Distance determination method of dust particles using Rosetta OSIRIS NAC and WAC data

Drolshagen E.; Ott T.; Koschny D.; Guetler C.; Tubiana C.; Agarwal J.; Sierks H.; Barbieri C.; Lamy P. I.; Rodrigo R.; Rickman H.; AHearn M. F.; Barucci M. A.; Bertaux J. -L.; Bertini I.; Cremonese G.; Da Deppo V.; Davidsson B.; Debei S.; De Cecco M.; Deller J.; Feller C.; Fornasier S.; Fulle M.; Gicquel A.; Groussin O.; Gutierrez P. J.; Hofmann M.; Hviid S. F.; Ip W. -H.; Jorda L.; Keller H. U.; Knollenberg J.; Kramm J. R.; Kuehrt E.; Kuppers M.; Lara L. M.; Lazzarin M.; Lopez Moreno J. J.; Marzari F.; Naletto G.; Oklay N.; Shi X.; Thomas N.; Poppe B.

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Distance determination method of dust particles using Rosetta OSIRIS NAC and WAC data

机译：利用Rosetta OSIRIS NAC和WAC数据确定尘埃颗粒的距离的方法

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摘要

The ESA Rosetta spacecraft has been tracking its target, the Jupiter-family comet 67P/Churyumov-Gerasimenko, in close vicinity for over two years. It hosts the OSIRIS instruments: the Optical, Spectroscopic, and Infrared Remote Imaging System composed of two cameras, see e.g. Keller et al. (2007). In some imaging sequences dedicated to observe dust particles in the comet's coma, the two cameras took images at the same time.

机译：欧空局罗塞塔号航天器一直在跟踪其目标，即木星家族彗星67P /丘留莫夫-格拉西缅科，近两年来。它托管OSIRIS仪器：由两个摄像头组成的光学，光谱和红外远程成像系统，请参见例如凯勒等。（2007）。在一些专门用于观察彗星昏迷中尘埃的成像序列中，两台摄像机同时拍摄图像。

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来源
《Planetary and space science 》 |2017年第9期| 256-264| 共9页
作者
Drolshagen E.; Ott T.; Koschny D.; Guetler C.; Tubiana C.; Agarwal J.; Sierks H.; Barbieri C.; Lamy P. I.; Rodrigo R.; Rickman H.; AHearn M. F.; Barucci M. A.; Bertaux J. -L.; Bertini I.; Cremonese G.; Da Deppo V.; Davidsson B.; Debei S.; De Cecco M.; Deller J.; Feller C.; Fornasier S.; Fulle M.; Gicquel A.; Groussin O.; Gutierrez P. J.; Hofmann M.; Hviid S. F.; Ip W. -H.; Jorda L.; Keller H. U.; Knollenberg J.; Kramm J. R.; Kuehrt E.; Kuppers M.; Lara L. M.; Lazzarin M.; Lopez Moreno J. J.; Marzari F.; Naletto G.; Oklay N.; Shi X.; Thomas N.; Poppe B.;
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作者单位

Carl von Ossietzky Univ Oldenburg, Ammerlander Heerstr 114, D-26111 Oldenburg, Germany;

Carl von Ossietzky Univ Oldenburg, Ammerlander Heerstr 114, D-26111 Oldenburg, Germany;

ESA ESTEC, NL-2201 AZ Noordwijk, Netherlands|Tech Univ Munich, Chair Astronaut, Munich, Germany;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

Univ Padua, Dept Phys & Astron, Vicolo Osservatorio 3, I-35122 Padua, Italy;

CNRS, UMR 7326, Lab Astrophys Marseille, F-13388 Marseille 13, France|Aix Marseille Univ, F-13388 Marseille 13, France;

CSIC, INTA, Ctr Astrobiol, Madrid 28850, Spain|Int Space Sci Inst, CH-3012 Bern, Switzerland;

Uppsala Univ, Dept Phys & Astron, S-75120 Uppsala, Sweden|PAS Space Res Ctr, PL-00716 Warsaw, Poland;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany|Univ Maryland, Dept Astron, College Pk, MD 20742 USA|Jet Prop Lab, M-S 183-301,4800 Oak Grove Dr, Pasadena, CA 91109 USA;

Sorbonne Univ, UPMC Univ Paris 06, PSL Res Univ, LESIA,Observ Paris,CNRS,Univ Paris Diderot,Sorbon, 5 Pl Jules Janssen, F-92195 Meudon, France;

UVSQ, CNRS, IPSL, LATMOS, 11 Blvd Alembert, F-78280 Guyancourt, France;

Univ Padua, Ctr Ateneo Studi & Attivita Spaziali Giuseppe Col, Via Venezia 15, I-35131 Padua, Italy;

INAF, Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy;

CNR, IFN UOS Padova LUXOR, Via Trasea 7, I-35131 Padua, Italy;

Univ Padua, Dept Ind Engn, Via Venezia 1, I-35131 Padua, Italy;

Univ Trento, Via Sommar 9, I-38123 Trento, Italy;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

INAF, Osservatorio Astron Trieste, Via Tiepolo 11, I-34143 Trieste, Italy;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

