Hybrid time dependent/independent solution for the He i line ratio temperature and density diagnostic for a thermal helium beam with applications in the scrape-off layer-edge regions in tokamaks

Spectroscopic studies of line emission intensities and ratios offer an attractive option in the\r\ndevelopment of non-invasive plasma diagnostics. Evaluating ratios of selected He I line\r\nemission profiles from the singlet and triplet neutral helium spin systems allows for simultaneous\r\nmeasurement of electron density (ne) and temperature (Te) profiles. Typically, this powerful\r\ndiagnostic tool is limited by the relatively long relaxation times of the 3S metastable term of helium\r\nthat populates the triplet spin system, and on which electron temperature sensitive lines are based.\r\nBy developing a time dependent analytical solution, we model the time evolution of the two spin\r\nsystems. We present a hybrid time dependent/independent line ratio solution that improves the\r\nrange of application of this diagnostic technique in the scrape-off layer (SOL) and edge plasma\r\nregions when comparing it against the current equilibrium line ratio helium model used at\r\nTEXTOR.

Dielectronic recombination of W20 + (4d104f8): Addressing the half-open f shell

A recent measurement of the dielectronic recombination (DR) of W20+ [Schippers et al., Phys.Rev.A 83, 012711 (2011)] found an exceptionally large contribution from near-threshold resonances (1 eV). This still affected the Maxwellian rate coefficient at much higher temperatures. The experimental result was found to be higher by a factor of 4 or more than that currently in use in the 100- to 300-eV range, which is of relevance for modeling magnetic fusion plasmas. We have carried out DR calculations with AUTOSTRUCTURE which include all significant single-electron promotions. Our intermediate-coupling (IC) results are more than a factor of 4 larger than our LS-coupling ones at 1 eV but still lie a factor of 3 below experiment here. If we assume complete (chaotic)mixing of near-threshold autoionizing states, then our results come into agreement (to within 20%)with experiment below 2 eV. Our total IC Maxwellian rate coefficients are 50%–30% smaller than those based on experiment over 100–300 eV.

Electron-impact ionization of B+

Electron-impact ionization cross sections are calculated for the ground and metastable states of B+. Com- parisons between perturbative distorted-wave and nonperturbative close-coupling calculations find reductions in the direct ionization cross sections due to long-range electron correlation effects of approximately 10% for the ground state and approximately 15% for the metastable state. Previous crossed-beams experiments, with a metastable to ground ratio of between 50% and 90%, are found to be in reasonable agreement with metastable state close-coupling results. New crossed-beams experiments, with a metastable to ground ratio of only 9%, are found to be in reasonable agreement with ground state close-coupling results. Combined with previous work on neutral B and B2+, the nonperturbative close-coupling calculations provide accurate ionization cross sections for the study of edge plasmas in controlled fusion research.

Electron-impact excitation of Xe 26+ and its resultant spectral signature

We have carried out a 129 close-coupling level Dirac-Coulomb R-matrix calculation for the electron-impact excitation of Ni-like Xe. We have utilized this data to generate the spectral signature of Xe26+ in terms of feature photon-emissivity coefficients (F-PεCs). We have compared these F-PεCs with those generated using semi-relativistic plane-wave Born excitation data, which forms the heavy species baseline for the Atomic Data and Analysis Structure (ADAS), We find that the Born-based F-PεCs give a reasonable qualitative description of the spectral signature but that, quantitatively, the R-matrix-based F-PεCs differ by up to a factor of 2. The spectral signature of heavy species is key to diagnosing hot plasmas such as will be found in the International Thermonuclear Experimental Reactor.

Electron-impact excitation of open d-shell ions

Astrophysics is driven by observations, and in the present era there are a wealth of state-of-the-art ground-based and satellite facilities. The astrophysical spectra emerging from these are of exceptional quality and quantity and cover a broad wavelength range. To meaningfully interpret these spectra, astronomers employ highly complex modelling codes to simulate the astrophysical observations. Important input to these codes include atomic data such as excitation rates, photoionization cross sections, oscillator strengths, transition probabilities and energy levels/line wavelengths. Due to the relatively low temperatures associated with many astrophysical plasmas, the accurate determination of electron-impact excitation rates in the low energy region is essential in generating a reliable spectral synthesis. Hence it is these atomic data, and the main computational methods used to evaluate them, which we focus on in this publication. We consider in particular the complicated open d- shell structures of the Fe-peak ions in low ionization stages. While some of these data can be obtained experimentally, they are usually of insufficient accuracy or limited to a small number of transitions.

