Literatura académica sobre el tema "Multi-Instrumental observations"
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Artículos de revistas sobre el tema "Multi-Instrumental observations"
Kozlovsky, A., S. Shalimov, J. Kero, T. Raita y M. Lester. "Multi-Instrumental Observations of Nonunderdense Meteor Trails". Journal of Geophysical Research: Space Physics 123, n.º 7 (julio de 2018): 5974–89. http://dx.doi.org/10.1029/2018ja025405.
Texto completoMoreno-Ibáñez, Manuel, Josep M. Trigo-Rodríguez, José María Madiedo, Jérémie Vaubaillon, Iwan P. Williams, Maria Gritsevich, Lorenzo G. Morillas et al. "Multi-instrumental observations of the 2014 Ursid meteor outburst". Monthly Notices of the Royal Astronomical Society 468, n.º 2 (9 de marzo de 2017): 2206–13. http://dx.doi.org/10.1093/mnras/stx592.
Texto completoNakariakov, V. M., M. K. Kosak, D. Y. Kolotkov, S. A. Anfinogentov, P. Kumar y Y. J. Moon. "Properties of Slow Magnetoacoustic Oscillations of Solar Coronal Loops by Multi-instrumental Observations". Astrophysical Journal 874, n.º 1 (19 de marzo de 2019): L1. http://dx.doi.org/10.3847/2041-8213/ab0c9f.
Texto completoParker, Q. A. y F. G. Watson. "A Flair for Multi-Object Spectroscopy". Symposium - International Astronomical Union 161 (1994): 85–88. http://dx.doi.org/10.1017/s0074180900047124.
Texto completoLiu, Lei, Yibin Yao y Ercha Aa. "Multi-Instrumental Observations of Early Morning Equatorial Plasma Depletions During the 2017 Memorial Weekend Storm". IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing 13 (2020): 5351–57. http://dx.doi.org/10.1109/jstars.2020.3022748.
Texto completoRamaprakash, A. N., S. N. Tandon y R. Gupta. "Imaging Polarimetry of Nearby Molecular Clouds". International Astronomical Union Colloquium 166 (1997): 243–46. http://dx.doi.org/10.1017/s0252921100071050.
Texto completoSzkop, Artur, Alnilam Fernandes y Aleksander Pietruczuk. "Towards a Multi-Instrumental Approach to Closing Aerosol Optical Extinction Profiles". Atmosphere 13, n.º 9 (6 de septiembre de 2022): 1443. http://dx.doi.org/10.3390/atmos13091443.
Texto completoKaltman, T. I., A. G. Stupishin, S. A. Anfinogentov, V. M. Nakariakov, M. A. Loukitcheva y A. V. Shendrik. "Hot Jets in the Solar Corona: Creating a Catalogue of Events Based on Multi-Instrumental Observations". Geomagnetism and Aeronomy 61, n.º 7 (diciembre de 2021): 1083–91. http://dx.doi.org/10.1134/s0016793221070070.
Texto completoAstafyeva, E., I. Zakharenkova, J. D. Huba, E. Doornbos y J. van den IJssel. "Global Ionospheric and Thermospheric Effects of the June 2015 Geomagnetic Disturbances: Multi-Instrumental Observations and Modeling". Journal of Geophysical Research: Space Physics 122, n.º 11 (noviembre de 2017): 11,716–11,742. http://dx.doi.org/10.1002/2017ja024174.
Texto completoBothe, Oliver, Sebastian Wagner y Eduardo Zorita. "Inconsistencies between observed, reconstructed, and simulated precipitation indices for England since the year 1650 CE". Climate of the Past 15, n.º 1 (15 de febrero de 2019): 307–34. http://dx.doi.org/10.5194/cp-15-307-2019.
Texto completoTesis sobre el tema "Multi-Instrumental observations"
Dolliou, Antoine. "L'impact de petits événements brillants UV-EUV sur le chauffage coronal du Soleil calme : analyse de données de Solar Orbiter et simulations hydrodynamiques de boucles magnétiques". Electronic Thesis or Diss., université Paris-Saclay, 2024. http://www.theses.fr/2024UPASP112.
