Zobrazeno 1 - 10
of 409
pro vyhledávání: '"Capria, M."'
Autor:
Bockelée-Morvan, Dominique, Crovisier, J., Erard, S., Capaccioni, F., Leyrat, C., Filacchione, G., Drossart, P., Encrenaz, T., Biver, N., de Sanctis, M.-C., Schmitt, B., Kührt, E., Capria, M.-T., Combes, M., Combi, M., Fougere, N., Arnold, G., Fink, U., Ip, W., Migliorini, A., Piccioni, G., Tozzi, G.
Infrared observations of the coma of 67P/Churyumov-Gerasimenko were carried out from 2015 July to September, i.e. around perihelion (2015 August 13), with the high-resolution channel of the Visible and Infrared Thermal Imaging Spectrometer instrument
Externí odkaz:
http://hdl.handle.net/10150/624745
http://arizona.openrepository.com/arizona/handle/10150/624745
http://arizona.openrepository.com/arizona/handle/10150/624745
Autor:
Migliorini, A., Piccioni, G., Capaccioni, F., Filacchione, G., Bockelée-Morvan, D., Erard, S., Leyrat, C., Combi, M. R., Fougere, N., Crovisier, J., Taylor, F. W., De Sanctis, M. C., Capria, M. T., Grassi, D., Rinaldi, G., Tozzi, G. P., Fink, U.
Context. Studying the coma environment of comet 67P/Churyumov-Gerasimenko (67P) is one of the primary scientific goals of the VIRTIS experiment on the ESA Rosetta mission. Aims. The distribution and variability of water vapour and carbon dioxide in t
Externí odkaz:
http://hdl.handle.net/10150/614953
http://arizona.openrepository.com/arizona/handle/10150/614953
http://arizona.openrepository.com/arizona/handle/10150/614953
Publikováno v:
Planetary and Space Science, Volume 212, March 2022, 105397
The link between the surface temperature of Mercury and the exosphere sodium content has been investigated. Observations show that, along the orbit of Mercury, two maxima of total Na content are present: one at aphelion and one at perihelion. Previou
Externí odkaz:
http://arxiv.org/abs/2202.11467
Autor:
Tubiana, C., Rinaldi, G., Güttler, C., Snodgrass, C., Shi, X., Hu, X., Marschall, R., Fulle, M., Bockelée-Morvan, D., Naletto, G., Capaccioni, F., Sierks, H., Arnold, G., Barucci, M. A., Bertaux, J. -L., Bertini, I., Bodewits, D., Capria, M. T., Ciarniello, M., Cremonese, G., Crovisier, J., Da Deppo, V., Debei, S., De Cecco, M., Deller, J., De Sanctis, M. C., Davidsson, B., Doose, L., Erard, S., Filacchione, G., Fink, U., Formisano, M., Fornasier, S., Gutiérrez, P. J., Ip, W. -H., Ivanovski, S., Kappel, D., Keller, H. U., Kolokolova, L., Koschny, D., Krueger, H., La Forgia, F., Lamy, P. L., Lara, L. M., Lazzarin, M., Levasseur-Regourd, A. C., Lin, Z. -Y., Longobardo, A., López-Moreno, J. J., Marzari, F., Migliorini, A., Mottola, S., Rodrigo, R., Taylor, F., Toth, I., Zakharov, V.
On 27 Apr 2015, when 67P/C-G was at 1.76 au from the Sun and moving towards perihelion, the OSIRIS and VIRTIS-M instruments on Rosetta observed the evolving dust and gas coma during a complete rotation of the comet. We aim to characterize the dust, H
Externí odkaz:
http://arxiv.org/abs/1905.03022
Autor:
Bockelée-Morvan, D., Leyrat, C., Erard, S., Andrieu, F., Capaccioni, F., Filacchione, G., Hasselmann, P. H., Crovisier, J., Drossart, P., Arnold, G., Ciarniello, M., Kappel, D., Longobardo, A., Capria, M. -T., De Sanctis, M. C., Rinaldi, G., Taylor, F.
Publikováno v:
A&A 630, A22 (2019)
We analyze 2-5 micrometre spectroscopic observations of the dust coma of comet 67P/Churyumov-Gerasimenko obtained with the VIRTIS-H instrument onboard Rosetta from 3 June to 29 October 2015 at heliocentric distances r_h = 1.24-1.55 AU. The 2-2.5 micr
Externí odkaz:
http://arxiv.org/abs/1901.03074
Autor:
Snodgrass, C., Jones, G. H., Boehnhardt, H., Gibbings, A., Homeister, M., Andre, N., Beck, P., Bentley, M. S., Bertini, I., Bowles, N., Capria, M. T., Carr, C., Ceriotti, M., Coates, A. J., Della Corte, V., Hanna, K. L. Donaldson, Fitzsimmons, A., Gutierrez, P. J., Hainaut, O. R., Herique, A., Hilchenbach, M., Hsieh, H. H., Jehin, E., Karatekin, O., Kofman, W., Lara, L. M., Laudan, K., Licandro, J., Lowry, S. C., Marzari, F., Masters, A., Meech, K. J., Moreno, F., Morse, A., Orosei, R., Pack, A., Plettemeier, D., Prialnik, D., Rotundi, A., Rubin, M., Sanchez, J. P., Sheridan, S., Trieloff, M., Winterboer, A.
