New Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe

The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral exponents close to −1 found at the lower frequencies below an inertial range with indices closer to [−1.5, −1.67]. The origi...

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Published inAstrophysical journal. Letters Vol. 950; no. 1; p. L8
Main Authors Huang, Zesen, Sioulas, Nikos, Shi, Chen, Velli, Marco, Bowen, Trevor, Davis, Nooshin, Chandran, B. D. G., Matteini, Lorenzo, Kang, Ning, Shi, Xiaofei, Huang, Jia, Bale, Stuart D., Kasper, J. C., Larson, Davin E., Livi, Roberto, Whittlesey, P. L., Rahmati, Ali, Paulson, Kristoff, Stevens, M., Case, A. W., de Wit, Thierry Dudok, Malaspina, David M., Bonnell, J. W., Goetz, Keith, Harvey, Peter R., MacDowall, Robert J.
Format Journal Article
LanguageEnglish
Published Austin The American Astronomical Society 01.06.2023
IOP Publishing
Bristol : IOP Publishing
Subjects
Advection
Alfven waves
Exponents
Frequency ranges
Heliosphere
Interplanetary turbulence
Magnetohydrodynamics
Power law
Sciences of the Universe
Solar probes
Solar wind
Space plasmas
Spectra
Turbulence
Alfven waves
Heliosphere
Magnetohydrodynamics
Physics - Space Physics
Physics - Fluid Dynamics
Physics - Plasma Physics
Interplanetary turbulence
Physics - Geophysics
Solar wind
Space plasmas
Astrophysics - Solar and Stellar Astrophysics
Online AccessGet full text
ISSN2041-8205
2041-8213
DOI10.3847/2041-8213/acd7f2

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Abstract The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral exponents close to −1 found at the lower frequencies below an inertial range with indices closer to [−1.5, −1.67]. The origin of the 1/ f range is still under debate. In this study, we selected 109 magnetically incompressible solar wind intervals ( δ ∣ B ∣/∣ B ∣ ≪ 1) from Parker Solar Probe encounters 1–13 that display such double power laws, with the aim of understanding the statistics and radial evolution of the low-frequency power spectral exponents from Alfvén point up to 0.3 au. New observations from closer to the Sun show that in the low-frequency range solar wind, turbulence can display spectra much shallower than 1/ f , evolving asymptotically to 1/ f as advection time increases, indicating a dynamic origin for the 1/ f range formation. We discuss the implications of this result on the Matteini et al. conjecture for the 1/ f origin as well as example spectra displaying a triple power law consistent with the model proposed by Chandran et al., supporting the dynamic role of parametric decay in the young solar wind. Our results provide new constraints on the origin of the 1/ f spectrum and further show the possibility of the coexistence of multiple formation mechanisms.
AbstractList The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral exponents close to -1 found at the lower frequencies below an inertial range with indices closer to [-1.5, -1.67]. The origin of the 1/f range is still under debate. In this study, we selected 109 magnetically incompressible solar wind intervals (δ∣ B ∣/∣ B ∣ ≪ 1) from Parker Solar Probe encounters 1-13 that display such double power laws, with the aim of understanding the statistics and radial evolution of the low-frequency power spectral exponents from Alfvén point up to 0.3 au. New observations from closer to the Sun show that in the low-frequency range solar wind, turbulence can display spectra much shallower than 1/f, evolving asymptotically to 1/f as advection time increases, indicating a dynamic origin for the 1/f range formation. We discuss the implications of this result on the Matteini et al. conjecture for the 1/f origin as well as example spectra displaying a triple power law consistent with the model proposed by Chandran et al., supporting the dynamic role of parametric decay in the young solar wind. Our results provide new constraints on the origin of the 1/f spectrum and further show the possibility of the coexistence of multiple formation mechanisms.
