Zobrazeno 1 - 10
of 1 237
pro vyhledávání: '"Owen, Christopher"'
Autor:
Davies, Emma E., Rüdisser, Hannah T., Amerstorfer, Ute V., Möstl, Christian, Bauer, Maike, Weiler, Eva, Amerstorfer, Tanja, Majumdar, Satabdwa, Hess, Phillip, Weiss, Andreas J., Reiss, Martin A., Green, Lucie M., Long, David M., Nieves-Chinchilla, Teresa, Trotta, Domenico, Horbury, Timothy S., O'Brien, Helen, Fauchon-Jones, Edward, Morris, Jean, Owen, Christopher J., Bale, Stuart D., Kasper, Justin C.
As both Parker Solar Probe (PSP) and Solar Orbiter (SolO) reach heliocentric distances closer to the Sun, they present an exciting opportunity to study the structure of CMEs in the inner heliosphere. We present an analysis of the global flux rope str
Externí odkaz:
http://arxiv.org/abs/2405.10810
Autor:
Soni, Shirsh Lata, Akhavan-Tafti, Mojtaba, Suen, Gabriel Ho Hin, Kasper, Justin, Velli, Marco, De Marco, Rossana, Owen, Christopher
Magnetic switchbacks are distinct magnetic structures characterized by their abrupt reversal in the radial component of the magnetic field within the pristine solar wind. Switchbacks are believed to lose magnetic energy with heliocentric distance. To
Externí odkaz:
http://arxiv.org/abs/2402.13964
Autor:
Zaslavsky, Arnaud, Kasper, Justin C., Kontar, Eduard P., Larson, Davin E., Maksimovic, Milan, Marques, José M. D. C., Nicolaou, Georgios, Owen, Christopher J., Romeo, Orlando, Whittlesey, Phyllis L.
This study explores the impact of a turbulent scattering mechanism, akin to those influencing solar and galactic cosmic rays propagating in the interplanetary medium, on the population of suprathermal electrons in the solar wind. We employ a Fokker-P
Externí odkaz:
http://arxiv.org/abs/2401.04222
Autor:
Lorfing, Camille Y., Reid, Hamish A. S., Gomez-Herrero, Raul, Maksimovic, Milan, Nicolaou, Georgios, Owen, Christopher J., Rodriguez-Pacheco, Javier, Ryan, Daniel F., Trotta, Domenico, Verscharen, Daniel
Solar Orbiter's four in-situ instruments have recorded numerous energetic electron events at heliocentric distances between 0.5 and 1au. We analyse energetic electron fluxes, spectra, pitch angle distributions, associated Langmuir waves, and type III
Externí odkaz:
http://arxiv.org/abs/2311.14444
Autor:
Dimmock, Andrew P., Gedalin, Michael, Lalti, Ahmad, Trotta, Domenico, Khotyaintsev, Yuri V., Graham, Daniel B., Johlander, Andreas, Vainio, Rami, Blanco-Cano, Xochitl, Kajdič, Primoz, Owen, Christopher J., Wimmer-Schweingruber, Robert F.
Solar Orbiter, a mission developed by the European Space Agency, explores in situ plasma across the inner heliosphere while providing remote-sensing observations of the Sun. Our study examines particle observations for the 30 October 2021 shock. The
Externí odkaz:
http://arxiv.org/abs/2310.09050
Autor:
Voshchepynets, Andrii, Agapitov, Oleksiy, Wilson III, Lynn, Angelopoulos, Vassilis, Alnussirat, Samer T., Balikhin, Michael, Hlebena, Myroslava, Korol, Ihor, Larson, Davin, Mitchell, David, Owen, Christopher, Rahmati, Ali, Analysis, Department of System, Theory, Optimization, University, Uzhhorod National, Uzhhorod, Ukraine, Laboratory, Space Sciences, Berkeley, University of California Berkeley, Astronomy, Department, Space Physics, Kyiv, National Taras Shevchenko University of, Kyiv, Center, Goddard Space Flight, Aeronautics, National, Administration, Space, Greenbelt, MD, Earth, Department of, Planetary, Sciences, Space, Angeles, University of California Los, Angeles, Los, CA}, Sheffield, University of, Sheffield, UK, Algebra, Department of, Equation, Differential, Analysis, Department of Mathematical, Lublin, The John Paul II Catholic University of, Lublin, Poland}
We present the results of processing the effects of the powerful Gamma Ray Burst GRB221009A captured by the charged particle detectors (electrostatic analyzers and solid-state detectors) onboard spacecraft at different points in the heliosphere on Oc
Externí odkaz:
http://arxiv.org/abs/2309.05856
Large-scale compressive slow-mode-like fluctuations can cause variations in the density, temperature, and magnetic-field magnitude in the solar wind. In addition, they also lead to fluctuations in the differential flow $U_{\rm p\alpha}$ between $\alp
Externí odkaz:
http://arxiv.org/abs/2308.02036
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