Thematische Bibliographien / Balloon observations

Auswahl der wissenschaftlichen Literatur zum Thema „Balloon observations“

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Veröffentlicht am 25. Mai 2024

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Zeitschriftenartikel zum Thema "Balloon observations"

1

Maruca, Bennett A., Raffaele Marino, David Sundkvist, Niharika H. Godbole, Stephane Constantin, Vincenzo Carbone und Herb Zimmerman. „Overview of and first observations from the TILDAE High-Altitude Balloon Mission“. Atmospheric Measurement Techniques 10, Nr. 4 (26.04.2017): 1595–607. http://dx.doi.org/10.5194/amt-10-1595-2017.

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Abstract. Though the presence of intermittent turbulence in the stratosphere has been well established, much remains unknown about it. In situ observations of this phenomenon, which have provided the greatest details of it, have mostly been achieved via sounding balloons (i.e., small balloons which burst at peak altitude) carrying constant-temperature hot-wire anemometers (CTAs). The Turbulence and Intermittency Long-Duration Atmospheric Experiment (TILDAE) was developed to test a new paradigm for stratospheric observations. Rather than flying on a sounding balloon, TILDAE was incorporated as an add-on experiment to the payload of a NASA long-duration balloon mission that launched in January 2016 from McMurdo Station, Antarctica. Furthermore, TILDAE's key instrument was a sonic anemometer, which (relative to a CTA) provides better-calibrated measurements of wind velocity and a more robust separation of velocity components. During the balloon's ascent, TILDAE's sonic anemometer provided atmospheric measurements up to an altitude of about 18 km, beyond which the ambient air pressure was too low for the instrument to function properly. Efforts are currently underway to scientifically analyze these observations of small-scale fluctuations in the troposphere, tropopause, and stratosphere and to develop strategies for increasing the maximum operating altitude of the sonic anemometer.
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2

Dorf, M., H. Bösch, A. Butz, C. Camy-Peyret, M. P. Chipperfield, A. Engel, F. Goutail et al. „Balloon-borne stratospheric BrO measurements: comparison with Envisat/SCIAMACHY BrO limb profiles“. Atmospheric Chemistry and Physics Discussions 5, Nr. 6 (19.12.2005): 13011–52. http://dx.doi.org/10.5194/acpd-5-13011-2005.

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Abstract. For the first time, results of all four existing stratospheric BrO profiling instruments, are presented and compared with reference to the SLIMCAT 3-dimensional chemical transport model (3-D CTM). Model calculations are used to infer a BrO profile validation set, measured by 3 different balloon sensors, for the new Envisat/SCIAMACHY (ENVIronment SATellite/SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY) satellite instrument. The balloon observations include (a) balloon-borne in situ resonance fluorescence detection of BrO, (b) balloon-borne solar occultation DOAS measurements (Differential Optical Absorption Spectroscopy) of BrO in the UV, and (c) BrO profiling from the solar occultation SAOZ (Systeme d'Analyse par Observation Zenithale) balloon instrument. Since stratospheric BrO is subject to considerable diurnal variation and none of the measurements are performed close enough in time and space for a direct comparison, all balloon observations are considered with reference to outputs from the 3-D CTM. The referencing is performed by forward and backward air mass trajectory calculations to match the balloon with the satellite observations. The diurnal variation of BrO is considered by 1-D photochemical model calculation along the trajectories. The 1-D photochemical model is initialised with output data of the 3-D model with additional constraints on the vertical transport, the total amount and photochemistry of stratospheric bromine as given by the various balloon observations. Total [Bry]=(20.1±2.8)pptv obtained from DOAS BrO observations at mid-latitudes in 2003, serves as an upper limit of the comparison. Most of the balloon observations agree with the photochemical model predictions within their given error estimates. First retrieval exercises of BrO limb profiling from the SCIAMACHY satellite instrument agree to <±50% with the photochemically-corrected balloon observations, and tend to show less agreement below 20 km.
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Dorf, M., H. Bösch, A. Butz, C. Camy-Peyret, M. P. Chipperfield, A. Engel, F. Goutail et al. „Balloon-borne stratospheric BrO measurements: comparison with Envisat/SCIAMACHY BrO limb profiles“. Atmospheric Chemistry and Physics 6, Nr. 9 (29.06.2006): 2483–501. http://dx.doi.org/10.5194/acp-6-2483-2006.