The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral exponents close to −1 found at the lower frequencies below an inertial range with indices closer to [−1.5, −1.67]. The origin of the 1/f range is still under debate. In this study, we selected 109 magnetically incompressible solar wind intervals (δ∣B∣/∣B∣ ≪ 1) from Parker Solar Probe encounters 1–13 that display such double power laws, with the aim of understanding the statistics and radial evolution of the low-frequency power spectral exponents from Alfvén point up to 0.3 au. New observations from closer to the Sun show that in the low-frequency range solar wind, turbulence can display spectra much shallower than 1/f, evolving asymptotically to 1/f as advection time increases, indicating a dynamic origin for the 1/f range formation. We discuss the implications of this result on the Matteini et al. conjecture for the 1/f origin as well as example spectra displaying a triple power law consistent with the model proposed by Chandran et al., supporting the dynamic role of parametric decay in the young solar wind. Our results provide new constraints on the origin of the 1/f spectrum and further show the possibility of the coexistence of multiple formation mechanisms.
The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral exponents close to −1 found at the lower frequencies below an inertial range with indices closer to [−1.5, −1.67]. The origin of the 1/ f range is still under debate. In this study, we selected 109 magnetically incompressible solar wind intervals ( δ ∣ B ∣/∣ B ∣ ≪ 1) from Parker Solar Probe encounters 1–13 that display such double power laws, with the aim of understanding the statistics and radial evolution of the low-frequency power spectral exponents from Alfvén point up to 0.3 au. New observations from closer to the Sun show that in the low-frequency range solar wind, turbulence can display spectra much shallower than 1/ f , evolving asymptotically to 1/ f as advection time increases, indicating a dynamic origin for the 1/ f range formation. We discuss the implications of this result on the Matteini et al. conjecture for the 1/ f origin as well as example spectra displaying a triple power law consistent with the model proposed by Chandran et al., supporting the dynamic role of parametric decay in the young solar wind. Our results provide new constraints on the origin of the 1/ f spectrum and further show the possibility of the coexistence of multiple formation mechanisms.
The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral exponents close to −1 found at the lower frequencies below an inertial range with indices closer to [−1.5, −1.67]. The origin of the 1/ f range is still under debate. In this study, we selected 109 magnetically incompressible solar wind intervals ( δ ∣ B ∣/∣ B ∣ ≪ 1) from Parker Solar Probe encounters 1–13 that display such double power laws, with the aim of understanding the statistics and radial evolution of the low-frequency power spectral exponents from Alfvén point up to 0.3 au. New observations from closer to the Sun show that in the low-frequency range solar wind, turbulence can display spectra much shallower than 1/ f , evolving asymptotically to 1/ f as advection time increases, indicating a dynamic origin for the 1/ f range formation. We discuss the implications of this result on the Matteini et al. conjecture for the 1/ f origin as well as example spectra displaying a triple power law consistent with the model proposed by Chandran et al., supporting the dynamic role of parametric decay in the young solar wind. Our results provide new constraints on the origin of the 1/ f spectrum and further show the possibility of the coexistence of multiple formation mechanisms.
Author Harvey, Peter R.
MacDowall, Robert J.
Malaspina, David M.
Shi, Xiaofei
Stevens, M.
Velli, Marco
Larson, Davin E.
Goetz, Keith
Rahmati, Ali
de Wit, Thierry Dudok
Whittlesey, P. L.
Bonnell, J. W.
Kang, Ning
Shi, Chen
Bale, Stuart D.
Huang, Jia
Huang, Zesen
Sioulas, Nikos
Paulson, Kristoff
Davis, Nooshin
Kasper, J. C.
Matteini, Lorenzo
Livi, Roberto
Bowen, Trevor
Chandran, B. D. G.
Case, A. W.
