Search Results - "Badman, S. T."

Parker Solar Probe Enters the Magnetically Dominated Solar Corona by 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, M, Case, A W, Bale, S D, Maksimovic, M, Moncuquet, M, Goetz, K, Halekas, J S, Malaspina, D, Raouafi, Nour E, Szabo, A, MacDowall, R, Velli, Marco, Dudok de Wit, Thierry, Zank, G P

“…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…”
Get full text

Highly Structured Slow Solar Wind Emerging From an Equatorial Coronal Hole by Bale, S D, Badman, S T, Bonnell, J W, Bowen, T A, Burgess, D, Case, A W, Cattell, C A, Chandran, B D G, Chaston, C C, Chen, C H K, Drake, J. F., Wit, T Dudok de, 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, J C, Kellogg, P J, Klimchuk, J A, Korreck, K 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, Salem, C, Stansby, D, Stevens, M, Szabo, A, Velli, M, Woolley, T, Wygant, J R

“…At solar minimum, the solar wind is observed at high solar latitudes as a predominantly fast (> 500 km/s), highly Alfvenic, rarefied stream of plasma…”
Get full text

Near-Sun In Situ and Remote-sensing Observations of a Coronal Mass Ejection and its Effect on the Heliospheric Current Sheet by Romeo, O. M., Braga, C. R., Badman, S. T., Larson, D. E., Stevens, M. L., Huang, J., Phan, T., Rahmati, A., Livi, R., Alnussirat, S. T., Whittlesey, P. L., Szabo, A., Klein, K. G., Niembro-Hernandez, T., Paulson, K., Verniero, J. L., Lario, D., Raouafi, N. E., Ervin, T., Kasper, J., Pulupa, M., Bale, S. D., Linton, M. G.

“…Abstract During the thirteenth encounter of the Parker Solar Probe (PSP) mission, the spacecraft traveled through a topologically complex interplanetary…”
Get full text

The Evolution of the 1/f Range within a Single Fast-solar-wind Stream between 17.4 and 45.7 Solar Radii by 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

“…Abstract 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…”
Get full text

Searching for a Solar Source of Magnetic-Field Switchbacks in Parker Solar Probe’s First Encounter by de Pablos, D., Samanta, T., Badman, S. T., Schwanitz, C., Bahauddin, S. M., Harra, L. K., Petrie, G., Mac Cormack, C., Mandrini, C. H., Raouafi, N. E., Martinez Pillet, V., Velli, M.

“…Parker Solar Probe observations show ubiquitous magnetic-field reversals closer to the Sun, often referred to as “switchbacks”. The switchbacks have been…”
Get full text

Dispersive Suprathermal Ion Events Observed by the Parker Solar Probe Mission by 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

“…Abstract 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…”
Get full text

A Solar Source of Alfvénic Magnetic Field Switchbacks: In Situ Remnants of Magnetic Funnels on Supergranulation Scales by Bale, S. D., Horbury, T. S., Velli, M., Desai, M. I., Halekas, J. S., McManus, M. D., Panasenco, O., Badman, S. T., Bowen, T. A., Chandran, B. D. G., Drake, J. F., Kasper, J. C., Laker, R., Mallet, A., Matteini, L., Phan, T. D., Raouafi, N. E., Squire, J., Woodham, L. D., Woolley, T.

“…Abstract One of the striking observations from the Parker Solar Probe (PSP) spacecraft is the prevalence in the inner heliosphere of large amplitude, Alfvénic…”
Get full text

Interchange reconnection as the source of the fast solar wind within coronal holes by 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.

“…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…”
Get full text

Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum by 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., Berčič, 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., Pokorný, P., Stenborg, G., Verniero, J. L., Viall, N., Vourlidas, A., Wood, B. E.

“…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…”
Get full text

Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R by 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.