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Abstract. For the first time, results of four stratospheric BrO profiling instruments, are presented and compared with reference to the SLIMCAT 3-dimensional chemical transport model (3-D CTM). Model calculations are used to infer a BrO profile validation set, measured by 3 different balloon sensors, for the new Envisat/SCIAMACHY (ENVIronment SATellite/SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY) satellite instrument. The balloon observations include (a) balloon-borne in situ resonance fluorescence detection of BrO (Triple), (b) balloon-borne solar occultation DOAS measurements (Differential Optical Absorption Spectroscopy) of BrO in the UV, and (c) BrO profiling from the solar occultation SAOZ (Systeme d'Analyse par Observation Zenithale) balloon instrument. Since stratospheric BrO is subject to considerable diurnal variation and none of the measurements are performed close enough in time and space for a direct comparison, all balloon observations are considered with reference to outputs from the 3-D CTM. The referencing is performed by forward and backward air mass trajectory calculations to match the balloon with the satellite observations. The diurnal variation of BrO is considered by 1-D photochemical model calculation along the trajectories. The 1-D photochemical model is initialised with output data of the 3-D model with additional constraints on the vertical transport, the total amount and photochemistry of stratospheric bromine as given by the various balloon observations. Total [Bry]=(20.1±2.5) pptv obtained from DOAS BrO observations at mid-latitudes in 2003, serves as an upper limit of the comparison. Most of the balloon observations agree with the photochemical model predictions within their given error estimates. First retrieval exercises of BrO limb profiling from the SCIAMACHY satellite instrument on average agree to around 20% with the photochemically-corrected balloon observations of the remote sensing instruments (SAOZ and DOAS). An exception is the in situ Triple profile, in which the balloon and satellite data mostly does not agree within the given errors. In general, the satellite measurements show systematically higher values below 25 km than the balloon data and a change in profile shape above about 25 km.
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Davenhall, Clive. „Dr Katterfelto and the Prehistory of Astronomical Ballooning1“. Culture and Cosmos 18, Nr. 1 (Juni 2014): 45–53. http://dx.doi.org/10.46472/cc.0118.0209.

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Regular telescopic astronomical observations made from balloons began after World War II, though scientific, particularly meteorological, ballooning dates from the mid-nineteenth century. However, astronomical ballooning has a curious prehistory at the dawn of lighter-than-air travel in the 1780s. The self-styled Dr Katterfelto (c.1743?-99) was a German-born travelling showman, lecturer and considerable self-publicist who in 1784-85 claimed to have made important astronomical discoveries from observations made from a balloon. It is unlikely that he made any such observations, or, indeed, any balloon flights. However, the episode throws some light on the world of the itinerant, eighteenth-century astronomical lecturer and the diffusion of contemporary astronomical and scientific knowledge.
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Choi, Yonghan, Jong-Chul Ha und Gyu-Ho Lim. „Investigation of the Effects of Considering Balloon Drift Information on Radiosonde Data Assimilation Using the Four-Dimensional Variational Method“. Weather and Forecasting 30, Nr. 3 (01.06.2015): 809–26. http://dx.doi.org/10.1175/waf-d-14-00161.1.

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Abstract Effects of balloon drift information (i.e., position and elapsed ascent time of the balloon) on the assimilation of radiosonde observations are investigated by using the Weather Research and Forecasting (WRF) Model and its data assimilation (WRFDA) system. Special radiosonde observations over the Korean Peninsula, which include the exact position and elapsed time of the balloon, are used instead of estimating the balloon drift information. To consider the balloon drift information appropriately, the four-dimensional variational data assimilation (4DVAR) and a high horizontal resolution (6 km) are used. Cycling experiments over the observation period from 20 June to 4 July 2013 are carried out to obtain the statistical robustness of the effects of considering the balloon drift information, and a single-case experiment is also conducted to show further details about the effects. The verification results of cycling experiments, such as root-mean-square errors (RMSEs) for meteorological-variable forecasts verified against the radiosonde observations and threat and bias scores for rainfall forecasts, show the positive impacts of considering the balloon drift information. Results of the single-case experiment also reveal that the simulated rainfall distribution, time series of hourly rainfall, and quantitative precipitation forecast (QPF) skills are improved through the assimilation of radiosonde observations while considering the balloon drift information. Additionally, forecasts of meteorological variables such as horizontal wind components, temperature, and dewpoint temperature are also improved by considering the balloon drift information in the single-case experiment.
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Fishman, G. J. „GAMMA-RAY BURSTS: A PERSONAL VIEW“. Revista Mexicana de Astronomía y Astrofísica Serie de Conferencias 53 (01.09.2021): 100–107. http://dx.doi.org/10.22201/ia.14052059p.2021.53.21.

