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Peer Reviewed
See detailInvolvement of z-MMP-2 in Zebrafish lymphangiogenesis
Paupert, Jenny ULg; Pendeville, Hélène; Detry, Benoît ULg et al

Conference (2011)

Detailed reference viewed: 16 (2 ULg)
See detailInvolving Students in planning the learning process
Schillings, Patricia ULg

in Garbe, C.; Holle, K.; Weinhold, S. (Eds.) Adore-Teaching struggling adolescent readers in European Countries. Key elements of good practices (2010)

Detailed reference viewed: 10 (5 ULg)
See detailInvolving Students in texts
Schillings, Patricia ULg; Gabelica, C.

in Garbe, C.; Holle, K.; Weinhold, S. (Eds.) Adore-Teaching struggling adolescent readers in European Countries. Key elements of good practices (2010)

Detailed reference viewed: 6 (3 ULg)
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See detailInżyneria powierzchni betonu. Część 1. Struktura geometryczna powierzchni.
Garbacz, Andrzej; Piotrowski, Tomasz; Courard, Luc ULg

in Materialy Budowlane (2006), 9

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See detailInżyneria powierzchni betonu. Część 1. Struktura geometryczna powierzchni.
Garbacz, Andrzej; Piotrowski, Tomasz; Courard, Luc ULg

in Materialy Budowlane (2006), 9

Detailed reference viewed: 12 (1 ULg)
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See detailInżyneria powierzchni betonu. Część 2. Wpływ obrobki na powstawanie rys
Courard, Luc ULg; Garbacz, Andrzej; Nieweglowska, Anna et al

in Materialy Budowlane (2006), 12

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See detailInżynieria powierzchni betonu. Część 3. Termodynamiczne uwarunkowania adhezji
Courard, Luc ULg; Garbacz, Andrzej; Piotrowski, Tomasz

in Materialy Budowlane (2007), 2

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See detailThe Io Footprint Morphology
Jacobsen, Sven; Saur, Joachim; Neubauer, F. M. et al

Conference (2008, September 23)

The innermost Galilean moon Io is embedded in a dense plasma torus. It disturbs the flow of the corotating torus plasma and generates MHD waves. Especially the Alfv ́ n e mode, which carries electric ... [more ▼]

The innermost Galilean moon Io is embedded in a dense plasma torus. It disturbs the flow of the corotating torus plasma and generates MHD waves. Especially the Alfv ́ n e mode, which carries electric currents along the magnetic field, is responsible for the famous Io footprint in the Jo- vian aurora. The Alfv ́ n waves are partly reflected at plasma e density gradients e.g. at the torus edges and form a compli- cated wave pattern. The footprint morphology in the Jovian aurora displays this pattern. Besides the main spot feature, a trailing wake extending over up to 100 degrees and occa- sionally occurring multiple spots indicating reflections have been identified. The intensity, the occurrence of multiple spots and the inter-spot distances have been found to vary strongly [1]. Io is moving up and down in the plasma torus confined to the centrifugal equator. It interacts with a dense plasma when located in the torus center and considerably thinner plasma at the torus flanks. The incoming plasma density controls the interaction strength and wave amplitude. This primar- ily leads to a relationship between the footprint brightness and Io’s centrifugal latitude [1]. However, it has also been shown that the reflection angle is strongly depending on the wave amplitude due to nonlinear effects [2]. This has an impact on the inter-spot distances. On the other hand this parameter is also directly affected when Io changes its posi- tion in the plasma torus. To deconvolve this system we present the results of our 3D MHD simulations showing the influence of Io’s centrifugal latitude and nonlinearities on the footprint morphology par- ticularly on the number of spots and inter-spot distances. We observe interference phenomena leading to locally en- hanced or reduced footprint brightness. We also discuss the recently observed leading spot feature [3]. [less ▲]

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See detailIo footprint: Position, Multiplicity, Variability
Bonfond, Bertrand ULg; Gérard, Jean-Claude ULg; Grodent, Denis ULg et al

Conference (2006, July)

Detailed reference viewed: 4 (1 ULg)
See detailIo plasma torus science through UV remote sensing
Grodent, Denis ULg

Scientific conference (2013, November)

In this presentation, I am providing a short review of the scientific information on the Io plasma torus that may be inferred from UV remote sensing. This includes past observations with the Hubble Space ... [more ▼]

In this presentation, I am providing a short review of the scientific information on the Io plasma torus that may be inferred from UV remote sensing. This includes past observations with the Hubble Space Telescope and the Cassini-UVIS spectrograph during the 2000-Jupiter flyby and future observations with the EXCEED (Sprint-A) telescope. [less ▲]

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See detailIo robot tu bambino
Denis, Brigitte ULg

in Compuscuola (1989), 38(juin), 43-48

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See detailThe Io UV footprint: Location, inter-spot distances and tail vertical extent
Bonfond, Bertrand ULg; Grodent, Denis ULg; Gérard, Jean-Claude ULg et al

in Journal of Geophysical Research. Space Physics (2009), 114

The Io footprint (IFP) consists of one or several spots observed in both jovian hemispheres and is related to the electromagnetic interaction between Io and the magnetosphere. These spots are followed by ... [more ▼]