Effective collision strengths for election impact excitation of Cl III

Effective collision strengths for electron-impact excitation of the phosphorus-like ion Cl III are presented for all fine-structure transitions among the levels arising from the lowest 23 LS states. The collisional cross sections are computed in the multichannel close-coupling R-matrix approximation, where sophisticated configuration-interaction wave functions are used to represent the target states. The 23 LS states are formed from the basis configurations 3s²3p³, 3s3p⁴, 3s²3p²3d, and 3s²3p²4s, and correspond to 49 fine-structure levels, leading to a total possible 1176 fine-structure transitions. The effective collision strengths, obtained by averaging the electron collision strengths over a Maxwellian distribution of electron velocities, are tabulated in this paper for all 1176 transitions and for electron temperatures in the ranges T(K)=7500-25,000 and log T(K)=4.4-5.4. The former range encompasses the temperatures of particular importance for application to gaseous nebulae, while the latter range is more applicable to the study of solar and laboratory-type plasmas. © 2001 Academic Press.

Laser Driven Nuclear Physics at ELI–NP

High power lasers have proven being capable to produce high energy γ-rays, charged particles and neutrons, and to induce all kinds of nuclear reactions. At ELI, the studies with high power lasers will enter for the first time into new domains of power and intensities: 10 PW and 10^23 W/cm^2. While the development of laser based radiation sources is the main focus at the ELI-Beamlines pillar of ELI, at ELI-NP the studies that will benefit from High Power Laser System pulses will focus on Laser Driven Nuclear Physics (this TDR, acronym LDNP, associated to the E1 experimental area), High Field Physics and QED (associated to the E6 area) and fundamental research opened by the unique combination of the two 10 PW laser pulses with a gamma beam provided by the Gamma Beam System (associated to E7 area). The scientific case of the LDNP TDR encompasses studies of laser induced nuclear reactions, aiming for a better understanding of nuclear properties, of nuclear reaction rates in laser-plasmas, as well as on the development of radiation source characterization methods based on nuclear techniques. As an example of proposed studies: the promise of achieving solid-state density bunches of (very) heavy ions accelerated to about 10 MeV/nucleon through the RPA mechanism will be exploited to produce highly astrophysical relevant neutron rich nuclei around the N~126 waiting point, using the sequential fission-fusion scheme, complementary to any other existing or planned method of producing radioactive nuclei.

The studies will be implemented predominantly in the E1 area of ELI-NP. However, many of them can be, in a first stage, performed in the E5 and/or E4 areas, where higher repetition laser pulses are available, while the harsh X-ray and electromagnetic pulse (EMP) environments are less damaging compared to E1.

A number of options are discussed through the document, having an important impact on the budget and needed resources. Depending on the TDR review and subsequent project decisions, they may be taken into account for space reservation, while their detailed design and implementation will be postponed.

The present TDR is the result of contributions from several institutions engaged in nuclear physics and high power laser research. A significant part of the proposed equipment can be designed, and afterwards can be built, only in close collaboration with (or subcontracting to) some of these institutions. A Memorandum of Understanding (MOU) is currently under preparation with each of these key partners as well as with others that are interested to participate in the design or in the future experimental program.