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The first observations in gamma-ray astronomy were made in the late 1960's, primarily by balloon-borne observations. In the early 1970's, gamma-ray bursts were discovered, completely by accident, by satellites looking for man-made nuclear explosions in space. The celestial nature of these events were soon confirmed by other satellites. The first large detector system designed for cosmic gamma-ray bursts observations was the BATSE instrument on the Compton Gamma-Ray Observatory. Some of the details of the instrumentation onboard ballons and satellites and the gamma-ray bursts observational properties they determined are presented.
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MANI, ANNA, K. R. SIVARAMAN und S. P. VENKITESHWARAN. „Evidence of turbulence in the stratosphere“. MAUSAM 10, Nr. 2 (27.11.2021): 179–84. http://dx.doi.org/10.54302/mausam.v10i2.4047.

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Arnold (1954) has observed considerable turbulence in the stratosphere on four different occasions at Belmar, New Jersey, while tracking balloons with a telescope and a radio direction finder. The turbulence was so severe that the radiosonde separated from the balloon, though it was suspended with a cord with a nominal breaking strength of about 70 lbs. During three observations in June 1950, the instrument separated from the balloon at heights ranging from 28 to 32 km, while in the observation in October it separated at 24 km. He has estimated that a descending current of about 11 m. sec-1 could provide the necessary conditions for a free fall of the sonde of about 10 ft which could break the line.
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Hertzog, Albert, Philippe Cocquerez, René Guilbon, Jean-Noël Valdivia, Stéphanie Venel, Claude Basdevant, Gillian Boccara et al. „Stratéole/Vorcore—Long-duration, Superpressure Balloons to Study the Antarctic Lower Stratosphere during the 2005 Winter“. Journal of Atmospheric and Oceanic Technology 24, Nr. 12 (01.12.2007): 2048–61. http://dx.doi.org/10.1175/2007jtecha948.1.

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Abstract In September and October 2005, the Stratéole/Vorcore campaign flew 27 superpressure balloons from McMurdo, Antarctica, into the stratospheric polar vortex. Long-duration flights were successfully achieved, 16 of those flights lasting for more than 2 months. Most flights were terminated because they flew out of the authorized flight domain or because of energy shortage in the gondola. The atmospheric pressure (1-Pa precision) was measured every minute during the flights, whereas air temperature observations (0.25-K accuracy) and balloon positions (absolute GPS observations, 10-m accuracy) were obtained every 15 min. Fifteen-minute-averaged horizontal velocities of the wind were deduced from the successive balloon positions with a corresponding accuracy ≲0.1 m s−1. The collected dataset (more than 150 000 independent observations) provides a thorough high-resolution sampling of the polar lower stratosphere in the Southern Hemisphere from its wintertime state up to the establishment of the summer circulation in December–January. Most of the balloons stayed inside the vortex until its final breakdown, although a few were ejected toward the midlatitudes in November during filamention events associated with an increase in planetary wave activity. The balloons behaved as quasi-Lagrangian tracers during the first part of the campaign (quiescent vortex) and after the vortex breakdown in early December. Large-amplitude mountain gravity waves were detected over the Antarctic Peninsula and caused one flight termination associated with the sudden burst in the balloon superpressure.
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Hay, D., G. Ryan, M. Somasundaram, V. Yip und L. Navaratne. „Laparoscopic management of a migrated intragastric balloon causing mechanical small bowel obstruction: a case report and review of the literature“. Annals of The Royal College of Surgeons of England 101, Nr. 8 (November 2019): e172-e177. http://dx.doi.org/10.1308/rcsann.2019.0104.

