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Browsing by Author "Badman, S. T."

Browsing by Author "Badman, S. T."

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  • Dispersive Suprathermal Ion Events Observed by the Parker Solar Probe Mission 
    Alnussirat, S. T.; Livi, R.; Larson, D. E.; Rahmati, A.; Whittlesey, P. L.; Romeo, O.; Badman, S. T.; Buitrago-Casas, Milo; Martínez Oliveros, Juan Carlos; Pulupa, M.; Bale, S. D.; Huang, J.; Verniero, J.; Raouafi, N.; Mitchell, Donald; McComas, D. J.; Hill, Matt; Cohen, Christina (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 ...
  • The Evolution of the 1/f Range within a Single Fast-solar-wind Stream between 17.4 and 45.7 Solar Radii 
    Davis, Nooshin; Chandran, B. D. G.; Bowen, T. A.; Badman, S. T.; de Wit, T. Dudok; Chen, C. H. K.; Bale, S. D.; Huang, Zesen; Sioulas, Nikos; Velli, Marco (2023)
    The power spectrum of magnetic field fluctuations in the fast solar wind (V <sub>SW</sub> > 500 km s<sup>-1</sup>) at magnetohydrodynamic scales is characterized by two different power laws on either side of a break frequency ...
  • Highly structured slow solar wind emerging from an equatorial coronal hole 
    Bale, S. D.; Badman, S. T.; Bonnell, J. W.; Bowen, T. A.; Burgess, D.; Case, Anthony W.; Cattell, C. A.; Chandran, B. D. G.; Chaston, C. C.; Chen, C. H. K.; Drake, J. F.; de Wit, T. Dudok; Eastwood, J. P.; Ergun, R. E.; Farrell, W. M.; Fong, C.; Goetz, K.; Goldstein, M.; Goodrich, K. A.; Harvey, P. R.; Horbury, T. S.; Howes, G. G.; Kasper, Justin C.; Kellogg, P. J.; Klimchuk, J. A.; Korreck, Kelly E.; Krasnoselskikh, V. V.; Krucker, S.; Laker, R.; Larson, D. E.; MacDowall, R. J.; Maksimovic, M.; Malaspina, D. M.; Martinez-Oliveros, J.; McComas, D. J.; Meyer-Vernet, N.; Moncuquet, M.; Mozer, F. S.; Phan, T. D.; Pulupa, M.; Raouafi, N. E.; Salem, C.; Stansby, D.; Stevens, Michael; Szabo, A.; Velli, M.; Woolley, T.; Wygant, J. R. (2019)
    During the solar minimum, when the Sun is at its least active, the solar wind<SUP>1,2</SUP> is observed at high latitudes as a predominantly fast (more than 500 kilometres per second), highly Alfvénic rarefied stream of ...
  • Interchange reconnection as the source of the fast solar wind within coronal holes 
    Bale, S. D.; Drake, J. F.; McManus, M. D.; Desai, M. I.; Badman, S. T.; Larson, D. E.; Swisdak, M.; Horbury, T. S.; Raouafi, N. E.; Phan, T.; Velli, M.; McComas, D. J.; Cohen, C. M. S.; Mitchell, D.; Panasenco, O.; Kasper, J. C. (2023)
    The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called `coronal holes'. The energy source responsible for accelerating the plasma is widely debated; ...
  • Near-Sun In Situ and Remote-sensing Observations of a Coronal Mass Ejection and its Effect on the Heliospheric Current Sheet 
    Romeo, O. M.; Braga, C. R.; Badman, S. T.; Larson, D. E.; Stevens, Michael L.; Huang, J.; Phan, T.; Rahmati, A.; Livi, R.; Alnussirat, S. T.; Whittlesey, P. L.; Szabo, A.; Klein, K. G.; Niembro-Hernandez, T.; Paulson, Kristoff; Verniero, J. L.; Lario, D.; Raouafi, N. E.; Ervin, T.; Kasper, J.; Pulupa, M.; Bale, S. D.; Linton, M. G. (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 ...
  • Parker Solar Probe Enters the Magnetically Dominated Solar Corona 
