References of "2005"
     in
Bookmark and Share    
Full Text
See detailFamilial basilar migraine associated with a new mutation in the ATP1A2 gene
Ambrosini, A.; D'Onofrio, M.; Grieco, G. S. et al

in Neurology (2005), 65(11), 1826-1828

Basilar migraine (BM), familial hemiplegic migraine (FHM), and sporadic hemiplegic migraine (SHM) are phenotypically similar subtypes of migraine with aura, differentiated only by motor symptoms, which ... [more ▼]

Basilar migraine (BM), familial hemiplegic migraine (FHM), and sporadic hemiplegic migraine (SHM) are phenotypically similar subtypes of migraine with aura, differentiated only by motor symptoms, which are absent in BM. Mutations in CACNA1A and ATP1A2 have been found in FHM. The authors detected a novel mutation in the ATP1A2 gene (R548H) in members of a family with BM, suggesting that BM and FHM may be allelic disorders. [less ▲]

Detailed reference viewed: 17 (0 ULg)
See detailEuropa's FUV auroral tail observed on Jupiter
Grodent, Denis ULg

Conference (2005, December 12)

Detailed reference viewed: 2 (0 ULg)
See detailInterview à Radio Nostalgie sur les négociations de l'OMC à Hong Kong
Burny, Philippe ULg

Diverse speeche and writing (2005)

Detailed reference viewed: 2 (0 ULg)
See detailAdmittance spectroscopy of OLEDs
Nguyen, Ngoc Duy ULg; Schmeits, Marcel

Scientific conference (2005, December 12)

Detailed reference viewed: 35 (1 ULg)
See detailSupply chain coordination through contract negotiation
Arda, Yasemin ULg; Hennet, Jean-Claude

in DC-ECC 06, 44th IEEE Conference on Decision and Control and the European Control Conference, Seville, Spain, 12-15 December 2005 (2005, December 12)

The purpose of the paper is to evaluate the efficiency of different types of contracts between the industrial partners of a supply chain. Such an evaluation is made on the basis of the relationship ... [more ▼]

The purpose of the paper is to evaluate the efficiency of different types of contracts between the industrial partners of a supply chain. Such an evaluation is made on the basis of the relationship between a producer facing a random demand and a supplier with a random lead time. The model combines queuing theory for evaluation aspects and game theory for decisional purposes. [less ▲]

Detailed reference viewed: 7 (4 ULg)
See detailPrésentation générale du projet CSI
Halleux, Jean-Marie ULg; Teller, Jacques ULg

Conference given outside the academic context (2005)

Detailed reference viewed: 2 (0 ULg)
See detailPromoter-driven high expression of metal homeostasis genes in Arabidopsis halleri
Hanikenne, Marc ULg

Conference (2005, December 08)

Detailed reference viewed: 5 (1 ULg)
See detailRecherches doctorales : méthodologie et résultats
Delfosse, Annick ULg

Scientific conference (2005, December 07)

Detailed reference viewed: 10 (3 ULg)
See detailQualité des travaux de fin d'études
Bruyère, Olivier ULg

Conference (2005, December 06)

Detailed reference viewed: 1 (1 ULg)
Full Text
See detailContribution to an adapted physiotherapy in the hyperlaxity syndromes
Kaux, Jean-François ULg; Foidart-Dessalle, Marguerite ULg; Toussaint, Geoffrey ULg et al

in First Annual Congress (of the new style) of the Royal Belgian Society of Physical and Rehabilitation Medicine (RBSPRM) (2005, December 02)

Detailed reference viewed: 64 (30 ULg)
See detailL’apprentissage du français par les enfants issus de l’immigration
Lucchini, Silvia ULg

Conference given outside the academic context (2005)

Detailed reference viewed: 4 (1 ULg)
See detailL’apprentissage du français par les enfants issus de l’immigration
Lucchini, Silvia ULg

Conference given outside the academic context (2005)

Detailed reference viewed: 5 (2 ULg)
See detailThe life of stars and their planets
Catala, C.; Aerts, C.; Aigrain, S. et al

in Favata, F.; Sanz-Forcada, J.; Giménez, A. (Eds.) et al 39TH ESLAB Symposium on Trends in Space Science and Cosmic Vision 2020 (2005, December 01)

We lack a reliable scenario for the formation and evolution of stars and their planetary systems, involving key factors such as magnetic fields and turbulence. We present the case for a mission concept ... [more ▼]

We lack a reliable scenario for the formation and evolution of stars and their planetary systems, involving key factors such as magnetic fields and turbulence. We present the case for a mission concept that will clarify these problems and give us a global view of the evolution of combined star and planetary systems. This will be achieved by simultaneously addressing the search for planetary transits in front of a large number of stars, including many nearby stars, the study of their internal structure and evolution via asteroseismology, and that of their magnetic activity, via UV monitoring. [less ▲]

Detailed reference viewed: 4 (0 ULg)
See detailOpen Flux Estimates and Reconnection Rates in Saturn's Magnetosphere, Derived Using HST and Cassini Data
Badman, S. V.; Bunce, E. J.; Clarke, J. T. et al

Conference (2005, December 01)

During January 2004, a sequence of 68 UV images of Saturn's southern aurora was obtained by the Hubble Space Telescope (HST), coordinated with measurements of the upstream interplanetary conditions made ... [more ▼]

During January 2004, a sequence of 68 UV images of Saturn's southern aurora was obtained by the Hubble Space Telescope (HST), coordinated with measurements of the upstream interplanetary conditions made by the Cassini spacecraft. Using the poleward edge of the observed aurora as a proxy for the open-closed field line boundary, the open flux content of the southern polar region has been estimated. It is found to range from 15 to 50 GWb during the interval, such a large variation providing evidence of a significant magnetospheric interaction with the solar wind, in particular with structures associated with corotating interaction regions (CIRs). Cassini measurements of the upstream interplanetary conditions have been used to estimate the rate of open flux production at the magnetopause. By comparison with the open flux values obtained from the images, the rate of open flux closure in Saturn's magnetotail is also estimated. We find that the rate of open flux production is high (200 kV) in the high-field strength intervals following the onset of CIR-related compressions, and elevated (30-40 kV) in an intermediate-field strength rarefaction region. High flux closure rates (100-200 kV) are estimated in association with the onset of solar wind compressions and are intermittently increased (30-60 kV) during a weak-field rarefaction region. The disturbed auroral forms seen in the images are discussed in relation to the estimated reconnection rates. Recent studies have suggested that Saturn Kilometric Radiation emissions are also disturbed by the onset of CIR compressions at Saturn. [less ▲]

Detailed reference viewed: 23 (3 ULg)