Texto completoThe Solar corona temperature is maintained at more than 1 MK. One of the main theories of the coronal formation (Parker, 1988) suggests that the magnetic energy is dissipated into the corona through a high number of impulsive, low energetic (1E24 ergs) heating events, called “nanoflares.” On 30 May 2020, during its first high temporal and spatial resolutions observations, 1463 small (400 - 4000 km) and short-lived (10-200 s) EUV brightenings, referred to as “events”, were detected in the Quiet Sun (QS) by the high-resolution UV imager HRIEUV (174 Angström), on board Solar Orbiter. I tested the possibility that they might be signatures of nanoflare heating.As HRIEUV is sensitive to continuous temperature coverage, in particular between 1 MK and 0.3 MK, my goal was to verify if these events do reach coronal temperatures and, thus, if they contribute directly to the coronal heating.For the 30 May 2020 dataset, only SDO/AIA data were available to perform temperature diagnostics. To do so, I applied the “time lags” method to the coronal channels of AIA. This method provides signatures on plasma cooling or heating above 1 MK, as most AIA channels have their sensitivity peak at these temperatures. I compared the statistics between the events and the rest of the QS and concluded that the events are characterized by short time lags below the AIA cadence of 12 s. These results were confirmed by extending the study to later datasets using a higher AIA cadence of 6s. I proposed two possible interpretations: (1) the events peak below 1 MK, where the AIA response functions behave similarly; (2) the events' cooling time scale is too short to be resolved by the AIA cadence. Spectroscopic observations are thus necessary to better constrain the temperature of these events.To complete this work, I used co-temporal 2022 and 2023 QS data from HRIEUV, AIA (imagers), from Solar Orbiter/SPICE and HINODE/EIS (spectroscopy). I first detected events in HRIEUV and identified them in SPICE or EIS and in AIA. Then, I extracted the light curves from spectral lines emitted in a wide range of temperatures and applied spectroscopic diagnostics to derive the density as a function of temperature. I concluded that the emission of these events mainly originates from plasma below 1 MK. As such, most of them hardly contribute directly to the coronal heating.In order to understand the physical properties driving these events, I reproduced their observational signatures using the HYDRAD 1D hydrodynamics code. To do so, I computed the synthetic light curves from different models of short loops submitted to impulsive heating by changing parameters such as the loop length or the heating strength. I looked for the models that best reproduce the observations, including the light curves co-temporal peak. The work compares the results for two different types of loops that have very distinct properties: “hot” (T > 1E5 K) and “cool” (T < 1E5 K) loops. The results showed that cool loops submitted to impulsive heating are good candidates to explain the origin of most of the events detected by HRIEUV.To conclude, most of these events are probably not the signature of coronal heating phenomena, unless their coronal emission is below the instrumental limitations. One consequence of this work would be to reconsider their role in heating the QS corona, as they might instead provide a major contribution to the heating of the cooler lower solar atmosphere
Capítulos de libros sobre el tema "Multi-Instrumental observations"
Jähnichen, Gisa. "Rituals with Music and Food, Food with Music and Rituals". En Wie wir leben wollen. Kompendium zu Technikfolgen von Digitalisierung, Vernetzung und Künstlicher Intelligenz, 193–204. Logos Verlag Berlin, 2021. http://dx.doi.org/10.30819/5319.15.
Texto completoActas de conferencias sobre el tema "Multi-Instrumental observations"
Zakharenkova, Irina, Iurii Cherniak, John Braun, Qian Wu y Sergey Sokolovskiy. "Multi-instrumental Monitoring of Equatorial Ionospheric Irregularities Using COSMIC-2 Observations". En XXXVth URSI General Assembly and Scientific Symposium. Gent, Belgium: URSI – International Union of Radio Science, 2023. http://dx.doi.org/10.46620/ursigass.2023.2865.lngt5063.
Texto completoShukla, Dhwanil, Nandeesh Hiremath, Sahaj Patel y Narayanan Komerath. "Aerodynamic Interactions Study on Low-Re Coaxial and Quad-Rotor Configurations". En ASME 2017 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2017. http://dx.doi.org/10.1115/imece2017-71005.
Texto completoAl Rubaya, Ahmed Meshaal, Alexey Alexeyenko y Ashraf Khateeb. "Advanced Downhole Torsional Oscillation Control Tool Improved Dynamics and Field Average ROP". En International Petroleum Technology Conference. IPTC, 2024. http://dx.doi.org/10.2523/iptc-24250-ea.
Texto completoCasero, A., A. Gomaa, J. Ronderos, K. Cawiezel y W. J. Giffin. "8070 Miles from the Field to the Lab and Back: A Pragmatic Sequencing of Laboratory and Field-Based Fluid Testing and QAQC, A Case History from Sichuan Region, China". En SPE Hydraulic Fracturing Technology Conference and Exhibition. SPE, 2021. http://dx.doi.org/10.2118/204189-ms.
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