    Kasper, J. C.; Klein, K. G.; Lichko, E.; Huang, Jia; Chen, C. H. K.; Badman, S. T.; Bonnell, J.; Whittlesey, P. L.; Livi, R.; Larson, D.; Pulupa, M.; Rahmati, A.; Stansby, D.; Korreck, K. E.; Stevens, Michael; Case, Anthony W.; Bale, S. D.; Maksimovic, M.; Moncuquet, M.; Goetz, K.; Halekas, J. S.; Malaspina, D.; Raouafi, Nour E.; Szabo, A.; MacDowall, R.; Velli, Marco; de Wit, Thierry Dudok; Zank, G. P. (2021)
    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 ...
  • Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum 
    Raouafi, N. E.; Matteini, L.; Squire, J.; Badman, S. T.; Velli, M.; Klein, K. G.; Chen, C. H. K.; Matthaeus, W. H.; Szabo, A.; Linton, M.; Allen, R. C.; Szalay, J. R.; Bruno, R.; Decker, R. B.; Akhavan-Tafti, M.; Agapitov, O. V.; Bale, S. D.; Bandyopadhyay, R.; Battams, K.; Bercic, L.; Bourouaine, S.; Bowen, T. A.; Cattell, C.; Chandran, B. D. G.; Chhiber, R.; Cohen, C. M. S.; D'Amicis, R.; Giacalone, J.; Hess, P.; Howard, R. A.; Horbury, T. S.; Jagarlamudi, V. K.; Joyce, C. J.; Kasper, J. C.; Kinnison, J.; Laker, R.; Liewer, P.; Malaspina, D. M.; Mann, I.; McComas, D. J.; Niembro-Hernandez, T.; Nieves-Chinchilla, T.; Panasenco, O.; Pokorný, P.; Pusack, A.; Pulupa, M.; Perez, J. C.; Riley, P.; Rouillard, A. P.; Shi, C.; Stenborg, G.; Tenerani, A.; Verniero, J. L.; Viall, N.; Vourlidas, A.; Wood, B. E.; Woodham, L. D.; Woolley, T. (2023)
    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 ...
  • Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R<sub>?</sub> 
    Badman, S. T.; Riley, P.; Jones, S. I.; Kim, T. K.; Allen, R. C.; Arge, C. N.; Bale, S. D.; Henney, C. J.; Kasper, J. C.; Mostafavi, P.; Pogorelov, N. V.; Raouafi, N. E.; Stevens, M. L.; Verniero, J. L. (2023)
    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 in situ timeseries. Furthermore, making ...
  • Solar Wind Streams and Stream Interaction Regions Observed by the Parker Solar Probe with Corresponding Observations at 1 au 
    Allen, R. C.; Lario, D.; Odstrcil, D.; Ho, G. C.; Jian, L. K.; Cohen, C. M. S.; Badman, S. T.; Jones, S. I.; Arge, C. N.; Mays, M. L.; Mason, G. M.; Bale, S. D.; Bonnell, John W.; Case, Anthony W.; Christian, E. R.; de Wit, T. Dudok; Goetz, K.; Harvey, P. R.; Henney, C. J.; Hill, M. E.; Kasper, Justin C.; Korreck, Kelly E.; Larson, D.; Livi, R.; MacDowall, R. J.; Malaspina, D. M.; McComas, D. J.; McNutt, R.; Mitchell, D. G.; Pulupa, M.; Raouafi, N.; Schwadron, N.; Stevens, Michael L.; Whittlesey, P. L.; Wiedenbeck, M. (2020)
    Several fast solar wind streams and stream interaction regions (SIRs) were observed by the Parker Solar Probe (PSP) during its first orbit (2018 September-2019 January). During this time, several recurring SIRs were also ...
  • Statistical analysis of orientation, shape, and size of solar wind switchbacks 
    Laker, R.; Horbury, T. S.; Bale, S. D.; Matteini, L.; Woolley, T.; Woodham, L. D.; Badman, S. T.; Pulupa, M.; Kasper, Justin C.; Stevens, Michael; Case, Anthony W.; Korreck, Kelly E. (2021)
    Context. One of the main discoveries from the first two orbits of Parker Solar Probe (PSP) was the presence of magnetic switchbacks, whose deflections dominated the magnetic field measurements. Determining their shape and ...

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