Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble
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– First fringes in the H band with the IOTA 3 telescopes interferometer by means of an integrated<br />
optics beam combiner (Monnier et al. 2004, Kraus et al. 2005) and first formal <strong>de</strong>monstration of<br />
single mo<strong>de</strong> guiding at 10 microns in the IODA project (Labadie et al. 2005).<br />
– Creation and <strong>de</strong>velopment of the Centre Jean-Marie Mariotti (JMMC) with partners (Nice, and<br />
ASHRA). Consecutive creation of the European interferometry Initiative (EII) coupling interferometry<br />
networks of the OPTICON EC I3, and high-level involvement (PI, PSci) in three of its four<br />
JRAs. The goal of JMMC is to <strong>de</strong>velop user-friendly software, and more generally preparation and<br />
advice, for the use and promotion of the VLTI. (See Appendix in chapter 20<br />
• Sherpa<br />
– Transport of cosmic rays in chaotic magnetic fields. The knowledge of the diffusion coefficients of<br />
cosmic rays is crucial for astrophysical applications and especially for astroparticle physics, both<br />
for mastering the cosmic ray propagation and the efficiency of Fermi acceleration. They have been<br />
computed with a Monte Carlo simulation as a function of the cosmic ray rigidity and the spectrum<br />
of the magnetic field (characterized by its in<strong>de</strong>x and its <strong>de</strong>gree of irregularities). It is found that<br />
the transverse diffusion coefficient follows a law which is nor Bohm nor quasi-linear, but a law that<br />
stems from the analysis of the spatial chaos of field lines. This result is important to estimate the<br />
confinement time of cosmic-rays in galaxies and in extragalactic jets (Casse et al. 2002).<br />
– Stationary accretion disks launching super-fast-magnetosonic waves. This is the last paper in the<br />
series on Magnetized Accretion-Ejection Structures (MAES), which represents the only available<br />
self-consistent mo<strong>de</strong>l of a self-confined jet driven by an accretion disk (with the disk fully resolved),<br />
able to cross all three MHD critical points. Biases induced by the self-similarity contraints are<br />
discussed (Ferreira & Casse 2004).<br />
– On the relevance of subcritical turbulence to accretion disk transport. This paper solves a riddle<br />
dating back to the seventies, and which has given rise to an important controversy in the last ten<br />
years. Namely, it is shown that a linearly stable, keplerian hydrodynamic flow is in<strong>de</strong>ed turbulent<br />
through non linear mechanisms, but that this turbulence has a low efficiency in terms of angular<br />
momentum transport, with a Shakura-Sunyaev parameter α < 10 −5 . The discrepancy between<br />
numerical simulations and laboratory experiments is explained away (Lesur & Longaretti 2005).<br />
– The bulk Lorentz factor crisis of TeV Blazars: evi<strong>de</strong>nce for an inhomogeneous pile-up energy distribution.<br />
It is shown that the theoretical Lorentz factors of Blazar jets are contradicted by the<br />
source statistics which implies Lorentz factors of or<strong>de</strong>r 3, whereas homogeneous mo<strong>de</strong>ls require 50 or<br />
more. The only way out of this conundrum is to take the jet stratification into account, so that high<br />
energy photons are not produced in the same region as low energy ones. Observations then require<br />
mono-energetic distribution functions whereas most mo<strong>de</strong>ls make use of power-law distributions. In<br />
contradistinction with the dominant view, this work shows that (1) jets do not need to be highly<br />
relativistic, and (2) turbulence rather than shocks is at the origin of the production of high energy<br />
particles (Henri & Saugé 2005).<br />
1.2 Bibliography<br />
A major innovation is the creation of an automated bibliography.<br />
Visit http://www-laog.obs.ujf-grenoble.fr/Laog/publications.php. The principle is that, once a list of<br />
names (LAOG personnel, evolving if necessary) is provi<strong>de</strong>d, an automated request is sent to ADS every week.<br />
Thus, new publications (including ArXiv preprints) are regularly ad<strong>de</strong>d to the bibliographical database. It is<br />
recognized that ADS does not cover all publications (for instance it does not access chemistry journals or some<br />
conferences), so that manual corrections and updates are still necessary, which is done un<strong>de</strong>r the responsibility of<br />
the LAOG authors. While this innovation (partly outsourced to a private software company) was implemented<br />
for the present Evaluation exercise, it is a long-term investment and an extremely useful tool that can be<br />
improved in the future (new names, new databases consulted, etc.).<br />
The major quantitative results emerging from the 2001-2005 report bibliography, available in a separate<br />
printed document are as follows: 2<br />
2 The bibliography to be used for the present report (covering the period 2001-2005) is however not exactly i<strong>de</strong>ntical to the web<br />
bibliography. In particular, care has been taken to weed out refereed papers of LAOG members before their arrival or after their<br />
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