Zobrazeno 1 - 10
of 178
pro vyhledávání: '"Szabó, Ádám"'
Autor:
Romanelli, Norberto, Andres, Nahuel, DiBraccio, Gina, Verniero, Jaye, Gruesbeck, Jacob, Szabo, Adam, Espley, Jared, Halekas, Jasper
Solar wind turbulence is a dynamical phenomenon that evolves with heliocentric distance. Orbiting Mars since September 2014, Mars Atmosphere and Volatile EvolutioN (MAVEN) offers a unique opportunity to explore some of its main properties beyond ~1.3
Externí odkaz:
http://arxiv.org/abs/2406.18349
In-situ measurements of the solar wind, a turbulent and anisotropic plasma flow originating at the Sun, are mostly carried out by single spacecraft, resulting in one-dimensional time series. The conversion of these measurements to the spatial frame o
Externí odkaz:
http://arxiv.org/abs/2405.12547
Autor:
Klein, Kristopher G., Spence, Harlan, Alexandrova, Olga, Argall, Matthew, Arzamasskiy, Lev, Bookbinder, Jay, Broeren, Theodore, Caprioli, Damiano, Case, Anthony, Chandran, Benjamin, Chen, Li-Jen, Dors, Ivan, Eastwood, Jonathan, Forsyth, Colin, Galvin, Antoinette, Genot, Vincent, Halekas, Jasper, Hesse, Michael, Hine, Butler, Horbury, Tim, Jian, Lan, Kasper, Justin, Kretzschmar, Matthieu, Kunz, Matthew, Lavraud, Benoit, Contel, Olivier Le, Mallet, Alfred, Maruca, Bennett, Matthaeus, William, Niehof, Jonathan, O'Brian, Helen, Owen, Christopher, Retino, Alessandro, Reynolds, Christopher, Roberts, Owen, Schekochihin, Alexander, Skoug, Ruth, Smith, Charles, Smith, Sonya, Steinberg, John, Stevens, Michael, Szabo, Adam, TenBarge, Jason, Torbert, Roy, Vasquez, Bernard, Verscharen, Daniel, Whittlesey, Phyllis, Wickizer, Brittany, Zank, Gary, Zweibel, Ellen
HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in p
Externí odkaz:
http://arxiv.org/abs/2306.06537
Autor:
Huang, Jia, Kasper, J. C., Larson, Davin E., McManus, Michael D., Whittlesey, P., Livi, Roberto, Rahmati, Ali, Romeo, Orlando, Klein, K. G., Sun, Weijie, van der Holst, Bart, Huang, Zhenguang, Jian, Lan K., Szabo, Adam, Verniero, J. L., Chen, C. H. K., Lavraud, B., Liu, Mingzhe, Badman, Samuel T., Niembro, Tatiana, Paulson, Kristoff, Stevens, M., Case, A. W., Pulupa, Marc, Bale, Stuart D., Halekas, J. S.
In general, slow solar wind from the streamer belt forms a high plasma beta equatorial plasma sheet around the heliospheric current sheet (HCS) crossing, namely the heliospheric plasma sheet (HPS). Current Parker Solar Probe (PSP) observations show t
Externí odkaz:
http://arxiv.org/abs/2302.07230
Autor:
Vessal, Arsalan, Alijanpourotaghsara, Amirreza, Strelnikov, David, Persely, Aliz, Piroska, Marton, Alijanpour, Amirmasoud, Jokkel, Zsofia, Szalontai, Laszlo, Forgo, Bianka, Kozak, Lajos Rudolf, Bekesy-Szabo, Adam, Maurovich-Horvat, Pal, Tarnoki, David Laszlo, Tarnoki, Adam Domonkos
Publikováno v:
In Psychiatry Research: Neuroimaging December 2024 345
Autor:
Lamdouar, Hala, Sundaresan, Sairam, Jungbluth, Anna, Saikia, Sudeshna Boro, Camarata, Amanda Joy, Miles, Nathan, Scoczynski, Marcella, Stone, Mavis, Sarah, Anthony, Muñoz-Jaramillo, Andrés, Narock, Ayris, Szabo, Adam
The solar wind consists of charged particles ejected from the Sun into interplanetary space and towards Earth. Understanding the magnetic field of the solar wind is crucial for predicting future space weather and planetary atmospheric loss. Compared
Externí odkaz:
http://arxiv.org/abs/2203.01184
Autor:
Bowen, Trevor A., Bale, Stuart D., Bonnell, John W., de Wit, Thierry Dudok, Goetz, Keith, Goodrich, Katherine, Gruesbeck, Jacob, Harvey, Peter R., Jannet, Guillaume, MacDowall, Andriy Koval Robert J., Malaspina, David M., Pulupa, Marc, Revillet, Claire, Sheppard, David, Szabo, Adam
NASA's Parker Solar Probe (PSP) mission is currently investigating the local plasma environment of the inner-heliosphere ($< $0.25$R_\odot$) using both {\em{in-situ}} and remote sensing instrumentation. Connecting signatures of microphysical particle
Externí odkaz:
http://arxiv.org/abs/2001.04587
Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe
Autor:
Krupar, Vratislav, Szabo, Adam, Maksimovic, Milan, Kruparova, Oksana, Kontar, Eduard P., Balmaceda, Laura A., Bonnin, Xavier, Bale, Stuart D., Pulupa, Marc, Malaspina, David M., Bonnell, John W., Harvey, Peter R., Goetz, Keith, de Wit, Thierry Dudok, MacDowall, Robert J., Kasper, Justin C., Case, Anthony W., Korreck, Kelly E., Larson, Davin E., Livi, Roberto, Stevens, Michael L., Whittlesey, Phyllis L., Hegedus, Alexander M.
Radio waves are strongly scattered in the solar wind, so that their apparent sources seem to be considerably larger and shifted than the actual ones. Since the scattering depends on the spectrum of density turbulence, better understanding of the radi
Externí odkaz:
http://arxiv.org/abs/2001.03476
Publikováno v:
In NeuroImage January 2023 265
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