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Intragastric balloons have been used as an invasive non-surgical treatment for obesity for over 30 years. Within the last 37 years, we have found only 27 cases reported in the literature of intestinal obstruction caused by a migrated intragastric balloon. We report the laparoscopic management of such a case and make observations from similar case presentations published in the literature. A 26-year-old woman had an intragastric balloon placed endoscopically for weight control 13 months previously. She presented to the emergency department with a four-day history of intermittent abdominal cramps and vomiting. Contrast enhanced computed tomography confirmed the presence of the intragastric balloon within the small bowel. At laparoscopic retrieval, the deflated intragastric balloon was found impacted in the terminal ileum approximately 15 cm from the ileocaecal valve. The balloon was retrieved by enterotomy and primary closure of the ileum without event. The risk of balloon deflation and subsequent migration increases over time but several published cases demonstrate that this complication can occur within six months of insertion. The initial approach to the treatment of migrated intragastric balloons causing small bowel obstruction should be determined by the location of impaction, severity of obstruction and the available skill set of the attending radiologist, endoscopist and/or surgeon. Balloons causing obstruction in the duodenum are likely amenable to endoscopic retrieval whereas impaction within the jejunum or ileum could be managed by percutaneous needle aspiration (in selected cases), endoscopy (double-balloon enteroscopy), laparoscopy or open surgery.
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Friedrich, Leon S., Adrian J. McDonald, Gregory E. Bodeker, Kathy E. Cooper, Jared Lewis und Alexander J. Paterson. „A comparison of Loon balloon observations and stratospheric reanalysis products“. Atmospheric Chemistry and Physics 17, Nr. 2 (19.01.2017): 855–66. http://dx.doi.org/10.5194/acp-17-855-2017.

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Abstract. Location information from long-duration super-pressure balloons flying in the Southern Hemisphere lower stratosphere during 2014 as part of X Project Loon are used to assess the quality of a number of different reanalyses including National Centers for Environmental Prediction Climate Forecast System version 2 (NCEP-CFSv2), European Centre for Medium-Range Weather Forecasts (ERA-Interim), NASA Modern Era Retrospective-Analysis for Research and Applications (MERRA), and the recently released MERRA version 2. Balloon GPS location information is used to derive wind speeds which are then compared with values from the reanalyses interpolated to the balloon times and locations. All reanalysis data sets accurately describe the winds, with biases in zonal winds of less than 0.37 m s−1 and meridional biases of less than 0.08 m s−1. The standard deviation on the differences between Loon and reanalyses zonal winds is latitude-dependent, ranging between 2.5 and 3.5 m s−1, increasing equatorward. Comparisons between Loon trajectories and those calculated by applying a trajectory model to reanalysis wind fields show that MERRA-2 wind fields result in the most accurate simulated trajectories with a mean 5-day balloon–reanalysis trajectory separation of 621 km and median separation of 324 km showing significant improvements over MERRA version 1 and slightly outperforming ERA-Interim. The latitudinal structure of the trajectory statistics for all reanalyses displays marginally lower mean separations between 15 and 35° S than between 35 and 55° S, despite standard deviations in the wind differences increasing toward the equator. This is shown to be related to the distance travelled by the balloon playing a role in the separation statistics.
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Dissertationen zum Thema "Balloon observations"

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Brodbeck, Roland. „Balloon-borne far-infrared Fabry-Perot spectrometer for astrophysical observations /“. [S.l.] : [s.n.], 1997. http://e-collection.ethbib.ethz.ch/show?type=diss&nr=12510.

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Zhang, Guochang. „Validation of target parameters of ENVISAT chemistry instruments with correlative balloon observations obtained by MIPAS-B“. Karlsruhe : FZKA, 2006. http://bibliothek.fzk.de/zb/berichte/FZKA7242.pdf.

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Zhang, Guochang [Verfasser]. „Validation of target parameters of ENVISAT chemistry instruments with correlative balloon observations obtained by MIPAS-B / Forschungszentrum Karlsruhe GmbH, Karlsruhe. Guochang Zhang“. Karlsruhe : FZKA, 2006. http://d-nb.info/98154696X/34.

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Corcos, Milena. „Processes affecting cirrus clouds life cycle at the tropical tropopause layer : contributions from the Stratéole-2 campaigns“. Electronic Thesis or Diss., Sorbonne université, 2023. http://www.theses.fr/2023SORUS119.