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Cites_doi 10.1063/5.0124703
10.3847/2041-8213/aaabbe
10.1007/s11214-015-0211-6
10.3847/1538-4357/ac0c12
10.1080/03091929108229128
10.1017/S0022377818000016
10.1093/mnras/staa2770
10.1029/JA089iA08p06813
10.3847/1538-4357/aa71b6
10.1103/PhysRevLett.63.1807
10.1051/0004-6361/202039879
10.1063/1.1761412
10.3847/1538-4357/aa9bef
10.1086/588093
10.3847/1538-4357/ac8b81
10.1086/152896
10.1086/426507
10.1103/PhysRevLett.48.1256
10.3847/1538-4357/ac93f5
10.1038/s41586-019-1818-7
10.3847/1538-4357/aaacd6
10.1098/rspa.1938.0032
10.3847/2041-8213/ac2606
10.1103/PhysRevE.76.036305
10.3847/1538-4365/ab9eba
10.3847/1538-4357/ac74c5
10.1051/0004-6361/202039442
10.1109/PROC.1982.12282
10.1088/1674-4527/ac49e4
10.3847/1538-4357/aadb8f
10.1029/JA085iA03p01311
10.1038/s41592-019-0686-2
10.1007/s11214-016-0244-5
10.1029/JA087iA04p02215
10.1103/PhysRevLett.57.495
10.1086/304442
10.3847/2041-8213/acaeff
10.3847/2041-8213/ac51da
10.3847/1538-4357/abebe5
10.1103/PhysRevLett.96.115002
10.1017/S0022377821000970
10.3847/1538-4357/ac7aa2
10.3847/1538-4365/ab53e1
10.1086/174600
10.1103/RevModPhys.58.741
10.3847/2041-8213/ac4a5c
10.1086/175121
10.5281/zenodo.7979740
10.1073/pnas.79.10.3380
10.1051/0004-6361/202039354
10.3847/1538-4365/ab5a84
10.3847/1538-4365/ab5e4b
10.1007/BF00748891
10.1109/MCSE.2007.55
10.1007/s11214-015-0206-3
10.3847/2041-8213/ac36d1
10.1007/s11214-018-0576-4
10.1038/s41586-020-2649-2
10.1145/2833157.2833162
10.1002/2013JA019293
10.1017/S0022377821000167
10.3847/1538-4357/ac7c11
10.3847/1538-4365/ab5853
10.1029/JA078i031p07221
10.1086/431649
10.3847/2041-8213/abf7d1
10.1029/2010GL044806
10.3847/2041-8213/aaf573
10.1086/510710
10.1086/513075
10.1017/S0022377814000579
10.3847/1538-4365/ab60a3
10.1007/BF00151617
10.1086/146579
10.1051/0004-6361/202039818
10.1002/2016JA023345
10.1007/s11214-023-00952-4
10.1051/0004-6361/201935841
10.1103/PhysRevLett.127.255101
10.1088/0004-637X/698/2/986
10.1088/0004-637X/733/2/76
10.3847/2041-8213/abbd4a
10.3847/2041-8213/ac73fd
10.1088/2041-8205/750/2/L33
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Issue 1
Keywords Alfven waves
Heliosphere
Magnetohydrodynamics
Physics - Space Physics
Physics - Fluid Dynamics
Physics - Plasma Physics
Interplanetary turbulence
Physics - Geophysics
Solar wind
Space plasmas
Astrophysics - Solar and Stellar Astrophysics
Language English
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The Sun and the Heliosphere
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References Keshner (apjlacd7f2bib35) 1982; 70
Huang (apjlacd7f2bib30) 2022; 935
Shi (apjlacd7f2bib66) 2021; 650
Huang (apjlacd7f2bib29) 2023
Taylor (apjlacd7f2bib72) 1938; 164
Harris (apjlacd7f2bib26) 2020; 585
Laker (apjlacd7f2bib38) 2021; 650
Zank (apjlacd7f2bib88) 2022; 926
Matteini (apjlacd7f2bib47) 2018; 869
Angelopoulos (apjlacd7f2bib1) 2019; 215
