Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Whittlesey, Phyllis L"'
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:
Palmerio, Erika, Carcaboso, Fernando, Khoo, Leng Ying, Salman, Tarik M., Sánchez-Cano, Beatriz, Lynch, Benjamin J., Rivera, Yeimy J., Pal, Sanchita, Nieves-Chinchilla, Teresa, Weiss, Andreas J., Lario, David, Mieth, Johannes Z. D., Heyner, Daniel, Stevens, Michael L., Romeo, Orlando M., Zhukov, Andrei N., Rodriguez, Luciano, Lee, Christina O., Cohen, Christina M. S., Rodríguez-García, Laura, Whittlesey, Phyllis L., Dresing, Nina, Oleynik, Philipp, Jebaraj, Immanuel C., Fischer, David, Schmid, Daniel, Richter, Ingo, Auster, Hans-Ulrich, Fraschetti, Federico, Mierla, Marilena
On 2022 February 15, an impressive filament eruption was observed off the solar eastern limb from three remote-sensing viewpoints, namely Earth, STEREO-A, and Solar Orbiter. In addition to representing the most-distant observed filament at extreme ul
Externí odkaz:
http://arxiv.org/abs/2401.01875
Autor:
Verscharen, Daniel, Chandran, Benjamin D. G., Boella, Elisabetta, Halekas, Jasper, Innocenti, Maria Elena, Jagarlamudi, Vamsee K., Micera, Alfredo, Pierrard, Viviane, Stverak, Stepan, Vasko, Ivan Y., Velli, Marco, Whittlesey, Phyllis L.
The electrons are an essential particle species in the solar wind. They often exhibit non-equilibrium features in their velocity distribution function. These include temperature anisotropies, tails (kurtosis), and reflectional asymmetries (skewness),
Externí odkaz:
http://arxiv.org/abs/2206.10403
Autor:
Abraham, Joel B., Owen, Christopher J, Verscharen, Daniel, Bakrania, Mayur, Stansby, David, Wicks, Robert T., Nicolaou, Georgios, Whittlesey, Phyllis L, Rueda, Jefferson A. Agudelo, Jeong, Seong-Yeop, Bercic, Laura
We develop and apply a bespoke fitting routine to a large volume of solar wind electron distribution data measured by Parker Solar Probe (PSP) over its first five orbits, covering radial distances from 0.13 to 0.5 au. We characterise the radial evolu
Externí odkaz:
http://arxiv.org/abs/2204.05001
Autor:
Fargette, Naïs, Lavraud, Benoit, Rouillard, Alexis, Réville, Victor, De Wit, Thierry Dudok, Froment, Clara, Halekas, Jasper S., Phan, Tai, Malaspina, David, Bale, Stuart D., Kasper, Justin, Louarn, Philippe, Case, Anthony W., Korreck, Kelly E., Larson, Davin E., Pulupa, Marc, Stevens, Michael L., Whittlesey, Phyllis L., Berthomier, Matthieu
Parker Solar Probe (PSP) data recorded within a heliocentric radial distance of 0.3 AU have revealed a magnetic field dominated by Alfv\'enic structures that undergo large local variations or even reversals of the radial magnetic field. They are call
Externí odkaz:
http://arxiv.org/abs/2109.01519
Autor:
Vech, Daniel, Martinovic, Mihailo M., Klein, Kristopher G., Malaspina, David M., Bowen, Trevor A., Verniero, Jenny L., Paulson, Kristoff, de Wit, Thierry Dudok, Kasper, Justin C., Huang, Jia, Stevens, Michael L., Case, Anthony W., Korreck, Kelly, Mozer, Forrest S., Goodrich, Katherine A., Bale, Stuart D., Whittlesey, Phyllis L., Livi, Roberto, Larson, Davin E., Pulupa, Marc, Bonnell, John, Harvey, Peter, Goetz, Keith, MacDowall, Robert
Context. The first studies with Parker Solar Probe (PSP) data have made significant progress toward the understanding of the fundamental properties of ion cyclotron waves in the inner heliosphere. The survey mode particle measurements of PSP, however
Externí odkaz:
http://arxiv.org/abs/2010.15189
Autor:
Chen, Yu, Hu, Qiang, Zhao, Lingling, Kasper, Justin C., Bale, Stuart D., Korreck, Kelly E., Case, Anthony W., Stevens, Michael L., Bonnell, John W., Goetz, Keith, Harvey, Peter R., Klein, Kristopher G., Larson, Davin E., Livi, Roberto, MacDowall, Robert J., Malaspina, David M., Pulupa, Marc, Whittlesey, Phyllis L.
Small-scale magnetic flux ropes (SFRs) are a type of structures in the solar wind that possess helical magnetic field lines. In a recent report (Chen & Hu 2020), we presented the radial variations of the properties of SFR from 0.29 to 8 au using in s
Externí odkaz:
http://arxiv.org/abs/2007.04551
Autor:
Whittlesey, Phyllis L, Larson, Davin E, Kasper, Justin C, Halekas, Jasper, Abatcha, Mamuda, Abiad, Robert, Berthomier, M., Case, A. W., Chen, Jianxin, Curtis, David W, Dalton, Gregory, Klein, Kristopher G, Korreck, Kelly E, Livi, Roberto, Ludlam, Michael, Marckwordt, Mario, Rahmati, Ali, Robinson, Miles, Slagle, Amanda, Stevens, M L, Tiu, Chris, Verniero, J L
Electrostatic analyzers of different designs have been used since the earliest days of the space age, beginning with the very earliest solar wind measurements made by Mariner 2 en route to Venus in 1962. The Parker Solar Probe (PSP) mission, NASA's f
Externí odkaz:
http://arxiv.org/abs/2002.04080
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
Autor:
Vech, Daniel, Kasper, Justin C., Klein, Kristopher G., Huang, Jia, Stevens, Michael L., Chen, Christopher H. K., Case, Anthony W., Korreck, Kelly, Bale, Stuart D., Bowen, Trevor A., Whittlesey, Phyllis L., Livi, Roberto, Larson, Davin E., Malaspina, David, Pulupa, Marc, Bonnell, John, Harvey, Peter, Goetz, Keith, de Wit, Thierry Dudok, MacDowall, Robert
In this Paper, we present the first results from the Flux Angle operation mode of the Faraday Cup instrument onboard Parker Solar Probe. The Flux Angle mode allows rapid measurements of phase space density fluctuations close to the peak of the proton
Externí odkaz:
http://arxiv.org/abs/1912.07719