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Cette thèse s'intéresse à l'observation des ondes de gravité dans la tropopause tropicale (TTL pour tropical tropopause layer) par ballons pressurisés, et à leur impact sur les cirrus. Dans un premier temps, l'activité des ondes de gravité est quantifiée grâce aux observations in-situ des ballons pressurisés des deux premières campagnes de Stratéole-2. Le lien entre la convection profonde tropicale et l'activité des ondes est démontré à l'échelle synoptique par la diminution de l'amplitude des ondes avec la distance aux cellules convectives. La variabilité géographique de l'activité des ondes de gravité, de leur intermittence, ainsi que leur variabilité inter-annuelle sont également évaluées. Dans un second temps, l'impact des ondes de gravité sur les cirrus est étudié grâce à la combinaison des mesures lagrangiennes des fluctuations de températures avec un modèle de microphysique prenant en compte la nucléation homogène, la croissance et la sédimentation des cristaux de glace, ainsi qu'une représentation très simplifiée du cisaillement de vent. L'impact des ondes sur la population de glace et les conséquences sur l'évolution des cirrus ainsi que sur leur capacité à assécher les masses d'air lors de l'ascension dans la TTL est quantifié. Les résultats sont comparés avec les observations de la campagne ATTREX dans la TTL au-dessus de l'océan Pacifique, et démontrent l'importance de la représentation réaliste des ondes dans les simulations de microphysique. Enfin, une étude de sensibilité à l'amplitude des ondes de gravité est discutée pour la structure des cirrus et la population de cristaux
This thesis focuses on the observation of gravity waves at the tropical tropopause layer (TTL) by superpressure balloons, and their impact on cirrus clouds. First, the gravity wave activity is quantified thanks to in-situ observations of superpressure balloons from the first two Stratéole-2 campaigns. The link between tropical deep convection and wave activity is demonstrated at a synoptic scale by the decrease of wave amplitude with distance to convective cell. The geographical variability of gravity wave activity, its intermittency, as well as its interannual variability are also studied. In a second step, the impact of gravity waves on cirrus clouds is studied thanks to the combination of Lagrangian measurements of temperature fluctuations with a microphysics model representing the homogeneous nucleation, growth and sedimentation of ice crystals, as well as a very simplified representation of the wind shear. The impact of the waves on ice crystals population and the consequences on the evolution of cirrus clouds and their capacity to dehydrate the air masses during the ascent in the TTL is quantified. The results are compared with observations from the ATTREX campaign in the TTL over the Pacific Ocean, and demonstrate the importance of realistic representation of waves in microphysics simulations. Finally, a sensitivity study to the amplitude of gravity waves is discussed for the cirrus structure and ice crystal population
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Kreycy, Sebastian [Verfasser], und Klaus [Akademischer Betreuer] Pfeilsticker. „Investigation of the Stratospheric Bromine Chemistry by Balloon-Borne Spectroscopic Observations and Photochemical Modelling: A Case Study of J(BrONO2) / k[BrO][NO2] / Sebastian Kreycy ; Betreuer: Klaus Pfeilsticker“. Heidelberg : Universitätsbibliothek Heidelberg, 2013. http://d-nb.info/1177040794/34.

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Boccara, Gillian. „Étude de la dynamique de la basse stratosphère polaire à l’aide des données Vorcore“. Paris 6, 2008. http://www.theses.fr/2008PA066281.

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Ce travail de thèse porte sur les ondes de gravité se propageant dans la basse stratosphère polaire. L’étude utilise les observations enregistrées par des ballons pressurisés de longue durée lors de la campagne Vorcore entre septembre 2005 et janvier 2006. La méthodologie développée s’appuie sur les différentes relations théoriques qui lient les perturbations de pression, de température et de vitesses enregistrées. Elle permet de déduire la direction horizontale de propagation, la vitesse de phase intrinsèque et le flux vertical de quantité de mouvement horizontal transporté par les ondes de gravité. La méthodologie a été testée et validée sur des simulations comportant une ou plusieurs ondes de gravité. En appliquant cette approche aux données Vorcore, les distributions géographiques et temporelles de ces flux ont été étudiées et les sources potentielles des ondes de gravité ont été examinées de même que leur intermittence. Nous avons montré que les montagnes sont des sources d'ondes de gravité prépondérantes, mais nous avons également mis en évidence l'importance des sources non-orographiques au-dessus des océans. Les échelles spatio-temporelles des ondes de gravité sont faibles, c’est pourquoi elles sont paramétrées dans les modèles de circulation générale. Nous avons comparé les flux observés lors de la campagne Vorcore aux flux produits par deux paramétrisations d’ondes de gravité : la première représente les sources d’ondes orographiques (Lott and Miller,1997) et la seconde décrit les sources d’ondes non-orographiques (Hines, 1997). Dans un deuxième temps, les observations de la campagne Vorcore ont été comparées aux analyses ECMWF et aux réanalyses NCEP/NCAR pour en estimer la fiabilité. Les biais et les écarts types obtenus suggèrent une prise en compte insuffisante des ondes de gravité dans les modèles et une mauvaise représentation du vortex polaire dans les réanalyses NCEP/NCAR.
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Court, A. J. „Hard X-ray astronomy from balloon altitudes“. Thesis, University of Southampton, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.377796.

