Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials
| ISSN: |
0019-1035
|
|---|---|
| Source: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
|
| Topics: |
Physics
|
| Type of Medium: |
Electronic Resource
|
| URL: |
| _version_ | 1798290861552828416 |
|---|---|
| autor | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. |
| autorsonst | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. |
| book_url | http://dx.doi.org/10.1016/0019-1035(90)90208-Q |
| datenlieferant | nat_lic_papers |
| fussnote | We present in this paper a simulation of P/Halley spectra between 3 and 4 μm obtained by means of extinction efficiencies measured in the laboratory for different carbonaceous materials: hydrogenated amorphous carbon and three kinds of vitrinite. The behavior of the laboratory spectra appears to satisfactorily fit the astronomical observations. In addition, in situ investigations on ''CHON'' particles performed with PUMA 1 and 2 and PIA mass spectrometers on board Vega 1 and 2 and Giotto spacecraft seem to confirm the similarity between cometary carbonaceous particles and those analyzed in the laboratory in terms of physical structure. |
| hauptsatz | hsatz_simple |
| identnr | NLZ180437046 |
| iqvoc_descriptor_title | iqvoc_00000786:Simulation iqvoc_00000092:materials |
| issn | 0019-1035 |
| journal_name | Icarus |
| materialart | 1 |
| package_name | Elsevier |
| publikationsort | Amsterdam |
| publisher | Elsevier |
| reference | 86 (1990), S. 198-207 |
| search_space | articles |
| shingle_author_1 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. |
| shingle_author_2 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. |
| shingle_author_3 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. |
| shingle_author_4 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. |
| shingle_catch_all_1 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials 0019-1035 00191035 Elsevier |
| shingle_catch_all_2 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials 0019-1035 00191035 Elsevier |
| shingle_catch_all_3 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials 0019-1035 00191035 Elsevier |
| shingle_catch_all_4 | Colangeli, L. Bussoletti, E. Papoular, R. Mennella, V. Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials 0019-1035 00191035 Elsevier |
| shingle_title_1 | Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials |
| shingle_title_2 | Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials |
| shingle_title_3 | Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials |
| shingle_title_4 | Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
| timestamp | 2024-05-06T08:23:28.003Z |
| titel | Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials |
| titel_suche | Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materials We present in this paper a simulation of P/Halley spectra between 3 and 4 μm obtained by means of extinction efficiencies measured in the laboratory for different carbonaceous materials: hydrogenated amorphous carbon and three kinds of vitrinite. The behavior of the laboratory spectra appears to satisfactorily fit the astronomical observations. In addition, in situ investigations on ''CHON'' particles performed with PUMA 1 and 2 and PIA mass spectrometers on board Vega 1 and 2 and Giotto spacecraft seem to confirm the similarity between cometary carbonaceous particles and those analyzed in the laboratory in terms of physical structure. |
| topic | U |
| uid | nat_lic_papers_NLZ180437046 |