Matteini (apjlacd7f2bib46) 2010; 37
Bale (apjlacd7f2bib2) 2019; 576
Dmitruk (apjlacd7f2bib18) 2007; 76
Burlaga (apjlacd7f2bib12) 1984; 89
Fox (apjlacd7f2bib22) 2016; 204
Bowen (apjlacd7f2bib10) 2018; 854
Mallet (apjlacd7f2bib44) 2021; 918
The Pandas Development Team (apjlacd7f2bib74) 2023
Cuesta (apjlacd7f2bib16) 2022; 932
Sioulas (apjlacd7f2bib69) 2022; 934
Tenerani (apjlacd7f2bib76) 2021; 919
Kasper (apjlacd7f2bib33) 2016; 204
Monin (apjlacd7f2bib53) 1987
Iroshnikov (apjlacd7f2bib32) 1964; 7
Parker (apjlacd7f2bib57) 1958; 128
Sioulas (apjlacd7f2bib70) 2023b
Lam (apjlacd7f2bib39) 2015
Magyar (apjlacd7f2bib42) 2022; 938
Bourouaine (apjlacd7f2bib9) 2020; 904
Cranmer (apjlacd7f2bib15) 2005; 156
Tenerani (apjlacd7f2bib79) 2020; 246
Goldreich (apjlacd7f2bib24) 1995; 438
Réville (apjlacd7f2bib63) 2018; 866
Raouafi (apjlacd7f2bib62) 2023; 219
Telloni (apjlacd7f2bib75) 2021; 912
Virtanen (apjlacd7f2bib85) 2020; 17
Mozer (apjlacd7f2bib55) 2020; 246
Fu (apjlacd7f2bib23) 2018; 855
Podesta (apjlacd7f2bib60) 2009; 698
Whang (apjlacd7f2bib86) 1973; 78
Forman (apjlacd7f2bib21) 2011; 733
Bemporad (apjlacd7f2bib6) 2008; 677
Heinemann (apjlacd7f2bib27) 1980; 85
Shi (apjlacd7f2bib65) 2022a; 29
Boldyrev (apjlacd7f2bib8) 2006; 96
Bale (apjlacd7f2bib3) 2016; 204
Perez (apjlacd7f2bib59) 2021b; 87
Sridhar (apjlacd7f2bib71) 1994; 432
Matthaeus (apjlacd7f2bib49) 1986; 57
Tu (apjlacd7f2bib80) 1995; 73
Martinović (apjlacd7f2bib45) 2021; 912
Bavassano (apjlacd7f2bib5) 1982; 78
Bruno (apjlacd7f2bib11) 2019; 627
Velli (apjlacd7f2bib82) 1991; 62
Pulupa (apjlacd7f2bib61) 2017; 122
Chen (apjlacd7f2bib14) 2020; 246
Matthaeus (apjlacd7f2bib50) 1982; 48
Nakagawa (apjlacd7f2bib56) 1974; 190
Chandran (apjlacd7f2bib13) 2018; 84
Kraichnan (apjlacd7f2bib37) 1965; 8
Montroll (apjlacd7f2bib54) 1982; 79
Kolmogorov (apjlacd7f2bib36) 1941; 30
Hernández (apjlacd7f2bib28) 2020; 922
Livi (apjlacd7f2bib41) 2022; 938
Tenerani (apjlacd7f2bib77) 2013; 118
Perez (apjlacd7f2bib58) 2021a; 650
Boldyrev (apjlacd7f2bib7) 2005; 626
Kasper (apjlacd7f2bib34) 2021; 127
Shi (apjlacd7f2bib67) 2017; 842
Meng (apjlacd7f2bib51) 2022; 22
Verdini (apjlacd7f2bib83) 2012; 750
Verdini (apjlacd7f2bib84) 2007; 662
Hunter (apjlacd7f2bib31) 2007; 9
Mallet (apjlacd7f2bib43) 2021; 87
Dudok de Wit (apjlacd7f2bib19) 2020; 246
Taylor (apjlacd7f2bib73) 1986; 58
Farrell (apjlacd7f2bib20) 2020; 249
Bandyopadhyay (apjlacd7f2bib4) 2022; 926
Denskat (apjlacd7f2bib17) 1982; 87
Shi (apjlacd7f2bib64) 2022b; 934
Larosa (apjlacd7f2bib40) 2021; 650
Tenerani (apjlacd7f2bib78) 2017; 851
Moncuquet (apjlacd7f2bib52) 2020; 246
Velli (apjlacd7f2bib81) 1989; 63
Zanna (apjlacd7f2bib89) 2015; 81
Woolley (apjlacd7f2bib87) 2020; 498
Goldreich (apjlacd7f2bib25) 1997; 485
Matthaeus (apjlacd7f2bib48) 2007; 657
Sioulas (apjlacd7f2bib68) 2023a; 943
References_xml – volume: 29
  year: 2022a
  ident: apjlacd7f2bib65
  publication-title: PhPl