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Da, Costa Ferreira Neri José Angelo. „Mesures des flux de photons gamma atmospherique et diffus a l'aide d'un telescope a temps de vol“. Toulouse 3, 1987. http://www.theses.fr/1987TOU30157.

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Un telescope a temps de vol a ete realise en vue de permettre la detection du rayonnement gamma de moyenne energie (4 mev a 50 mev). On presente les principes de fonctionnement et d'etalonnage ainsi que les caracteristiques determinees par des mesures en laboratoire et des simulations par ordinateur. Les intensites du rayonnement gamma atmospherique en fonction de la pression, les courbes spectrales en energie ainsi que l'inclinaison angulaire sont calculees et comparees aux resultats publies par d'autres observateurs. Le flux de radiations gamma d'origine diffuse cosmique est deduit a partir des courbes de montee des rayonnements atmospheriques
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BAAS, LEFORT MARIE-JOSEPHE. „Maladie de horton et atteinte pulmonaire : a propos d'une observation“. Lyon 1, 1991. http://www.theses.fr/1991LYO1M179.

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Shiomi, Hiroki. „Association of onset to balloon and door to balloon time with long term clinical outcome in patients with ST elevation acute myocardial infarction having primary percutaneous coronary intervention: observational study“. Kyoto University, 2013. http://hdl.handle.net/2433/174776.

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Bücher zum Thema "Balloon observations"

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Fazio, Giovanni G. A balloon-borne 102-cm telescope for far-infrared astronomy. Cambridge, MA: Smithsonian Astrophysical Observatory, 1990.

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Fazio, Giovanni G. A balloon-borne 102-cm telescope for far-infrared astronomy. Cambridge, MA: Smithsonian Astrophysical Observatory, 1990.

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ESA, Symposium on European Rocket &. Balloon Programmes &. Related Research (14th 1999 Potsdam Germany). 14th ESA Symposium on European Rocket and Balloon Programmes and Related Research: Potsdam, Germany, 31 May - 3 June 1999. Noordwijk: European Space Agency, 1999.

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Deutsche Forschungsanstalt für Luft- und Raumfahrt., European Space Agency und ESA Symposium on European Rocket and Balloon Programmes and Related Research (9th : 1989 : Lahnstein, Germany), Hrsg. European rocket and balloon programmes and related research: Proceedings of the ninth ESA/PAC symposium. Paris, France: European Space Agency, 1988.

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L, Conroy, und European Space Agency, Hrsg. 18th ESA Symposium on European Rocket and Balloon Programmes and Related Research: 3-7 June 2007, Visby, Sweden. Noordwijk, the Netherlands: ESA Communication Production Office, ESTEC, 2007.

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ESA, Symposium on European Rocket and Balloon Programmes and Related Research (12th 1995 Lillehammer Norway). 12th ESA Symposium on European Rocket and Balloon Programmes and Related Research, Lillehammer, Norway, 29 May-1 June 1995. Noordwijk, The Netherlands: European Space Agency, 1995.

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ESA Symposium on European Rocket & Balloon Programmes & Related Research (7th 1985 Loen, Norway). Proceedings of the seventh ESA Symposium on ESA Symposium on European Rocket & Balloon Programmes and Related Research Loen, Norway, 5-11 May 1985. Noordwick, Netherlands: ESA Scientific & Technical Publications Branch, 1985.

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8

Meeting, COSPAR Plenary. Balloon technology and observations: Proceedings of Symposium P3 of the COSPAR twenty-ninth Plenary Meeting held in Washington, DC, U.S.A., 28 August-5 September, 1992. Oxford: Published for The Committee on Space Research by Pergamon Press, 1993.

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9

Ryan, Craig. The pre-astronauts: Manned ballooning on the threshold of space. Annapolis, Md: Naval Institute Press, 1995.

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10

United States. Office of Space Science., Hrsg. Infrared, submillimeter, and radio astronomy research and analysis program: Consolidated solicitation for detector and instrument technology development, balloon- and rocket-based observations, laboratory astrophysics : NASA research announcement soliciting proposals ... for the period fiscal year 1997 to fiscal year 1999. Washington, DC: Office of Space Science, National Aeronautics and Space Administration, 1996.

