|
|
|
题名
|
作者
|
年代
|
出处
|
被引量
|
| 1 | Detection of methane in the atmosphere of mars显示文摘 | Formisano V Atreya S Encrenaz T | 2004 | Science2004，306，： | 1 |
| 2 | Detection of methane in the atmosphere of Mars 显示文摘 | FORMISANO V ATREYA S ENCRENAZ T | 2004 | Science2004，306，： | 1 |
| 3 | Water in the Solar System显示文摘 | Thérèse Encrenaz | 2008 | Annual Review of Astronomy and Astrophysics2008，，： | 1 |
| 4 | Detection of Methane in the Atmosphere of Mars显示文摘 | FORMISANO V ATREYA S ENCRENAZ T | 2004 | Science2004，06，： | 1 |
| 5 | A tool for automatic de- tection of deadlock in wormhole networks on chip显示文摘 | S Taktak E Encrenaz J Desbarbieux | 2008 | ACM Transactions on Design Automation of Electronic Systems2008，13，1： | 1 |
| 6 | Ctl-property transformations along an incremental design process显示文摘 | BRAUNSTEIN C ENCRENAZ E | 2007 | Int J Softw Tools Technol Transf2007，9，1： | 1 |
| 7 | Recent developments in millimeter and submillimeter waves显示文摘 | ENCRENAZ P BEAUDIN G | 2000 | Techniques astronomiques/Astronomical Techniques2000，1，10： | 1 |
| 8 | Recent developments in millimeter and suhmillimeter waves显示文摘 | P Encrenaz G Beaudin | 2000 | Techniques astronomiques/ Astronomical techniques2000，1，10： | 1 |
| 9 | Hot salt stress corrosion resistance of Ti 5153 alloy 显示文摘 | Encrenaz M Faure P Petit J A | 1998 | Corrosion Science1998，39，5： | 1 |
| 10 | Detection of methane in the atmosphere of Mars显示文摘 | Formisano V Atreya S Encrenaz T | 2004 | Science2004，306，5702： | 1 |
| 11 | From Solar System to Exoplanets:What can we learn from Planetary Spectroscopy?显示文摘The purpose of this paper is to address the question:Using our knowledge of infrared planetary spectroscopy,what can we learn about the atmospheres of exoplanets?In a first part,a simplified classification of exoplanets,assuming thermochemical equilibrium,is presented,based on their masses and their equilibrium temperatures,in order to propose some possible estimations about their atmospheric composition.In the second part,infrared spectra of planets are discussed,in order to see what lessons can be drawn for exoplanetary spectroscopy.In the last part,we consider the solar system as it would appear from a star located in the ecliptic plane.It first appears that the solar system(except in a few specific cases)would not be seen as a multiple system,because,contrary to many exoplanetary systems,the planets are too far from the Sun and the inclinations of their orbits with respect to the ecliptic plane are too high.Primary transit synthetic spectra of solar system planets are used to discuss the relative merits of transmission and direct emission spectroscopy for probing exoplanetary atmospheres. | Therese Encrenaz | 2022 | Research in Astronomy and Astrophysics2022，22，12： | 0 |
您所在的机构暂未开通此部分的功能，请联系管理员