Les sprites sont de gigantesques phénomènes lumineux qui sont produits entre 40 et 90 km d’altitude généralement par des éclairs nuage-sol positifs. Les sprites sont des phénomènes très brefs (durée de quelques millisecondes) qui appartiennent à la famille des TLEs (évènements lumineux transitoires) et qui sont composés de structures filamentaires nommées streamers. Les streamers sont des filaments de plasma, qui se propagent à des vitesses allant jusqu’à ∼10⁷ m/s et qui possèdent des champs électriques très forts souvent proches de 150 kV/cm (champs réduit à la pression atmosphérique). Lors de ce travail, on a développé un modèle fluide de plasma qui simule les décharges streamers couplées avec un modèle simulant les émissions optiques afin d’étudier la physique des streamers, des TLEs et plus particulièrement des sprites dans le cadre de la mission spatiale TARANIS. Cette mission a pour objectif d’étudier le système Atmosphère-Ionosphère-Magnétosphère, et observera les TLEs et leurs émissions associées: électromagnétiques, optiques, et probablement radiations énergétiques depuis le nadir. Dans cette thèse, on propose d’étudier certains problèmes liés aux streamers et aux sprites qui sont cruciaux pour préparer la mission TARANIS. Plus particulièrement nous abordons certains mécanismes de production de radiations énergétiques par les streamers récemment proposés dans la littérature et nous développons une méthode qui permet de déterminer l’altitude, la vitesse et le champ électrique des streamers des sprites, à partir d’une analyse spectroscopique de leurs émissions optiques. Nos résultats renforceront donc le retour scientifique des futures missions spatiales observant les TLE depuis le nadir et particulièrement TARANIS. / Sprites are large optical phenomena usually produced between 40 and 90 km altitude generally by positive cloud-to-ground lightning (+CG). These are short lifetime phenomena (duration of few milliseconds) that belong to the family of transient luminous events (TLEs) and composed of complex filamentary structures called streamers. Streamers are non-thermal plasma filament, highly collisional, propagating with velocities up to 10⁷ m/s, and characterized with high electric fields at their heads often close to 150 kV/cm when scaled to ground level air. In this work, we have developed a streamer plasma fluid model coupled with an optical emission model to investigate the physics of streamers and sprites in the framework of the TARANIS space mission. TARANIS will observe TLEs from a nadir-viewing geometry along with their related emissions (electromagnetic and particles). In this dissertation, we investigate some mechanisms of emission of energetic radiation from streamers recently proposed in the literature and we present an original spectroscopic method to determine sprite streamers altitudes, velocities, and electric fields through their optical emissions. This method is especially useful for increasing the scientific return of space missions that have adopted nadir-based observation strategies.

International Telemetering Conference Proceedings / October 23-26, 2000 / Town & Country Hotel and Conference Center, San Diego, California / This student paper was produced as part of the team design competition in the University of Arizona course ECE 485, Radiowaves and Telemetry. It presents a telemetering system proposed for UASat, a small satellite being designed for launch in the year 2004. The overall system architecture is described, including the transducers used by each subsystem, the command and telemetry packet formats, the antennas and modulation schemes, the link budget, and some hardware recommendations. A discussion of the data analysis is also included.

Sprites, halos, and elves are members of a family of short-lived, luminous phenomena known as Transient Luminous Events (TLEs), which occur in the middle atmosphere. Sprites are vertical glows occurring at altitudes typically ranging from ~40 to 90 km. In video imagery they exhibit a red color at their top, with blue tendril-like structure at low altitudes. Elves are disk-like glows that occur at the base of the ionosphere, with diameters of ~100-300 km, and have very short lifetimes (~2-3 ms). Halos are diffuse glows that occur at low altitudes, have diameters <100 km, and have a duration that may last up to 10s of ms. A majority of the studies of TLEs have taken place over the Midwestern U.S. where they were first discovered. This area produces large thunderstorms, which in turn generate large lightning discharges that have been associated with the formation of TLEs. Studies have used the low frequency radiation that initiates with these strokes to study characteristics of these events. This low frequency radiation has been used to determine where large numbers of TLEs may occur. Extreme southern Brazil is a region of the globe believed to have many TLEs, but few studies on these phenomena. Two collaborative campaigns involving Utah State University proceeded in 2002-2003, and in 2006. Multiple TLE images were made, proving this is, indeed, a region of the globe where these types of events are prominent. In particular, one storm in February 2003 produced over 440 TLEs imaged by USU video cameras. Of these events, over 100 of them had associated halos. Statistical studies for halos previously had been performed in the U.S., but never abroad. Also, several events from the February storm have been associated with negative cloud to ground lightning, a surprising occurrence, as to date, less than a handful of such events have ever been witnessed or published. In analyzing the TLEs from this campaign, we have shown the halos are similar to those seen in the U.S., even though the storms may be somewhat different. Also, detailed analyses of the negative events show both temporal and spatial morphology heretofore never reported on.