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Buchteile zum Thema "Balloon observations"

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Bowman, Daniel, Jonathan Lees, James Cutts, Attila Komjathy, Eliot Young, Kayla Seiffert, Mark Boslough und Stephen Arrowsmith. „Geoacoustic Observations on Drifting Balloon-Borne Sensors“. In Infrasound Monitoring for Atmospheric Studies, 125–71. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-75140-5_4.

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2

Visser, C. A., W. Jaarsma, F. D. H. Haagen und S. M. P. G. Ernst. „Transesophageal Echocardiographic Observations During Percutaneous Balloon Mitral Valvuloplasty“. In Transesophageal Echocardiography, 244–50. Berlin, Heidelberg: Springer Berlin Heidelberg, 1989. http://dx.doi.org/10.1007/978-3-642-74257-6_29.

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3

Sbarra, C., S. Cortiglioni, G. Bernardi, E. Carretti, S. Cecchini, C. Macculi, G. Ventura et al. „BaR-SPOrt: Balloon-Borne Radiometers for Sky Polarization Observations“. In ESO ASTROPHYSICS SYMPOSIA, 481–82. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/10857580_65.

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4

Bering, Edgar A., James R. Benbrook, Gregory J. Byrne, Danqing Liang und Zhong-Min Lin. „Balloon Observations of the Electric Field Over South Pole: Convection Patterns“. In Electromagnetic Coupling in the Polar Clefts and Caps, 137–50. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0979-3_10.

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5

Bernardis, P., S. Masi, B. Melchiorri und F. Melchiorri. „Balloon-Borne Observations of CMB Anisotropies at Intermediate Angular Scales, at Submm and MM Wavelengths“. In Observational Tests of Cosmological Inflation, 443–46. Dordrecht: Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3510-8_47.

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6

Teegarden, B. J. „Balloon Observations of the Galactic Center 511 keV Line and their Relationship to Satellite Results“. In The Gamma Ray Sky with Compton GRO and SIGMA, 255–66. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0067-0_21.

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Mironova, Irina A., und Galina A. Bazilevskaya. „Estimation of Characterized Ionization Rates During Geomagnetic Disturbances with Kp = 4 Based on Balloon Observations“. In Springer Proceedings in Earth and Environmental Sciences, 383–89. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-40728-4_29.

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8

Boreiko, R. T., T. A. Clark, D. A. Naylor und J. R. Busler. „High-n Hydrogen Lines in Solar Infrared Spectra from Balloon-Borne, Mauna Kea, and ATMOS Observations“. In Infrared Solar Physics, 365–70. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1926-9_45.

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9

Isobe, S., H. Tanabe, T. Hirayama, Y. Koma, J. Soegijo und N. Baba. „Balloon Observation of the F-corona at the 1983 Total Solar Eclipse“. In Properties and Interactions of Interplanetary Dust, 49–54. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5464-9_11.

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Agrinier, B., E. Costa, G. Gerardi, C. Gouiffes, P. Mandrou, J. L. Masnou, E. Massaro et al. „Balloon observation of the Crab pulsar in the energy range 0.2–6 MeV“. In Timing Neutron Stars, 343–46. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2273-0_30.

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Konferenzberichte zum Thema "Balloon observations"

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Ramon, Didier, Colette Brogniez, P. Lecomte, Jacqueline Lenoble, Christian Verwaerde, Paul C. Simon und C. Muller. „Detection of aerosols from balloon limb observations“. In Satellite Remote Sensing II, herausgegeben von Richard P. Santer. SPIE, 1995. http://dx.doi.org/10.1117/12.228528.

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2

Jacob, Jamey D., Brian R. Elbing, Emalee Hough, Taylor Swaim, Zach Yap und Alexis Vance. „Solar Balloon Development for High Altitude Observations“. In AIAA AVIATION 2022 Forum. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2022. http://dx.doi.org/10.2514/6.2022-4113.

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A. G., Sreejith, Joice Mathew, Mayuresh Sarpotdar, Nirmal K., Ambily S., Ajin Prakash, Margarita Safonova und Jayant Murthy. „Balloon UV experiments for astronomical and atmospheric observations“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Christopher J. Evans, Luc Simard und Hideki Takami. SPIE, 2016. http://dx.doi.org/10.1117/12.2232246.