  doi: 10.1063/5.0124703
– volume: 854
  start-page: L33
  year: 2018
  ident: apjlacd7f2bib10
  publication-title: ApJL
  doi: 10.3847/2041-8213/aaabbe
– volume: 204
  start-page: 7
  year: 2016
  ident: apjlacd7f2bib22
  publication-title: SSRv
  doi: 10.1007/s11214-015-0211-6
– volume: 918
  start-page: 62
  year: 2021
  ident: apjlacd7f2bib44
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac0c12
– volume: 62
  start-page: 101
  year: 1991
  ident: apjlacd7f2bib82
  publication-title: GApFD
  doi: 10.1080/03091929108229128
– volume: 84
  start-page: 905840106
  year: 2018
  ident: apjlacd7f2bib13
  publication-title: JPlPh
  doi: 10.1017/S0022377818000016
– volume: 498
  start-page: 5524
  year: 2020
  ident: apjlacd7f2bib87
  publication-title: MNRAS
  doi: 10.1093/mnras/staa2770
– volume: 89
  start-page: 6813
  year: 1984
  ident: apjlacd7f2bib12
  publication-title: JGRA
  doi: 10.1029/JA089iA08p06813
– volume: 842
  start-page: 63
  year: 2017
  ident: apjlacd7f2bib67
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa71b6
– volume: 63
  start-page: 1807
  year: 1989
  ident: apjlacd7f2bib81
  publication-title: PhRvL
  doi: 10.1103/PhysRevLett.63.1807
– volume: 650
  start-page: A22
  year: 2021a
  ident: apjlacd7f2bib58
  publication-title: A&A
  doi: 10.1051/0004-6361/202039879
– volume: 8
  start-page: 1385
  year: 1965
  ident: apjlacd7f2bib37
  publication-title: PhFl
  doi: 10.1063/1.1761412
– volume: 851
  start-page: 99
  year: 2017
  ident: apjlacd7f2bib78
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa9bef
– volume: 677
  start-page: L137
  year: 2008
  ident: apjlacd7f2bib6
  publication-title: ApJL
  doi: 10.1086/588093
– volume: 938
  start-page: 98
  year: 2022
  ident: apjlacd7f2bib42
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac8b81
– volume: 190
  start-page: 441
  year: 1974
  ident: apjlacd7f2bib56
  publication-title: ApJ
  doi: 10.1086/152896
– year: 2023
  ident: apjlacd7f2bib29
– volume: 156
  start-page: 265
  year: 2005
  ident: apjlacd7f2bib15
  publication-title: ApJS
  doi: 10.1086/426507
– volume: 48
  start-page: 1256
  year: 1982
  ident: apjlacd7f2bib50
  publication-title: PhRvL
  doi: 10.1103/PhysRevLett.48.1256
– volume: 938
  start-page: 138
  year: 2022
  ident: apjlacd7f2bib41
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac93f5
– volume: 576
  start-page: 237
  year: 2019
  ident: apjlacd7f2bib2
  publication-title: Natur
  doi: 10.1038/s41586-019-1818-7
– volume: 855
  start-page: 139
  year: 2018
  ident: apjlacd7f2bib23
  publication-title: ApJ
  doi: 10.3847/1538-4357/aaacd6
– volume: 164
  start-page: 476
  year: 1938
  ident: apjlacd7f2bib72
  publication-title: RSPSA
  doi: 10.1098/rspa.1938.0032
– volume: 919
  start-page: L31
  year: 2021
  ident: apjlacd7f2bib76
  publication-title: ApJL
  doi: 10.3847/2041-8213/ac2606
– volume: 76
  start-page: 036305