Aix Marseille Univ, CNRS, Lab Astrophys Marseille, UMR 7326, 38 Rue Frederic Joliot Curier, F-13388 Marseille, France;

CSIC, Inst Astrofis Andalucia, C Glorieta Astron S-N, E-18008 Granada, Spain;

Deutsch Zentrum Luft & Raumfahrt DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany;

Natl Cent Univ, Grad Inst Astron, 300 Chung Da Rd, Chungli 32054, Taiwan|Macau Univ Sci & Technol, Space Sci Inst, Macau, Peoples R China;

Aix Marseille Univ, CNRS, Lab Astrophys Marseille, UMR 7326, 38 Rue Frederic Joliot Curier, F-13388 Marseille, France;

Deutsch Zentrum Luft & Raumfahrt DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany|Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, Mendelssohnstr 3, D-38106 Braunschweig, Germany;

Deutsch Zentrum Luft & Raumfahrt DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany;

Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany;

Deutsch Zentrum Luft & Raumfahrt DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany;

European Space Astron Ctr ESA, Operat Dept, POB 78, Madrid 28691, Spain;

CSIC, Inst Astrofis Andalucia, C Glorieta Astron S-N, E-18008 Granada, Spain;

CSIC, Inst Astrofis Andalucia, C Glorieta Astron S-N, E-18008 Granada, Spain;

Univ Padua, Ctr Ateneo Studi & Attivita Spaziali Giuseppe Col, Via Venezia 15, I-35131 Padua, Italy|CNR, IFN UOS Padova LUXOR, Via Trasea 7, I-35131 Padua, Italy|Univ Padua, Dept Informat Engn, I-35131 Padua, Italy;

Deutsch Zentrum Luft & Raumfahrt DLR, Inst Planetenforsch, Rutherfordstr 2, D-12489 Berlin, Germany;

Univ Bern, Phys Inst, Sidlerstr 5, CH-3012 Bern, Switzerland|Univ Bern, Ctr Space & Habitabil, CH-3012 Bern, Switzerland;

Carl von Ossietzky Univ Oldenburg, Ammerlander Heerstr 114, D-26111 Oldenburg, Germany;

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正文语种 eng
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关键词
Parallax; Stereo observations; Comets; 67P/Churyumov-Gerasimenko; Rosetta; Dust;

机译：视差;立体观测;彗星;67P / Churyumov-Gerasimenko;Rosetta;灰尘;

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专利

1. The dust environment of comet 67P/Churyumov-Gerasimenko from Rosetta OSIRIS and VLT observations in the 4.5 to 2.9 AU heliocentric distance range inbound [J] . F. Moreno, C. Snodgrass, O. Hainaut, Astronomy and astrophysics . 2016 ,第21期

机译：Rosetta OSIRIS的67P / Churyumov-Gerasimenko彗星的尘埃环境和4.5至2.9 AU日心距离范围内的VLT观测
2. The northern hemisphere of asteroid (21) Lutetia-topography and orthoimages from Rosetta OSIRIS NAC image data [J] . Frank Preusker, Frank Scholten, Joerg Knollenberg, Planetary and space science . 2012 ,第1期

机译：小行星的北半球（21）Lutetia地形和来自Rosetta OSIRIS NAC图像数据的正射像
3. Diurnal variation of dust and gas production in comet 67P/Churyumov-Gerasimenko at the inbound equinox as seen by OSIRIS and VIRTIS-M on board Rosetta [J] . C. Tubiana, G. Rinaldi, C. Güttler, Astronomy and astrophysics . 2019 ,第19期

机译：如罗塞塔号上的OSIRIS和VIRTIS-M所见，在入口春分点，67P / Churyumov-Gerasimenko彗星的尘埃和气体产生的昼夜变化
4. Data processing unit for the rosetta osiris instrument [C] . Anja Christen, Richard Wiest, Paul Rastetter, Conference on DASIA 2000: DAta Systems In Aerospace 22-26, May 2000 Montreal, Canada . 2000

机译：Rosetta Osiris仪器的数据处理单元
5. Determination of the Exposure of Furnace Slag Bagging Operators to Nuisance Dusts and Heavy Metals at a Furnace Slag Bagging Operation. [D] . Sologub, Joseph W. 1991

机译：确定炉渣装袋操作员在炉渣装袋操作中暴露于有害粉尘和重金属的暴露。
6. Comparison of two methods for indirect measurement of atmospheric dust deposition: Street-dust composition and vegetation-health status derived from hyperspectral image data [O] . Gorazd Žibret, Veronika Kopačková 2019

机译：两种间接测量大气尘埃沉积的方法的比较：高光谱图像数据得出的街道尘埃组成和植被健康状况
7. Distance determination method of dust particles using Rosetta OSIRIS NAC and WAC data [O] . Drolshagen, Esther, Ott, Theresa, Koschny, Detlef, 2017

机译：利用Rosetta OSIRIS NAC和WAC数据确定尘埃颗粒的距离的方法
8. Dust particle calibration of instrumentation for dust particle velocity and trajectory determination [R] . Simpson, J. A. 1990

机译：用于尘埃粒子速度和轨迹确定的仪器的尘埃粒子校准

Distance determination method of dust particles using Rosetta OSIRIS NAC and WAC data

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