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See detailLes marqueurs tissulaires dans l'infarctus du myocarde
Chapelle, Jean-Paul ULg

Conference (1989, December 02)

Detailed reference viewed: 14 (0 ULg)
Peer Reviewed
See detailMarqueurs tumoraux
Charlier, Corinne ULg; Plomteux, Guy ULg

in Focus Diagnostica (1994), 2

Detailed reference viewed: 9 (0 ULg)
See detailLe Marquis de Sade : un libre-penseur ?
Durand, Pascal ULg

Conference given outside the academic context (2011)

Detailed reference viewed: 34 (8 ULg)
Full Text
Peer Reviewed
See detailMarrow stromal cell recovery after radiation-induced aplasia in mice
Almohamad, Khaled; Thiry, Albert ULg; Hubin, Frédérique et al

in International Journal of Radiation Biology (2003), 79(4), 259-67

Detailed reference viewed: 29 (2 ULg)
See detailMars atmospheric escape constrained using MAVEN IUVS coronal observations
Chaffin, Michael S.; Deighan, Justin; Chaufray, Jean-Yves et al

in AAS/Division for Planetary Sciences Meeting Abstracts (2015, November 01)

Every planetary atmosphere is capped by a corona: an extended, extremely tenuous region where collisions are negligible and particles follow ballistic trajectories. At Mars, the corona is especially ... [more ▼]

Every planetary atmosphere is capped by a corona: an extended, extremely tenuous region where collisions are negligible and particles follow ballistic trajectories. At Mars, the corona is especially extended due to the low gravity of the planet, and a large number of coronal particles are on escaping trajectories. Such escape has played a critical role in the history of the Mars system, likely removing a substantial fraction of the water initially present on the planet, but the mechanism and magnitude of this escape remains poorly constrained. Currently in orbit at Mars, MAVEN's Imaging Ultraviolet Spectrograph (IUVS) is mapping the distribution of oxygen and hydrogen above 200 km at a high spatial and temporal cadence, revealing a dynamic corona in unprecedented detail. Results will be presented demonstrating that the H in the corona is not spherically symmetric in its distribution, and can potentially be used as a tracer of thermospheric general circulation; and that non-thermal "hot" O (in contrast with more spatially confined "cold" thermal O) is ionospherically sourced with a characteristic energy of 1.1 eV and responds to solar EUV forcing. These results will be interpreted in terms of their impact on our current understanding of how atmospheric escape operates today. We will also discuss how these processes may have acted in the past to deplete Mars' initial water inventory, potentially altering the redox balance of the planet and atmosphere through differential escape of H and O. [less ▲]

Detailed reference viewed: 5 (1 ULg)
See detailMars atmospheric escape constrained using MAVEN IUVS coronal observations
Chaffin; Deighan; Chauffray et al

Conference (2015, October)

Detailed reference viewed: 17 (1 ULg)
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See detailMars aurora review
Stiepen, Arnaud ULg

Conference (2014, July)

Detailed reference viewed: 35 (4 ULg)
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See detailMars dayglow review
Stiepen, Arnaud ULg

Conference (2014, July)

Detailed reference viewed: 16 (1 ULg)
See detailThe Mars discrete aurora: Mars Express observations and modeling.
Gérard, Jean-Claude ULg

Scientific conference (2015, June)

Summary of earlier work Detection of additional ultraviolet auroral events (nadir and limb) Concurrent SPICAM-­‐ASPERA 3 observations Model results Perspectives

Detailed reference viewed: 38 (2 ULg)
See detailThe Mars discrete aurora: morphology, altitude and role of crustal magnetic field
Gérard, Jean-Claude ULg

Scientific conference (2015, December 01)

We present results obtained during 2015 in the framework of BELSPO's SCOOP/BRAIN project. They concern the morphology, frequency, structure of the Mars discrete aurora and the influence of the residual ... [more ▼]

We present results obtained during 2015 in the framework of BELSPO's SCOOP/BRAIN project. They concern the morphology, frequency, structure of the Mars discrete aurora and the influence of the residual crustal magnetic field. [less ▲]

Detailed reference viewed: 47 (5 ULg)
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See detailMars nightglow review
Stiepen, Arnaud ULg

Conference (2014, July)

Detailed reference viewed: 23 (4 ULg)
Full Text
See detailMars nighttime aurora
European Space Agency, ESA/ATG medialab; Gérard, Jean-Claude ULg; Soret, Lauriane ULg

E-print/Working paper (2015)

Press release by the European Space Agency (ESA) on the occasion of the publication in two journals of the peer-reviewed literature

Detailed reference viewed: 26 (1 ULg)
See detailMars Ozone mapping with MAVEN IUVS
Lefèvre; Stiepen, Arnaud ULg; IUVS team

Conference (2017, January 20)

Detailed reference viewed: 13 (1 ULg)
See detailMars Ozone Mapping with MAVEN IUVS
Lefèvre; IUVS team; Stiepen, Arnaud ULg

Poster (2015, December)

Detailed reference viewed: 14 (0 ULg)