Distribuição por tamanhos do aerosol atmosférico na Península Ibérica

Um dos principais fatores que afetam negativamente a qualidade do ambiente em muitas cidades em todo o mundo é o material particulado (PM). A sua presença na atmosfera pode ter impactos negativos na saúde humana, clima, património edificado e ecossistemas. Muitos dos estudos realizados em áreas urbanas focam apenas as frações respiráveis (PM10 e PM2,5). No entanto, os processos de formação, a identificação das fontes emissoras e os efeitos dependem muito da distribuição granulométrica das partículas. A atenção tem recaído na análise de hidrocarbonetos poliaromáticos (PAHs), devida à sua carcinogenicidade e a informação disponível sobre outros compostos é escassa. O presente estudo consistiu na obtenção do PM distribuído por diferentes frações de tamanho e na análise detalhada da sua composição química, em dois locais urbanos da Península Ibérica (Madrid e Lisboa). Dado que os veículos representam uma das principais fontes emissoras em ambientes urbanos, efetuou-se uma caracterização mais detalhada deste tipo de emissões, conduzindo uma campanha de amostragem num túnel rodoviário (Marquês de Pombal, Lisboa). As amostragens, em ambas as cidades, decorreram durante um mês, quer no verão quer no inverno, em dois locais urbanos distintos, um junto a uma via com influência de tráfego e outro numa área urbana de fundo. No túnel a amostragem foi realizada apenas durante uma semana. Em Madrid e no túnel, o PM foi recolhido utilizando um amostrador de elevado volume com impactor em cascata com quatro tamanhos: 10-2,5, 2,5-0,95, 0,95-0,49 e < 0,49 μm. Em Lisboa, foi utilizado um impactor em cascata com apenas dois tamanhos, 10- 2,5 e < 2,5 μm. As amostras foram quimicamente analisadas e determinadas as concentrações de compostos carbonados (OC, EC e carbonatos), iões inorgânicos solúveis em água (Cl−, NO3−, SO42−, Na+, NH4+, K+, Mg2+, Ca2+),metais e compostos orgânicos. Em Madrid, as concentrações médias de PM10 foram 44 e 48% maiores nas amostras recolhidas junto à estrada do que as de fundo urbano no verão e inverno, respetivamente. A fração grosseira e o PM0,5 apresentaram concentrações mais elevadas no verão do que no inverno devido às condições climatéricas pouco usuais. No verão, as amostragens decorreram num mês em que as temperaturas foram muito elevadas e em que ocorreram vários episódios de intrusão de poeira africana. Durante o período de amostragem de inverno, as temperaturas foram muito baixas e registaram-se vários dias de precipitação quer sob a forma de chuva, quer sob a forma de neve. As situações meteorológicas sinóticas mais comuns, incluindo aquelas que causam o transporte de massas de ar com poeiras Africanas, foram identificadas em ambas as estações do ano. As concentrações mássicas de PM10, EC e OC foram encontrados predominantemente na fração de tamanho ultrafino em ambos os locais de amostragem e estações do ano. Nas restantes frações não se observou nenhuma tendência sazonal. O carbono orgânico secundário (SOC) mostrou um claro padrão sazonal, com concentrações muito mais elevadas no verão do que no inverno, em ambos os lugares. A partir do balanço mássico de iões, observou-se que, no verão, a formação de compostos inorgânicos secundários (SIC) conduziu a um enriquecimento pouco comum de Ca2+ na fração submicrométrica, quer nas amostras de tráfego, quer em fundo urbano. Os alcanos, PAHs, os álcoois e os ácidos foram as classes de compostos orgânicos identificados e quantificados no material particulado. Globalmente, representaram 0,26 e 0,11 μg m−3 no verão e inverno, respetivamente, no local de tráfego e 0,28 e 0,035 μg m−3 na área urbana de fundo. Os diferentes compostos orgânicos também apresentaram padrões sazonais, sugerindo fontes de emissão (e.g. escapes dos veículos e fontes biogénicas) ou processos de formação com contribuições variáveis ao longo do ano. As concentrações de benzoapireno equivalente foram menores que 1 ng m-3 e o risco carcinogénico estimado é baixo. No verão, os maiores enriquecimentos de metais ocorreram na fração submicrométrica, e no inverno na fração grosseira. No verão, os enriquecimentos foram ≥ 80% para o Mn, Ni, Cu, Zn, Cd, Sb e Co, no inverno, estes traçadores de emissões do tráfego foram menores, exceto para o Zn. Em Lisboa, a concentração média de PM10 foi de 48 μg m-3 no verão e de 44 μg m-3 no inverno, junto à estrada. Na área de fundo urbano, registaram-se níveis comparáveis nas duas estações (27 μg m-3 e 26 μg m-3). A média do rácio PM2,5/PM10 foi de 65% no verão e 44% no inverno na área de tráfego e 62% e 59% na área urbana de fundo. Estes resultados significam que o PM2,5 é um dos principais contaminantes que afetam a qualidade do ar no centro da cidade de Lisboa. A relação OC/EC, que reflete a composição das emissões de combustão dos veículos, variou entre 0,3 e 0,4 no interior do túnel. Os rácios de OC/EC mínimos obtidos junto às vias de tráfego em Madrid e em Lisboa encontram-se entre os do túnel e os registados em atmosferas urbanas de fundo, sugerindo que os valores mínimos habitualmente obtidos para este parâmetro em ambientes urbanos abertos sobrestimam as emissões diretas de OC pelo transporte rodoviário. Espera-se que os resultados deste trabalho contribuam para suprir, pelo menos em parte, as lacunas de informação quer sobre a composição de várias granulometrias de PM, quer sobre fontes e processos de formação em atmosferas urbanas. Como a exposição a poluentes do ar ultrapassa o controle dos indivíduos e exige ação das autoridades públicas a nível nacional, regional e até mesmo internacional, é importante propor medidas mitigadoras focadas nas principais fontes de emissão identificadas.

