
http://arxiv.org/abs/1210.4727
Autor:
Filacchione, G., Capaccioni, F., Ciarniello, M., Clark, R. N., Cuzzi, J. N., Nicholson, P. D., Cruikshank, D. P., Hedman, M. M., Buratti, B. J., Lunine, J. I., Soderblom, L. A., Tosi, F., Cerroni, P., Brown, R. H., McCord, T. B., Jaumann, R., Stephan, K., Baines, K. H., Flamini, E.
In the last few years Cassini-VIMS, the Visible and Infared Mapping Spectrometer, returned to us a comprehensive view of the Saturn's icy satellites and rings. After having analyzed the satellites' spectral properties (Filacchione et al. (2007a)) and
Externí odkaz:
http://arxiv.org/abs/1203.6230
Publikováno v:
Meteoritics & Planetary Science, vol. 45, 2010, p. 1124
The variation in sizes of chondrules from one chondrite to the next is thought to be due to some sorting process in the early solar nebula. Hypotheses for the sorting process include chondrule sorting by mass and sorting by some aerodynamic mechanism
Externí odkaz:
http://arxiv.org/abs/1110.4111
Autor:
Roellig, T. L., Becklin, E. E., Evans, N. J., De Buizer, J. M., Meixner, M., Tielens, A. G. G. M., Stacey, G. J., Vacca, W. D., Cuzzi, J. N., Backman, D. E.
An updated Science Vision for the SOFIA project is presented, including an overview of the characteristics and capabilities of the observatory and first generation instruments. A primary focus is placed on four science themes: 'The Formation of Stars
Externí odkaz:
http://arxiv.org/abs/0905.4271
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We present a mechanism for chondrules to stick together by means of compaction of a porous dust rim they sweep up as they move through the dusty nebula gas. It is shown that dust aggregates formed out of micron-sized grains stick to chondrules, formi
Externí odkaz:
http://arxiv.org/abs/0802.4048
Autor:
Waite, J. H., Perryman, R. S., Perry, M. E., Miller, K. E., Belll, J., Cravens, T. E., Glein, C. R., Grimes, J., Hedman, M., Cuzzi, J., Brockwell, T., Teolis, B., Moore, L., Mitchell, D. G., Persoon, A., Kurth, W. S., Wahlund, J.-E., Morooka, M., Hadid, L. Z., S. Chocron, J. Walker, Nagy, A., Yelle, R., Ledvina, S., Johnson, R., Tseng, W., Tucker, O. J., Ip, W.-H.
Publikováno v:
Science, 2018 Oct 01. 362(6410), 51-51.
Externí odkaz:
https://www.jstor.org/stable/26568281
Autor:
Ormel, C. W., Cuzzi, J. N.
In this note we present complete, closed-form expressions for random relative velocities between colliding particles of arbitrary size in nebula turbulence. These results are exact for very small particles (those with stopping times much shorter than
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702303