Filter your results
- 3
- 2
- 4
- 1
- 5
- 1
- 1
- 2
- 1
- 1
- 5
- 5
- 5
- 2
- 1
- 1
- 1
- 1
- 5
- 5
- 4
- 3
- 2
- 2
- 2
- 2
- 2
- 2
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
|
|
sorted by
|
Titan’s surface properties inferred from the seasonal brightness variation at 2-cm wavelengthEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-263
Conference papers
insu-01211569v1
|
|||
Why is Enceladus' surface so radar-bright?American Geophysical Union, Fall Meeting 2012, Dec 2012, San Francisco, United States. pp.abstract #P32A-08
Conference papers
hal-01076945v1
|
|||
|
Cryovolcanic Features on TitanEuropean Planetary Science Congress 2013, Sep 2013, Londres, United Kingdom. pp.EPSC2013-253-2
Conference papers
hal-01073782v1
|
||
|
Composition, seasonal change and bathymetry of Ligeia Mare, Titan, derived from its 2.2-cm thermal emissionEuropean Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-504
Conference papers
insu-01211601v1
|
||
|
Composition, seasonal change and bathymetry of Ligeia Mare, Titan, derived from its microwave thermal emissionJournal of Geophysical Research. Planets, 2016, 121 (2), pp.233-251. ⟨10.1002/2015JE004920⟩
Journal articles
hal-01259869v1
|