We describe Castalia, a proposed mission to rendezvous with a Main Belt Comet (MBC), 133P/Elst-Pizarro. MBCs are a recently discovered population of apparently icy bodies within the main asteroid belt between Mars and Jupiter, which may represent the
Externí odkaz:
http://arxiv.org/abs/1709.03405
Autor:
Bockelée-Morvan, D., Rinaldi, G., Erard, S., Leyrat, C., Capaccioni, F., Drossart, P., Filacchione, G., Migliorini, A., Quirico, E., Mottola, S., Tozzi, G., Arnold, G., Biver, N., Combes, M., Crovisier, J., Longobardo, A., Blecka, M., Capria, M. -T.
Publikováno v:
MNRAS, 469, S443-S458 (2017) - erratum: S842-S843
We present 2-5 $\mu$m spectroscopic observations of the dust coma of 67P/Churyumov-Gerasimenko obtained with the VIRTIS-H instrument onboard Rosetta during two outbursts that occurred on 2015, 13 September 13.6 h UT and 14 September 18.8 h UT at 1.3
Externí odkaz:
http://arxiv.org/abs/1708.00210
Autor:
Raponi, A., Ciarniello, M., Capaccioni, F., Filacchione, G., Tosi, F., De Sanctis, M. C., Capria, M. T., Barucci, M. A., Longobardo, A., Palomba, E., Kappel, D., Arnold, G., Mottola, S., Rousseau, B., Quirico, E., Rinaldi, G., Erard, S., Bockelee-Morvan, D., Leyrat, C.
Water ice-rich patches have been detected on the surface of comet 67P/Churyumov-Gerasimenko by the VIRTIS hyperspectral imager on-board the Rosetta spacecraft, since the orbital insertion in late August 2014. Among those, three icy patches have been
Externí odkaz:
http://arxiv.org/abs/1612.02231
Autor:
Bockelée-Morvan, D., Crovisier, J., Erard, S., Capaccioni, F., Leyrat, C., Filacchione, G., Drossart, P., Encrenaz, T., Biver, N., de Sanctis, M. -C., Schmitt, B., Kührt, E., Capria, M. -T., Combes, M., Combi, M., Fougere, N., Arnold, G., Fink, U., Ip, W., Migliorini, A., Piccioni, G., Tozzi, G.
Publikováno v:
MNRAS, 462, S170-S183 (2016)
Infrared observations of the coma of 67P/Churyumov-Gerasimenko were carried out from July to September 2015, i.e., around perihelion (13 August 2015), with the high-resolution channel of the VIRTIS instrument onboard Rosetta. We present the analysis
Externí odkaz:
http://arxiv.org/abs/1609.07252
Autor:
Barucci, M. A., Filacchione, G., Fornasier, S., Raponi, A., Deshapriya, J. D. P., Tosi, F., Feller, C., Ciarniello, M., Sierks, H., Capaccioni, F., Pommerol, A., Massironi, M., Oklay, N., Merlin, F., Vincent, J. -B., Fulchignoni, M., Guilbert-Lepoutre, A., Perna, D., Capria, M. T., Hasselmann, P. H., Rousseau, B., Barbieri, C., Bockelee-Morvan, D., Lamy, P. L., De Sanctis, C., Rodrigo, R., Erard, S., Koschny, D., Leyrat, C., Rickman, H., Drossart, P., Keller, H. U., A'Hearn, M. F., Arnold, G., Bertaux, J. -L., Bertini, I., Cerroni, P., Cremonese, G., Da Deppo, V., Davidsson, B. J. R., El-Maarry, Fonti, S., Fulle, M., Groussin, O., Guttler, C.
Publikováno v:
A&A 595, A102 (2016)
Since the orbital insertion of the Rosetta spacecraft, comet 67P/Churyumov-Gerasimenko (67P/C-G) has been mapped by OSIRIS camera and VIRTIS spectro-imager, producing a huge quantity of images and spectra of the comet's nucleus. The aim of this work
Externí odkaz:
http://arxiv.org/abs/1609.00551