Analyse du profil d’expression de la protéine pro-apoptotique Dap-3 dans les vésicules extracellulaires produites dans le contexte de l’infection au VIH-1

L’immunopathogenèse de l’infection au VIH-1 est principalement causée par la déplétion des LT CD4 (lymphocytes T-CD4). Cette mort des LT CD4 dépend de plusieurs facteurs comme la lyse des LT CD4 infectés et la présence de vésicules extracellulaires et d’exosomes libérées par les cellules dendritiques et les LT CD4 infectés au VIH-1. L’analyse protéomique des exosomes issus des cellules dendritiques mises en culture avec le VIH-1 a révélé la présence de molécules pro-apoptotiques comme le Dap-3 (Death Associated Protein 3). Nous avons proposé comme hypothèse que le Dap-3 puisse être contenu dans d’autres types de vésicules extracellulaires et que le Dap-3 vésiculaire contribue à la déplétion des LT CD4. Après avoir optimisé l’immunobuvardage avec l’anti-Dap-3, nous avons déterminé la présence de Dap-3 dans les vésicules extracellulaires issues des cellules RAJI-CD4-DCIR infectées au VIH-1. L’utilisation de gradients de vélocité nous a permis d’observer la présence de Dap-3 dans les fractions du gradient contenant les exosomes issus des cellules RAJI-CD4-DCIR infectées, mais également dans d’autres fractions du gradient de vélocité encore non caractérisées. Chez les patients, nous avons montré une hétérogénéité des vésicules extracellulaires dans les fractions du gradient de vélocité issues des plasmas des patients VIH-1+. Ces résultats indiquent la présence de plusieurs populations de vésicules extracellulaires séparées par la méthode du gradient de vélocité. Enfin, la transfection des cellules RAJI-CD4-DCIR et des cellules dendritiques a été mise au point avec les ARN anti-sens de Dap-3 afin de produire éventuellement des vésicules Dap-3 négatives. Ce projet de recherche aura permis de valider les outils nécessaires à la poursuite de l’étude du rôle de Dap-3 dans la pathogenèse de l’infection au VIH-1.

Porta substratos para um sistema de pulverização catódica. Aplicação na obtenção de TiO2.

Dissertação apresentada na Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa para obtenção do Grau de Mestre em Engenharia Física

1969-70 Hockey Team

1969-71 Brock Generals Hockey team. Members from left to right - Back row: Tom Kearney (Trainer), Al Kellogg (Coach), John Hull, Craig Morrison, Gregg Law, Frank Mucci, Dale Andreas, Eric Stevens, Serge Girrard, John Clarey, Wayne Kenyon, Reg Egilsson, Dusty Papke, Randy Oiling (Manager). Front row: Ron Powel, Barry Hopkins, Bruce Wormald, Miller Hicks, Fred Carter, Mike Nicholson, Dick Overholt, Chris Shott. Missing: John O'Brien, Barry Elliot.

The effect of pH and ethanol on the astringent sub-qualities of red wine, and the implications for optimum grape maturity /