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Young, Eliot F., Mark A. Bullock, Alan Kraut, Graham Orr, Kevin Swartzlander, Tony Wimer, Elton Wong et al. „A balloon-borne stratospheric telescope for Venus observations“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Larry M. Stepp und Roberto Gilmozzi. SPIE, 2008. http://dx.doi.org/10.1117/12.790032.

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5

Komhyr, W. D., J. A. Lathrop und D. P. Opperman. „ECC Ozonesonde and Dobson Umkehr Observations During STOIC 1989“. In Optical Remote Sensing of the Atmosphere. Washington, D.C.: Optica Publishing Group, 1990. http://dx.doi.org/10.1364/orsa.1990.wb7.

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Annotation:
Ten electrochemical concentration cell (ECC) ozonesondes were successfully flown at the Jet Propulsion Laboratory’s Table Mountain Facility during the Stratospheric Ozone Intercomparison Campaign (STOIC) conducted July 19 to August 2, 1989. Umkehr observations were made with a Dobson spectrophotometer during most mornings and afternoons. Ozone measurements were conducted primarily to assess the performance of lidar and microwave instrumentation destined for use in the planned station Network for Detection of Stratospheric Change (NDSC). Because the lidar and microwave are remote ozone measurement techniques, it was of interest to compare data obtained with these instruments with data from balloon-borne ECC ozonesondes that measure ozone directly by counting ozone molecules during balloon ascent. While most of the balloon soundings reached altitudes of 30-34 km, ozone measurements to about 39 km were obtained for two of the soundings.
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Kobayashi, Ken, Saku Tsuneta, Tomonori Tamura, Kazuyoshi Kumagai, Yukio Katsukawa, Masahito Kubo, Takamasa Yamagami und Yoshitaka Saito. „Balloon-borne hard x-ray spectrometer for flare observations“. In Astronomical Telescopes and Instrumentation, herausgegeben von Joachim E. Truemper und Harvey D. Tananbaum. SPIE, 2003. http://dx.doi.org/10.1117/12.461284.

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Eaton, Frank D., Patrick R. Kelly, Demos T. Kyrazis und Sheldon S. Stokes. „Refractivity turbulence observations using a new balloon-ring platform“. In AeroSense 2002, herausgegeben von William E. Thompson und Paul H. Merritt. SPIE, 2002. http://dx.doi.org/10.1117/12.472364.

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8

Carli, B. „Far-Infrared Remote Sensing from Balloon Platforms“. In Optical Remote Sensing of the Atmosphere. Washington, D.C.: Optica Publishing Group, 1990. http://dx.doi.org/10.1364/orsa.1990.tha1.

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Degiacomi, C. G., A. Holenstein, F. K. Kneubuhl und D. Huguenin. „Balloon-Borne Observations Of The Cygnus Region In The Far Infrared“. In 13 Intl Conf on Infrared and Millimeter Waves, herausgegeben von Richard J. Temkin. SPIE, 1988. http://dx.doi.org/10.1117/12.978338.

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10

Kunieda, Hideyo. „Balloon-borne hard x-ray imaging observations of non-thermal phenomena“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Martin J. L. Turner und Günther Hasinger. SPIE, 2006. http://dx.doi.org/10.1117/12.671002.

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Berichte der Organisationen zum Thema "Balloon observations"

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Novak, Giles. Keynote Presentation: Balloon-Borne Observations of Cosmic Magnetism. Ames (Iowa): Iowa State University. Library. Digital Press, Januar 2015. http://dx.doi.org/10.31274/ahac.5584.

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2

Krishnamoorthy, Siddharth, Attila Komjathy, James A. Cutts, Philippe Lognonne, Raphael F. Garcia, Mark P. Panning, Paul K. Byrne et al. Seismology on Venus with infrasound observations from balloon and orbit. Office of Scientific and Technical Information (OSTI), März 2020. http://dx.doi.org/10.2172/1603861.

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3

Beasley, William H. Balloon-Borne Electric-Field Observations Relevant to Models for Sprites and Jets. Fort Belvoir, VA: Defense Technical Information Center, September 1999. http://dx.doi.org/10.21236/ada380886.

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4

Guzik, T. Gregory, A. Spring, R. Dupruis, W. Freeman, Hannah Gardiner und C. Myers. The Pressure, Humidity, And Temperature—Tests and Camera Observations (PHAT-TACO) Student-Built Balloon Payload. Ames (Iowa): Iowa State University. Library. Digital Press, Januar 2011. http://dx.doi.org/10.31274/ahac.8147.

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