Measures of Scale-dependent Alfvénicity in the First PSP Solar Encounter

dc.contributor.authorParashar, T. N.
dc.contributor.authorGoldstein, Melvyn
dc.contributor.authorMaruca, B. A.
dc.contributor.authorMatthaeus, W. H.
dc.contributor.authoret al
dc.date.accessioned2022-08-24T20:43:04Z
dc.date.available2022-08-24T20:43:04Z
dc.date.issued2020-02-03
dc.descriptionAuthors: T. N. Parashar, Melvyn Goldstein, B. A. Maruca, W. H. Matthaeus, D. Ruffolo, R. Bandyopadhyay, R. Chhiber, A. Chasapis, R. Qudsi, D. Vech, D. A. Roberts, S. D. Bale, J. W. Bonnell, T. Dudok de Wit, K. Goetz, P. R. Harvey, R. J. MacDowall, D. Malaspina, M. Pulupa, J. C. Kasper, K. E. Korreck, A. W. Case, M. Stevens, P. Whittlesey, D. Larson, R. Livi, M. Velli, and N. Raouafien_US
dc.description.abstractThe solar wind shows periods of highly Alfvénic activity, where velocity fluctuations and magnetic fluctuations are aligned or antialigned with each other. It is generally agreed that solar wind plasma velocity and magnetic field fluctuations observed by the Parker Solar Probe (PSP) during the first encounter are mostly highly Alfvénic. However, quantitative measures of Alfvénicity are needed to understand how the characterization of these fluctuations compares with standard measures from prior missions in the inner and outer heliosphere, in fast wind and slow wind, and at high and low latitudes. To investigate this issue, we employ several measures to quantify the extent of Alfvénicity—the Alfvén ratio rA, the normalized cross helicity σc, the normalized residual energy σr, and the cosine of angle between velocity and magnetic fluctuations $\cos {\theta }_{{vb}}$. We show that despite the overall impression that the Alfvénicity is large in the solar wind sampled by PSP during the first encounter, during some intervals the cross helicity starts decreasing at very large scales. These length scales (often >1000di) are well inside inertial range, and therefore, the suppression of cross helicity at these scales cannot be attributed to kinetic physics. This drop at large scales could potentially be explained by large scale shears present in the inner heliosphere sampled by PSP. In some cases, despite the cross helicity being constant down to the noise floor, the residual energy decreases with scale in the inertial range. These results suggest that it is important to consider all these measures to quantify Alfvénicity.en_US
dc.description.sponsorshipThe authors acknowledge useful discussions with Chris Chen. This research as been supported in part by the Parker Solar Probe mission under the ISʘIS project (contract NNN06AA01C) and a subcontract to University of Delaware from Princeton University (SUB0000165). Additional support is acknowledged from the NASA LWS program (NNX17AB79G), the HSR program (80NSSC18K1210 and 80NSSC18K1648), NASA HGI program (80NSSC19K0284), and grant RTA6280002 from Thailand Science Research and Innovation. D.V. was supported by NASA's Future Investigators in NASA Earth and Space Science and Technology Program Grant (80NSSC19K1430). Parker Solar Probe was designed, built, and is now operated by the Johns Hopkins Applied Physics Laboratory as part of NASA's Living with a Star (LWS) program (contract NNN06AA01C). Support from the LWS management and technical team has played a critical role in the success of the Parker Solar Probe mission.en_US
dc.description.urihttps://iopscience.iop.org/article/10.3847/1538-4365/ab64e6en_US
dc.format.extent8 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2lozl-qvbk
dc.identifier.citation“Measures of Scale Dependent Alfvénicity in the First PSP Encounter, T.N. Parashar, Melvyn L. Goldstein, B.A. Maruca, W.H. Matthaeus, D. Ruffolo, Riddhi Bandyopadhyay, R. Chhiber, A. Chasapis, R. Qudsi, D.A. Roberts, S.D. Bale, W. Bonnell, T. Dudok de Wit, K. Goetz, P.R. Harvey, R.J. MacDowall, D. Malaspina, M. Pulupa, J.C. Kasper, K.E. Korreck, A.W. Case, M. Stevens, P. Whittlesey, D. Larson, R. Livi, M. Velli, and N. Raouafi, The Astrophys. J. Suppl. Series, 246:58, https://doi.org/10.3847/1538-4365/ab64e6.en_US
dc.identifier.urihttps://doi.org/10.3847/1538-4365/ab64e6
dc.identifier.urihttp://hdl.handle.net/11603/25558
dc.language.isoen_USen_US
dc.publisherAASen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.*
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleMeasures of Scale-dependent Alfvénicity in the First PSP Solar Encounteren_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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