The first objective of this study was to identify appropriate sensory descriptors to assess the astringent sub-qualities of red wine. The influence of pH and ethanol on the sensation of astringency in red wine was evaluated, using a de-alcoholized red wine. A portion of the wine was adjusted to the pH values of 3.2, 3.4, 3.6 and 3.8, and another portion was adjusted to ethanol concentrations of 0%, 6%, 12%, and 15%. In addition, the pH 3.4 and 3.6 treatments were adjusted to an ethanol concentration of 12% and 15% all wines were then assessed sensorially and seventeen terms were identified, through panel discussion, to describe the mouth-feel and taste qualities: velvet, aggressive, silk/satin, dry, fleshy, unripe, pucker viscosity, abrasive, heat, chewy, acidity, grippy/adhesive, bitter, balance, overall astringency, and mouth-coat. Descriptive analysis profiling techniques were used to train the panel and measure the intensity of these attributes. It was found that decreasing pH values (averaged across all ethanol concentrations) showed an increase in the overall astringency of the wine. The combined treatments of ethanol and pH, real wine parameters (pH 3.4 and 3.6; 12% and 15% ethanol) did not have an effect on the perception of the astringent sub-qualities of the wine. A time intensity study was also included using the pH and ethanol adjusted wines, which showed that as the ethanol level of the wines increased so did the time to maximum intensity. The second objective was to identify appropriate sensory descriptors to evaluate the influence of grape maturity and maceration technique (grape skin contact) on the astringency sub-qualities of red vinifera wines from Niagara. The grapes were harvested across two dates, representing an early harvest and a late harvest. A portion of the Cabernet Sauvignon grapes wine was divided into three maceration treatments of oneweek maceration, standard two-week maceration, three-week maceration, and MCM. Another portion of both the early and late harvest Cabernet Sauvignon grapes were chaptalized to yield a final ethanol concentration of 14.5%. The wines were assessed sensorially and thirteen terms were identified, through panel discussion, to describe the mouth-feel and taste qualities: carbon dioxide, pucker, acidity, silk/chamois, dusty/chalky/powdery, sandpaper, numbing, grippy/adhesive, dry, mouthcoat, bitter, balance and, overall astringency. Descriptive analysis techniques were used to train the panel and measure the intensity of these attributes. The data revealed few significant differences in the mouth-feel of the wines with respect to maturity; which included differences in overall astringency and balance. There were varietal differences between Cabernet Sauvignon, Cabernet Franc, and Pinot Noir and differences for Cabernet Sauvignon wines due to the length and manner of maceration and as a result of chaptalization. Statistical analysis revealed a more complex mouth-feel for the Pinot Noir wines; and an increase in the intensity of the astringent sub-qualities as a result of the addition of sugar to the wines. These findings have implications for how processing decisions, such as optimum grape maturity and vinification methods may affect red wine quality.

Élaboration d’un simulateur de gravure par plasma de haute densité basé sur une approche cellulaire pour l’étude de profils dans divers matériaux

La réalisation de dispositifs à des dimensions sous-micrométriques et nanométriques demande une maîtrise parfaite des procédés de fabrication, notamment ceux de gravure. La réalisation des ces dispositifs est complexe et les exigences en termes de qualité et de géométrie des profils de gravure imposent de choisir les conditions opératoires les mieux adaptées. Les simulations de l'évolution spatio-temporelle des profils de gravure que nous proposons dans cette thèse s'inscrivent parfaitement dans ce contexte. Le simulateur que nous avons réalisé offre la possibilité de mieux comprendre les processus qui entrent en jeu lors de la gravure par plasma de profils dans divers matériaux. Il permet de tester l'influence des paramètres du plasma sur la forme du profil et donc de déterminer les conditions opératoires optimales. La mise au point de ce simulateur s'appuie sur les concepts fondamentaux qui gouvernent la gravure par plasma. À partir de l'état des lieux des différentes approches numériques pouvant être utilisées, nous avons élaboré un algorithme stable et adaptable permettant de mettre en évidence l'importance de certains paramètres clés pour la réalisation de profils de gravure par un plasma à haute densité et à basse pression. Les capacités de cet algorithme ont été testées en étudiant d'une part la pulvérisation de Si dans un plasma d'argon et d'autre part, la gravure chimique assistée par les ions de SiO2/Si dans un plasma de chlore. Grâce aux comparaisons entre profils simulés et expérimentaux, nous avons montré l'importance du choix de certains paramètres, comme la nature du gaz utilisé et la pression du plasma, la forme initiale du masque, la sélectivité masque/matériau, le rapport de flux neutre/ion, etc. Nous avons aussi lié ces paramètres à la formation de défauts dans les profils, par exemple celle de facettes sur le masque, de parois concaves, et de micro-tranchées. Enfin, nous avons montré que le phénomène de redépôt des atomes pulvérisés entre en compétition avec la charge électrique de surface pour expliquer la formation de profils en V dans le Pt pulvérisé par un plasma d'argon.