  year: 2007
  ident: apjlacd7f2bib18
  publication-title: PhRvE
  doi: 10.1103/PhysRevE.76.036305
– volume: 249
  start-page: 28
  year: 2020
  ident: apjlacd7f2bib20
  publication-title: ApJS
  doi: 10.3847/1538-4365/ab9eba
– volume: 935
  start-page: 60
  year: 2022
  ident: apjlacd7f2bib30
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac74c5
– volume: 650
  start-page: A3
  year: 2021
  ident: apjlacd7f2bib40
  publication-title: A&A
  doi: 10.1051/0004-6361/202039442
– volume: 70
  start-page: 212
  year: 1982
  ident: apjlacd7f2bib35
  publication-title: IEEEP
  doi: 10.1109/PROC.1982.12282
– volume: 22
  start-page: 035018
  year: 2022
  ident: apjlacd7f2bib51
  publication-title: RAA
  doi: 10.1088/1674-4527/ac49e4
– volume: 866
  start-page: 38
  year: 2018
  ident: apjlacd7f2bib63
  publication-title: ApJ
  doi: 10.3847/1538-4357/aadb8f
– volume: 85
  start-page: 1311
  year: 1980
  ident: apjlacd7f2bib27
  publication-title: JGRA
  doi: 10.1029/JA085iA03p01311
– volume: 17
  start-page: 261
  year: 2020
  ident: apjlacd7f2bib85
  publication-title: NatMe
  doi: 10.1038/s41592-019-0686-2
– volume: 204
  start-page: 49
  year: 2016
  ident: apjlacd7f2bib3
  publication-title: SSSRv
  doi: 10.1007/s11214-016-0244-5
– volume: 87
  start-page: 2215
  year: 1982
  ident: apjlacd7f2bib17
  publication-title: JGRA
  doi: 10.1029/JA087iA04p02215
– volume: 30
  start-page: 301
  year: 1941
  ident: apjlacd7f2bib36
  publication-title: DoSSR
– volume: 57
  start-page: 495
  year: 1986
  ident: apjlacd7f2bib49
  publication-title: PhRvL
  doi: 10.1103/PhysRevLett.57.495
– volume: 485
  start-page: 680
  year: 1997
  ident: apjlacd7f2bib25
  publication-title: ApJ
  doi: 10.1086/304442
– volume: 943
  start-page: L8
  year: 2023a
  ident: apjlacd7f2bib68
  publication-title: ApJL
  doi: 10.3847/2041-8213/acaeff
– volume: 926
  start-page: L16
  year: 2022
  ident: apjlacd7f2bib88
  publication-title: ApJL
  doi: 10.3847/2041-8213/ac51da
– volume: 912
  start-page: 28
  year: 2021
  ident: apjlacd7f2bib45
  publication-title: ApJ
  doi: 10.3847/1538-4357/abebe5
– volume: 96
  start-page: 115002
  year: 2006
  ident: apjlacd7f2bib8
  publication-title: PhRvL
  doi: 10.1103/PhysRevLett.96.115002
– volume: 87
  start-page: 175870601
  year: 2021
  ident: apjlacd7f2bib43
  publication-title: JPlPh
  doi: 10.1017/S0022377821000970
– volume: 934
  start-page: 143
  year: 2022
  ident: apjlacd7f2bib69
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac7aa2
– volume: 246
  start-page: 32
  year: 2020
  ident: apjlacd7f2bib79
  publication-title: ApJS
  doi: 10.3847/1538-4365/ab53e1
– volume: 432
  start-page: 612
  year: 1994
  ident: apjlacd7f2bib71
  publication-title: ApJ
  doi: 10.1086/174600
– volume: 58
  start-page: 741
  year: 1986
  ident: apjlacd7f2bib73
  publication-title: RvMP
  doi: 10.1103/RevModPhys.58.741
