Zobrazeno 1 - 9
of 9
pro vyhledávání: '"S. T. Badman"'
Autor:
S. T. Alnussirat, R. Livi, D. E. Larson, A. Rahmati, P. L. Whittlesey, O. Romeo, S. T. Badman, Milo Buitrago-Casas, Juan Carlos Martínez Oliveros, M. Pulupa, S. D. Bale, J. Huang, J. Verniero, N. Raouafi, Donald Mitchell, D. J. McComas, Matt Hill, Christina Cohen
Publikováno v:
The Astrophysical Journal Letters, Vol 954, Iss 1, p L32 (2023)
During Encounter 11, Parker Solar Probe observed a low-energy dispersive ions event of solar origin. The event was observed in the SPAN-I and IS⊙IS EPI-Lo sensors. The event started at a few MeV energy in the EPI-Lo sensor and progressed down in en
Externí odkaz:
https://doaj.org/article/856fff196b314d2ba911ec876c2c32d8
Autor:
O. M. Romeo, C. R. Braga, S. T. Badman, D. E. Larson, M. L. Stevens, J. Huang, T. Phan, A. Rahmati, R. Livi, S. T. Alnussirat, P. L. Whittlesey, A. Szabo, K. G. Klein, T. Niembro-Hernandez, K. Paulson, J. L. Verniero, D. Lario, N. E. Raouafi, T. Ervin, J. Kasper, M. Pulupa, S. D. Bale, M. G. Linton
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 2, p 168 (2023)
During the thirteenth encounter of the Parker Solar Probe (PSP) mission, the spacecraft traveled through a topologically complex interplanetary coronal mass ejection (ICME) beginning on 2022 September 5. PSP traversed through the flank and wake of th
Externí odkaz:
https://doaj.org/article/b903da2065b0484397ff347fe97d820d
Autor:
Nooshin Davis, B. D. G. Chandran, T. A. Bowen, S. T. Badman, T. Dudok de Wit, C. H. K. Chen, S. D. Bale, Zesen Huang, Nikos Sioulas, Marco Velli
Publikováno v:
The Astrophysical Journal, Vol 950, Iss 2, p 154 (2023)
The power spectrum of magnetic field fluctuations in the fast solar wind ( V _SW > 500 km s ^−1 ) at magnetohydrodynamic scales is characterized by two different power laws on either side of a break frequency f _b . The low-frequency range at frequ
Externí odkaz:
https://doaj.org/article/e44033fcd63c44ecadd8f54e97b407d8
Autor:
S. T. Badman, P. Riley, S. I. Jones, T. K. Kim, R. C. Allen, C. N. Arge, S. D. Bale, C. J. Henney, J. C. Kasper, P. Mostafavi, N. V. Pogorelov, N. E. Raouafi, M. L. Stevens, J. L. Verniero
Publikováno v:
Journal of Geophysical Research: Space Physics. 128
Drawing connections between heliospheric spacecraft and solar wind sources is a vital step in understanding the evolution of the solar corona into the solar wind and contextualizing \textit{in situ} timeseries. Furthermore, making advanced prediction
Autor:
N. E. Raouafi, L. Matteini, J. Squire, S. T. Badman, M. Velli, K. G. Klein, C. H. K. Chen, W. H. Matthaeus, A. Szabo, M. Linton, R. C. Allen, J. R. Szalay, R. Bruno, R. B. Decker, M. Akhavan-Tafti, O. V. Agapitov, S. D. Bale, R. Bandyopadhyay, K. Battams, L. Berčič, S. Bourouaine, T. A. Bowen, C. Cattell, B. D. G. Chandran, R. Chhiber, C. M. S. Cohen, R. D’Amicis, J. Giacalone, P. Hess, R. A. Howard, T. S. Horbury, V. K. Jagarlamudi, C. J. Joyce, J. C. Kasper, J. Kinnison, R. Laker, P. Liewer, D. M. Malaspina, I. Mann, D. J. McComas, T. Niembro-Hernandez, T. Nieves-Chinchilla, O. Panasenco, P. Pokorný, A. Pusack, M. Pulupa, J. C. Perez, P. Riley, A. P. Rouillard, C. Shi, G. Stenborg, A. Tenerani, J. L. Verniero, N. Viall, A. Vourlidas, B. E. Wood, L. D. Woodham, T. Woolley
Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to determine the structure and dynamics of the Sun's coronal magnetic field, understand
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::564aec0a61159d55b3ccc75c260fcd40
http://arxiv.org/abs/2301.02727
http://arxiv.org/abs/2301.02727
Autor:
D. de Pablos, T. Samanta, S. T. Badman, C. Schwanitz, S. M. Bahauddin, L. K. Harra, G. Petrie, C. Mac Cormack, C. H. Mandrini, N. E. Raouafi, V. Martinez Pillet, M. Velli
Publikováno v:
Solar Physics, 297 (7)
Parker Solar Probe observations show ubiquitous magnetic-field reversals closer to the Sun, often referred to as "switchbacks". The switchbacks have been observed before in the solar wind near 1 AU and beyond, but their occurrence was historically ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35b8867a896b06d4207ced4619cfd114
https://hdl.handle.net/20.500.11850/559662
https://hdl.handle.net/20.500.11850/559662
Autor:
J. C. Kasper, K. G. Klein, E. Lichko, Jia Huang, C. H. K. Chen, S. T. Badman, J. Bonnell, P. L. Whittlesey, R. Livi, D. Larson, M. Pulupa, A. Rahmati, D. Stansby, K. E. Korreck, M. Stevens, A. W. Case, S. D. Bale, M. Maksimovic, M. Moncuquet, K. Goetz, J. S. Halekas, D. Malaspina, Nour E. Raouafi, A. Szabo, R. MacDowall, Marco Velli, Thierry Dudok de Wit, G. P. Zank
Publikováno v:
Physical review letters. 127(25)
The high temperatures and strong magnetic fields of the solar corona form streams of solar wind that expand through the Solar System into interstellar space. At 09:33 UT on 28 April 2021 Parker Solar Probe entered the magnetized atmosphere of the Sun
Autor:
S. D. Bale, T. S. Horbury, M. Velli, M. I. Desai, J. S. Halekas, M. D. McManus, O. Panasenco, S. T. Badman, T. A. Bowen, B. D. G. Chandran, J. F. Drake, J. C. Kasper, R. Laker, A. Mallet, L. Matteini, T. D. Phan, N. E. Raouafi, J. Squire, L. D. Woodham, T. Woolley
Publikováno v:
The Astrophysical Journal. 923:174
One of the striking observations from the Parker Solar Probe (PSP) spacecraft is the prevalence in the inner heliosphere of large amplitude, Alfv\'enic magnetic field reversals termed 'switchbacks'. These $\delta B_R/B \sim \mathcal{O}(1$) fluctuatio
Autor:
R. C. Allen, D. Lario, D. Odstrcil, G. C. Ho, L. K. Jian, C. M. S. Cohen, S. T. Badman, S. I. Jones, C. N. Arge, M. L. Mays, G. M. Mason, S. D. Bale, J. W. Bonnell, A. W. Case, E. R. Christian, T. Dudok de Wit, K. Goetz, P. R. Harvey, C. J. Henney, M. E. Hill
Publikováno v:
Astrophysical Journal Supplement Series; Feb2020, Vol. 246 Issue 2, p1-1, 1p