“…Drawing connections between heliospheric spacecraft and solar wind sources is a vital step in understanding the evolution of the solar corona into the solar…”
Get full text

Tracking solar radio bursts using Bayesian multilateration by Cañizares, L. A, Badman, S. T, Maloney, S. A, Owens, M. J, Weigt, D. M, Carley, E. P, Gallagher, P. T

“…Solar radio bursts (SRBs), are emitted by electrons propagating through the corona and interplanetary space. Tracking such bursts is key to understanding the…”
Get full text

The Evolution of the 1/f Range Within a Single Fast-Solar-Wind Stream Between 17.4 and 45.7 Solar Radii by 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

“…The power spectrum of magnetic-field fluctuations in the fast solar wind ($V_{\rm SW}> 500 \mbox{ km} \mbox{ s}^{-1}$) at magnetohydrodynamic (MHD) scales is…”
Get full text

Interchange reconnection as the source of the fast solar wind within coronal holes by 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

“…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…”
Get full text

Sensitivity of solar wind mass flux to coronal temperature by Stansby, D, Berčič, L, Matteini, L, Owen, C. J, French, R, Baker, D, Badman, S. T

“…A&A 650, L2 (2021) Solar wind models predict that the mass flux carried away from the Sun in the solar wind should be extremely sensitive to the temperature in…”
Get full text

The active region source of a type III radio storm observed by Parker Solar Probe during Encounter 2 by Harra, L, Brooks, D. H, Bale, S. D, Mandrini, C. H, Barczynski, K, Sharma, R, Badman, S. T, Dominguez, S. Vargas, Pulupa, M

“…A&A 650, A7 (2021) Context. To investigate the source of a type III radio burst storm during encounter 2 of NASA's Parker Solar Probe (PSP) mission. Aims. It…”
Get full text

Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum by 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, Berčič, L, Bourouaine, S, Bowen, T, 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, 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

“…Space Science Reviews 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…”
Get full text

Constraining Global Coronal Models with Multiple Independent Observables by Badman, Samuel T., Brooks, David H., Poirier, Nicolas, Warren, Harry P., Petrie, Gordon, Rouillard, Alexis P., Nick Arge, C., Bale, Stuart D., de Pablos Agüero, Diego, Harra, Louise, Jones, Shaela I., Kouloumvakos, Athanasios, Riley, Pete, Panasenco, Olga, Velli, Marco, Wallace, Samantha

“…Global coronal models seek to produce an accurate physical representation of the Sun's atmosphere that can be used, for example, to drive space-weather models…”
Get full text

Switchbacks as signatures of magnetic flux ropes generated by interchange reconnection in the corona by Drake, J. F, Agapitov, O, Swisdak, M, Badman, S. T, Bale, S. D, Horbury, T. S, Kasper, Justin C, MacDowall, R. J, Mozer, F. S, Phan, T. D, Pulupa, M, Szabo, A, Velli, M

“…A&A 650, A2 (2021) The structure of magnetic flux ropes injected into the solar wind during reconnection in the coronal atmosphere is explored with…”
Get full text

Energetic Particle Increases Associated with Stream Interaction Regions by Cohen, C. M. S, Christian, E. R, Cummings, A. C, Davis, A. J, Desai, M. I, Giacalone, J, Hill, M. E, Joyce, C. J, Labrador, A. W, Leske, R. A, Matthaeus, W. H, McComas, D. J, McNutt,Jr, R. L, Mewaldt, R. A, Mitchell, D. G, Rankin, J. S, Roelof, E. C, Schwadron, N. A, Stone, E. C, Szalay, J. R, Wiedenbeck, M. E, Allen, R. C, Ho, G. C, Jian, L. K, Lario, D, Odstrcil, D, Bale, S. D, Badman, S. T, Pulupa, M, MacDowall, R. J, Kasper, J. C, Case, A. W, Korreck, K. E, Larson, D. E, Livi, Roberto, Stevens, M. L, Whittlesey, Phyllis

“…The Parker Solar Probe was launched on 2018 August 12 and completed its second orbit on 2019 June 19 with perihelion of 35.7 solar radii. During this time, the…”
Get full text

A solar source of Alfv\'enic magnetic field switchbacks: {\em in situ} remnants of magnetic funnels on supergranulation scales by Bale, S. D, Horbury, T. S, Velli, M, Desai, M. I, Halekas, J. S, McManus, M. D, Panasenco, O, Badman, S. T, Bowen, T. A, Chandran, B. D. G, Drake, J. F, Kasper, J. C, Laker, R, Mallet, A, Matteini, L, Phan, T. D, Raouafi, N. E, Squire, J, Woodham, L. D, Wooley, T

“…One of the striking observations from the Parker Solar Probe (PSP) spacecraft is the prevalence in the inner heliosphere of large amplitude, Alfv\'enic…”
Get full text