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pro vyhledávání: '"M, Maurette"'
Autor:
M. Maurette
Publikováno v:
EAS Publications Series
Path and the Universe: A symposium to celebrate the 25th anniversary of the Path hypothesis
Path and the Universe: A symposium to celebrate the 25th anniversary of the Path hypothesis, May 2010, Toulouse, France. pp.319-326, ⟨10.1051/eas/1146033⟩
Path and the Universe: A symposium to celebrate the 25th anniversary of the Path hypothesis
Path and the Universe: A symposium to celebrate the 25th anniversary of the Path hypothesis, May 2010, Toulouse, France. pp.319-326, ⟨10.1051/eas/1146033⟩
Lunar minerals and impact glasses, convert the polyatomic beam of solar wind (SW) ions into a flux of small molecules ( e.g. , H 2 , N 2 , H 2 O, CO, CO 2 , CH 4 , C 2 H 4 , C 2 H 6 , HCN, metal carbides and deuterides, etc.). They thus behave as “
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec5a3c7f10752cb18e61b8168d16a1e7
https://doi.org/10.1051/978-2-7598-2482-3-035
https://doi.org/10.1051/978-2-7598-2482-3-035
Publikováno v:
Advances in Space Research. 39:605-611
We recovered micrometeorites from surface snow layers near the French-Italian station CONCORDIA. The unique weather and isolation conditions of Dome C allowed us to recover micrometeorites that are much better preserved than those extracted from blue
Publikováno v:
Advances in Space Research. 38:701-708
The contribution of the accretion of “juvenile” micrometeorites to the volatile inventory of the Martian atmosphere had to mostly occur during the period of the late heavy bombardment of the inner solar system, prior to about 3.5 Ga ago, when the
Autor:
Matthieu Gounelle, Franz Brandstätter, Kevin D. McKeegan, M. Maurette, Gero Kurat, C. Engrand
Publikováno v:
Meteoritics & Planetary Science. 40:917-932
We have investigated the texture, bulk chemistry, mineralogy, as well as the anhydrous minerals oxygen isotopic composition of 67 small Antarctic micrometeorites (AMMs) collected at Cap Prudhomme, Antarctica, and belonging to the currently poorly stu
Publikováno v:
EAS Publications Series. 14:51-56
We launched a program to recover cosmic dust (micrometeorites) from Dome C surface snow near the French-Italian station CONCORDIA. The Dome C snow is uniquely shielded from both morainic debris and aeolian dust within the micrometeorite size range (
Publikováno v:
Photodermatology, Photoimmunology & Photomedicine. 19:182-189
Background/Aims: The ultraviolet (UV) portion of sunlight is involved in the induction and development of skin cancers against which a limited photoprotection may be provided by reduced time of exposure, clothing, and sunscreen applications. The conc
Autor:
M. Maurette
Publikováno v:
Autonomous Robots. 14:199-208
Autonomous navigation of a rover on Mars surface can improve very significantly the daily traverse, particularly when driving away from the lander, into unknown areas. The autonomous navigation process developed at CNES is based on stereo cameras per
Publikováno v:
Meteoritics and Planetary Science
Meteoritics and Planetary Science, Wiley, 2001, 36, pp.1377-1396
Meteoritics and Planetary Science, Wiley, 2001, 36, pp.1377-1396
— Depending on their velocity, entry angle and mass, micrometeorites suffer different degrees of heating during their deceleration in the Earth's atmosphere, leading, in most cases, to significant textural, mineralogical and chemical modifications.
Publikováno v:
Meteoritics and Planetary Science
Meteoritics and Planetary Science, Wiley, 1999, 34, pp.773-786
Meteoritics and Planetary Science, Wiley, 1999, 34, pp.773-786
— The D/H ratios and water contents were measured by ion microprobe analysis in 52 individual Antarctic micrometeorites (AMMs) and 10 Antarctic cosmic spherules (ACSs) containing nuggets of iron hydroxide (COPS phase). In AMMs, δD values vary from
Autor:
M. Maurette, C. Engrand
Publikováno v:
Meteoritics and Planetary Science
Meteoritics and Planetary Science, Wiley, 1998, 33, pp.565-580
Meteoritics and Planetary Science, Wiley, 1998, 33, pp.565-580
Over 100 000 large interplanetary dust particles in the 50-500 micrometers size range have been recovered in clean conditions from approximately 600 tons of Antarctic melt ice water as both unmelted and partially melted/dehydrated micrometeorites and