– volume: 926
  start-page: L1
  year: 2022
  ident: apjlacd7f2bib4
  publication-title: ApJL
  doi: 10.3847/2041-8213/ac4a5c
– volume: 438
  start-page: 763
  year: 1995
  ident: apjlacd7f2bib24
  publication-title: ApJ
  doi: 10.1086/175121
– year: 2023
  ident: apjlacd7f2bib74
  doi: 10.5281/zenodo.7979740
– volume: 79
  start-page: 3380
  year: 1982
  ident: apjlacd7f2bib54
  publication-title: PNAS
  doi: 10.1073/pnas.79.10.3380
– volume: 650
  start-page: A1
  year: 2021
  ident: apjlacd7f2bib38
  publication-title: A&A
  doi: 10.1051/0004-6361/202039354
– volume: 246
  start-page: 44
  year: 2020
  ident: apjlacd7f2bib52
  publication-title: ApJS
  doi: 10.3847/1538-4365/ab5a84
– volume: 246
  start-page: 50
  year: 2020
  ident: apjlacd7f2bib55
  publication-title: ApJS
  doi: 10.3847/1538-4365/ab5e4b
– year: 2023b
  ident: apjlacd7f2bib70
– volume: 73
  start-page: 1
  year: 1995
  ident: apjlacd7f2bib80
  publication-title: SSRv
  doi: 10.1007/BF00748891
– volume: 9
  start-page: 90
  year: 2007
  ident: apjlacd7f2bib31
  publication-title: CSE
  doi: 10.1109/MCSE.2007.55
– volume: 204
  start-page: 131
  year: 2016
  ident: apjlacd7f2bib33
  publication-title: SSRv
  doi: 10.1007/s11214-015-0206-3
– volume: 922
  start-page: L11
  year: 2020
  ident: apjlacd7f2bib28
  publication-title: ApJL
  doi: 10.3847/2041-8213/ac36d1
– volume: 215
  start-page: 9
  year: 2019
  ident: apjlacd7f2bib1
  publication-title: SSRv
  doi: 10.1007/s11214-018-0576-4
– volume: 585
  start-page: 357
  year: 2020
  ident: apjlacd7f2bib26
  publication-title: Natur
  doi: 10.1038/s41586-020-2649-2
– start-page: 1
  year: 2015
  ident: apjlacd7f2bib39
  doi: 10.1145/2833157.2833162
– volume: 118
  start-page: 7507
  year: 2013
  ident: apjlacd7f2bib77
  publication-title: JGRA
  doi: 10.1002/2013JA019293
– volume: 87
  year: 2021b
  ident: apjlacd7f2bib59
  publication-title: JPlPh
  doi: 10.1017/S0022377821000167
– volume: 934
  start-page: 152
  year: 2022b
  ident: apjlacd7f2bib64
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac7c11
– volume: 246
  start-page: 39
  year: 2020
  ident: apjlacd7f2bib19
  publication-title: ApJS
  doi: 10.3847/1538-4365/ab5853
– volume: 78
  start-page: 7221
  year: 1973
  ident: apjlacd7f2bib86
  publication-title: JGR
  doi: 10.1029/JA078i031p07221
– volume: 626
  start-page: L37
  year: 2005
  ident: apjlacd7f2bib7
  publication-title: ApJL
  doi: 10.1086/431649
– volume: 912
  start-page: L21
  year: 2021
  ident: apjlacd7f2bib75
  publication-title: ApJL
  doi: 10.3847/2041-8213/abf7d1
– volume: 37
  year: 2010
  ident: apjlacd7f2bib46
  publication-title: GeoRL
  doi: 10.1029/2010GL044806
– volume: 869
  start-page: L32
  year: 2018
  ident: apjlacd7f2bib47
  publication-title: ApJL
  doi: 10.3847/2041-8213/aaf573
– volume: 662
  start-page: 669
  year: 2007
  ident: apjlacd7f2bib84
  publication-title: ApJ