Étude des effets secondaires associés à un traitement prolongé de fluticasone inhalée chez les chevaux atteints de souffle (asthme équin)

Le souffle équin est une maladie inflammatoire chronique des petites voies respiratoires, très fréquente chez les chevaux gardés à l’intérieur avec de la paille et du foin moisi et poussiéreux. Les signes cliniques peuvent être prévenus par le contrôle de l’environnement et soulagés par l’administration de corticostéroïdes systémiques et inhalés. L’objectif de cette étude était de déceler les effets secondaires présents sur des chevaux atteints de souffle traités à la fluticasone (Flovent 250 μg HFA®, 2000 μg BID, pendant six mois, et puis 2000 μg SID, pendant six autres mois) par le cortisol sérique et la présence d’ulcères gastriques. Cinq chevaux exempts de maladie respiratoire et onze chevaux atteints du souffle ont été gardés à l’intérieur d’une écurie avec du foin moisi et de la paille dans le but de provoquer la maladie chez le groupe atteints du souffle. Une fois les chevaux atteints de souffle devenus symptomatique, ils ont été divisés en deux groupes : un premier groupe traité avec de la fluticasone, nourri avec du foin et gardé sur une litière de paille, et un deuxième groupe non traité nourrie avec de la moulée et gardé sur une litière de ripe, pendant six mois. Par la suite, les deux groupes ont été mis au pâturage. Le cortisol a été mesuré par Immunoessai enzymatique par chimiluminescence (CEIA, Immunolite 1000, Siemmens®) les 12e et 10e jours avant et les 7e, 28e, 80e, 160e, 200e, 250e, 290e et 320e jours après le début du traitement afin de déterminer le degré de suppression du cortisol sérique. On a également fait une suivi de la présence d`ulcères gastriques à l`aide de vidéo endoscopique. La fluticasone inhalée deux fois par jour cause une diminution du cortisol sérique les 28e, 80e et 160e jours, mais elle n’entraîne pas d’effets sur le score des ulcères gastriques. Les pellets de luzerne causent quant à elles, une augmentation du score des ulcères gastrique chez les animaux exempts de maladie respiratoire.

Étude critique de la densité électronique et des températures (excitation et ionisation) d'un plasma d'aluminium induit par laser

La caractérisation de matériaux par spectroscopie optique d’émission d’un plasma induit par laser (LIPS) suscite un intérêt qui ne va que s’amplifiant, et dont les applications se multiplient. L’objectif de ce mémoire est de vérifier l’influence du choix des raies spectrales sur certaines mesures du plasma, soit la densité électronique et la température d’excitation des atomes neutres et ionisés une fois, ainsi que la température d’ionisation. Nos mesures sont intégrées spatialement et résolues temporellement, ce qui est typique des conditions opératoires du LIPS, et nous avons utilisé pour nos travaux des cibles binaires d’aluminium contenant des éléments à l’état de trace (Al-Fe et Al-Mg). Premièrement, nous avons mesuré la densité électronique à l’aide de l’élargissement Stark de raies de plusieurs espèces (Al II, Fe II, Mg II, Fe I, Mg I, Halpha). Nous avons observé que les densités absolues avaient un comportement temporel différent en fonction de l’espèce. Les raies ioniques donnent des densités électroniques systématiquement plus élevées (jusqu’à 50 % à 200 ns après l’allumage du plasma), et décroissent plus rapidement que les densités issues des raies neutres. Par ailleurs, les densités obtenues par les éléments traces Fe et Mg sont moindres que les densités obtenues par l’observation de la raie communément utilisée Al II à 281,618 nm. Nous avons parallèlement étudié la densité électronique déterminée à l’aide de la raie de l’hydrogène Halpha, et la densité électronique ainsi obtenue a un comportement temporel similaire à celle obtenue par la raie Al II à 281,618 nm. Les deux espèces partagent probablement la même distribution spatiale à l’intérieur du plasma. Finalement, nous avons mesuré la température d’excitation du fer (neutre et ionisé, à l’état de trace dans nos cibles), ainsi que la température d’ionisation, à l’aide de diagrammes de Boltzmann et de Saha-Boltzmann, respectivement. À l’instar de travaux antérieurs (Barthélémy et al., 2005), il nous est apparu que les différentes températures convergeaient vers une température unique (considérant nos incertitudes) après 2-3 microsecondes. Les différentes températures mesurées de 0 à 2 microsecondes ne se recoupent pas, ce qui pourrait s’expliquer soit par un écart à l’équilibre thermodynamique local, soit en considérant un plasma inhomogène où la distribution des éléments dans la plume n’est pas similaire d’un élément à l’autre, les espèces énergétiques se retrouvant au cœur du plasma, plus chaud, alors que les espèces de moindre énergie se retrouvant principalement en périphérie.