As a part of the European research program CAL, sprite observations were carried out from the OMP observatory in the French Pyrenees during the summer 2003. Images of the sprites were taken by two remotely controlled CCD cameras. The 23 July was considered particularly interesting because we then had access to data concerning both cloud-to-ground and intracloud lightning activity. This day was therefore chosen as the object of the present study. A large thunderstorm with two convective cores, one to the north and the other to the south, developed over the South of France during the late afternoon, and about two hours after sunset, the first sprite was detected. During a little more than three hours, 13 sprites were observed, 7 over the northern system and 6 over the southern system. The images enabled us to determine the azimuth angle of each sprite from the OMP observatory. 12 of the 13 sprites could be associated to positive cloud-to-ground flashes, and by putting together the sprite directions and the locations of the associated flashes on the radar images, we managed to get a rough idea of the position of the sprites in the storm system, and also to estimate their vertical and horizontal extent. Satellite images were included at this point of the study, and it appeared clear that sprites tend to occur over the stratiform region of the storm system in the area with the coldest (highest) cloud tops. The associated positive flashes were also within or close to this portion of the storm. The sprite occurrences were studied in relation to the cloud-to-ground and to the intracloud activity. We found that sprites seem to occur in a late stage of each storm system, when the rate of negative cloud-to-ground flashes has considerably decreased, and when the ratio of positive cloud-to-ground flashes is much higher then during the most active phase of the storm. Globally, the intracloud activity is also low during the sprite-producing periods, but sudden "bursts" of intracloud lightning could frequently be observed at the moment of the sprite. The peak current of the positive flashes was found to be rather weakly correlated to their sprite-generating capacity. The available Schumann resonance measurements seem to indicate that the charge moment is a much more adequate parameter in this respect. The areal coverage of the radar echo was calculated. The result supports the idea that sprite events tend to appear almost exclusively over large thunderstorm systems.

Encore jamais été observé, le rayonnement infrarouge moyen et lointain consécutif aux sprites a été prédit et serait lié à l’excitation des états vibrationnels de CO2. En sciences de l’atmosphère, la composition chimique peut être retrouvée par des méthodes de télédétection infrarouge. Pour la Défense, les émissions infrarouges naturelles peuvent causer de fausses alarmes à travers les systèmes de veille optronique satellitaires ou aéroportés. C’est pourquoi il est nécessaire de caractériser les émissions infrarouges des sprites. Pour cela, un modèle de cinétique plasma-vibrationnelle a été développé et couplé à un modèle de transfert radiatif atmosphérique. Celui-ci permet de simuler les effets énergétiques et chimiques consécutifs à la perturbation électrique des streamers, éléments constitutifs des sprites. Les signatures infrarouges évaluées devraient être détectables pour un observateur situé dans la stratosphère ou dans l’espace. Par ailleurs, les effets des incertitudes sur les principaux paramètres du modèle ont été quantifiés à travers une étude de sensibilité. Enfin, ces travaux ont permis de définir certaines spécifications instrumentales pour la mission HALESIS (High Altitude Luminous Events Studied by Infrared Spectro-imagery), qui aura pour but d’observer les sprites et autres phénomènes lumineux de moyenne atmosphère dans l’infrarouge. / Even if it hasn’t been observed yet, the existence of emissions in the middle and far infrared following a sprite is suspected and could be related to vibrational excitation of CO2. In atmospheric sciences, the chemical composition can be retrieved through different remote sensing methods. For the Defense, natural infrared emissions could cause false alarms through airborne and spaceborne optronic detection systems. That is why it is necessary to characterize the infrared emissions of sprites. To do so, a plasma-vibrational kinetic model has been developed and coupled to an atmospheric radiative transfer model. This model allows evaluating the energetic and chemical effects following the electrical perturbation caused by the propagation of streamers, main constituent elements of sprites. The evaluated signatures could be detectable for an observer situated in the stratosphere or in space. Otherwise, the effects of the uncertainties on the principal parameters of the model have been quantified through a sensitivity analysis. Finally, this work allowed defining instrumental specifications for the future mission HALESIS (High Altitude Luminous Events Studied by Infrared Spectro-imagery), which will record hyperspectral infrared images of sprites and other middle atmosphere luminous events.