  doi: 10.1086/510710
– volume: 657
  start-page: L121
  year: 2007
  ident: apjlacd7f2bib48
  publication-title: ApJL
  doi: 10.1086/513075
– volume: 81
  start-page: 325810102
  year: 2015
  ident: apjlacd7f2bib89
  publication-title: JPlPh
  doi: 10.1017/S0022377814000579
– volume: 246
  start-page: 53
  year: 2020
  ident: apjlacd7f2bib14
  publication-title: ApJS
  doi: 10.3847/1538-4365/ab60a3
– volume: 78
  start-page: 373
  year: 1982
  ident: apjlacd7f2bib5
  publication-title: SoPh
  doi: 10.1007/BF00151617
– volume: 128
  start-page: 664
  year: 1958
  ident: apjlacd7f2bib57
  publication-title: ApJ
  doi: 10.1086/146579
– volume: 650
  start-page: A21
  year: 2021
  ident: apjlacd7f2bib66
  publication-title: A&A
  doi: 10.1051/0004-6361/202039818
– volume: 122
  start-page: 2836
  year: 2017
  ident: apjlacd7f2bib61
  publication-title: JGRA
  doi: 10.1002/2016JA023345
– volume: 219
  start-page: 8
  year: 2023
  ident: apjlacd7f2bib62
  publication-title: SSRv
  doi: 10.1007/s11214-023-00952-4
– volume: 627
  start-page: A96
  year: 2019
  ident: apjlacd7f2bib11
  publication-title: A&A
  doi: 10.1051/0004-6361/201935841
– year: 1987
  ident: apjlacd7f2bib53
– volume: 127
  start-page: 255101
  year: 2021
  ident: apjlacd7f2bib34
  publication-title: PhRvL
  doi: 10.1103/PhysRevLett.127.255101
– volume: 7
  start-page: 566
  year: 1964
  ident: apjlacd7f2bib32
  publication-title: SvA
– volume: 698
  start-page: 986
  year: 2009
  ident: apjlacd7f2bib60
  publication-title: ApJ
  doi: 10.1088/0004-637X/698/2/986
– volume: 733
  start-page: 76
  year: 2011
  ident: apjlacd7f2bib21
  publication-title: ApJ
  doi: 10.1088/0004-637X/733/2/76
– volume: 904
  start-page: L30
  year: 2020
  ident: apjlacd7f2bib9
  publication-title: ApJL
  doi: 10.3847/2041-8213/abbd4a
– volume: 932
  start-page: L11
  year: 2022
  ident: apjlacd7f2bib16
  publication-title: ApJL
  doi: 10.3847/2041-8213/ac73fd
– volume: 750
  start-page: L33
  year: 2012
  ident: apjlacd7f2bib83
  publication-title: ApJL
  doi: 10.1088/2041-8205/750/2/L33
SSID ssj0020618
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Snippet The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with...
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StartPage L8
SubjectTerms Advection
Alfven waves
Exponents
Frequency ranges
Heliosphere
Interplanetary turbulence
Magnetohydrodynamics
Power law
Sciences of the Universe
Solar probes
Solar wind
Space plasmas
Spectra
Turbulence
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Title New Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe
URI https://iopscience.iop.org/article/10.3847/2041-8213/acd7f2
https://www.proquest.com/docview/2825212493
https://insu.hal.science/insu-04151711
https://doaj.org/article/33c34356d4694432afa015931f33dbf6
Volume 950
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