The Io footprint (IFP) consists of one or several spots observed in both jovian hemispheres and is related to the electromagnetic interaction between Io and the magnetosphere. These spots are followed by an auroral curtain, called the tail, extending more than 90° longitude in the direction of planetary rotation. We use recent Hubble Space Telescope images of Jupiter to analyze the location of the footprint spots and tail as a function of Io's location in the jovian magnetic field. We present here a new IFP reference contour---the locus of all possible IFP positions---with an unprecedented accuracy, especially in previously poorly covered sectors. We also demonstrate that the lead angle - the longitudinal shift between Io and the actual IFP position - is not a reliable quantity for validation of the interaction models. Instead, the evolution of the inter-spot distances appears to be a better diagnosis of the Io-Jupiter interaction. Moreover, we present observations of the tail vertical profiles as seen above the limb. The emission peak altitude is ~900 km and remains relatively constant with the distance from the main spot. The altitudinal extent of the vertical emission profiles is not compatible with precipitation of a mono-energetic electron population. The best fit is obtained for a kappa distribution with a characteristic energy of ~70 eV and a spectral index of 2.3. The broadness of the inferred electron energy spectrum gives insight into the physics of the electron acceleration mechanism at play above the IFP tail. [less ▲]

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See detailIo's interaction with Jupiter's magnetosphere
Dols, Vincent ULg

Doctoral thesis (2011)

Io, the innermost Galilean moon of Jupiter, is the most volcanic body of the solar system. This volcanism is responsible for a tenuous atmosphere composed mainly of S, O and SO2. This atmosphere is ... [more ▼]

Io, the innermost Galilean moon of Jupiter, is the most volcanic body of the solar system. This volcanism is responsible for a tenuous atmosphere composed mainly of S, O and SO2. This atmosphere is constantly bombarded by the plasma that co-rotates with the magnetic field of Jupiter, producing new ions and perturbing locally the magnetic field. This local perturbation is responsible for auroral emissions in the atmosphere of Jupiter, at the foot of Io’s flux tube. The spacecraft Galileo made five flybys of Io between 1995 and 2001 at very low altitude (~100’s km) and made plasma and magnetic field measurements that reveal the complexity of Io’s interaction with Jupiter. Past studies have tackled the modeling of this interaction using different complementary approaches, each shedding a new light on the issue but each involving some simplifications. The MHD models (Linker et al., 1998) are based on an a priori parameterization of the ionization in the atmosphere, generally assuming spherical symmetry and a single atmospheric and plasma species (representative of O and S). They ignore the important effect of the cooling of electrons as well as the multi-species composition of both the plasma and the atmosphere. The two-fluid approach (Saur et al., 1999) computes precisely the ionization and collisions in the atmosphere of Io but make the assumption of a constant magnetic field, limiting the self-consistency of the model and potentially introducing large quantitative errors. We combine a multi-species chemistry model of the interaction that includes atomic and molecular species with a self-consistent Hall-MHD calculation of the flow and magnetic perturbation to model as self-consistently as possible the plasma variables along the different flybys of Io by the Galileo probe. [less ▲]

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See detailIo's volcanism controls Jupiter's radio emissions
Yoneda, Mizuki; Tsuchiya, F.; Misawa, H. et al

in Geophysical Research Letters (2013)

Jupiter's sodium nebula showed an enhancement in late May through beginning of June, 2007. This means Io's volcanic activity and the magnetosphere's plasma content increased during this period. On the ... [more ▼]

Jupiter's sodium nebula showed an enhancement in late May through beginning of June, 2007. This means Io's volcanic activity and the magnetosphere's plasma content increased during this period. On the other hand, Jupiter's radio emission called HOM became quiet after the sodium nebula enhancement. The HOM emission is considered to be related to activity of aurorae on Jupiter. These observation results therefore suggest that the increase in plasma supply from Io into Jupiter's magnetosphere weakens its field aligned current, which generates the radio emissions and aurorae on Jupiter. By comparing our observation results to recent model and observation results we add supporting evidence to the possibility that Io's volcanism controls Jupiter's magnetospheric activity. [less ▲]

Detailed reference viewed: 51 (9 ULg)
Peer Reviewed
See detailIodide organification disorder in autonomous thyroid nodule.
Tang, B. N. T.; Corvilain, B.; Seret, Alain ULg et al

Poster (2005, November 15)

Detailed reference viewed: 17 (0 ULg)
Peer Reviewed
See detailIodide organification disorder in autonomous thyroid nodule.
Tang, B.; Corvilain, B.; Seret, Alain ULg et al

in European Journal of Nuclear Medicine and Molecular Imaging (2006), 33(S2), 351

Detailed reference viewed: 32 (1 ULg)