@article{Telloni:2021:2041-8213/abf7d1,
author = {Telloni, D and Sorriso-Valvo, L and Woodham, LD and Panasenco, O and Velli, M and Carbone, F and Zank, GP and Bruno, R and Perrone, D and Nakanotani, M and Shi, C and D'Amicis, R and De, Marco R and Jagarlamudi, VK and Steinvall, K and Marino, R and Adhikari, L and Zhao, L and Liang, H and Tenerani, A and Laker, R and Horbury, TS and Bale, SD and Pulupa, M and Malaspina, DM and MacDowall, RJ and Goetz, K and de, Wit TD and Harvey, PR and Kasper, JC and Korreck, KE and Larson, D and Case, AW and Stevens, ML and Whittlesey, P and Livi, R and Owen, CJ and Livi, S and Louarn, P and Antonucci, E and Romoli, M and O'Brien, H and Evans, V and Angelini, V},
doi = {2041-8213/abf7d1},
journal = {Letters of the Astrophysical Journal},
pages = {1--8},
title = {Evolution of solar wind turbulence from 0.1 to 1 au during the first parker solar probe-solar orbiter radial alignment},
url = {http://dx.doi.org/10.3847/2041-8213/abf7d1},
volume = {912},
year = {2021}
}

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TY  - JOUR
AB  - The first radial alignment between Parker Solar Probe and Solar Orbiter spacecraft is used to investigate the evolution of solar wind turbulence in the inner heliosphere. Assuming ballistic propagation, two 1.5 hr intervals are tentatively identified as providing measurements of the same plasma parcels traveling from 0.1 to 1 au. Using magnetic field measurements from both spacecraft, the properties of turbulence in the two intervals are assessed. Magnetic spectral density, flatness, and high-order moment scaling laws are calculated. The Hilbert–Huang transform is additionally used to mitigate short sample and poor stationarity effects. Results show that the plasma evolves from a highly Alfvénic, less-developed turbulence state near the Sun, to fully developed and intermittent turbulence at 1 au. These observations provide strong evidence for the radial evolution of solar wind turbulence.
AU  - Telloni,D
AU  - Sorriso-Valvo,L
AU  - Woodham,LD
AU  - Panasenco,O
AU  - Velli,M
AU  - Carbone,F
AU  - Zank,GP
AU  - Bruno,R
AU  - Perrone,D
AU  - Nakanotani,M
AU  - Shi,C
AU  - D'Amicis,R
AU  - De,Marco R
AU  - Jagarlamudi,VK
AU  - Steinvall,K
AU  - Marino,R
AU  - Adhikari,L
AU  - Zhao,L
AU  - Liang,H
AU  - Tenerani,A
AU  - Laker,R
AU  - Horbury,TS
AU  - Bale,SD
AU  - Pulupa,M
AU  - Malaspina,DM
AU  - MacDowall,RJ
AU  - Goetz,K
AU  - de,Wit TD
AU  - Harvey,PR
AU  - Kasper,JC
AU  - Korreck,KE
AU  - Larson,D
AU  - Case,AW
AU  - Stevens,ML
AU  - Whittlesey,P
AU  - Livi,R
AU  - Owen,CJ
AU  - Livi,S
AU  - Louarn,P
AU  - Antonucci,E
AU  - Romoli,M
AU  - O'Brien,H
AU  - Evans,V
AU  - Angelini,V
DO  - 2041-8213/abf7d1
EP  - 8
PY  - 2021///
SN  - 2041-8205
SP  - 1
TI  - Evolution of solar wind turbulence from 0.1 to 1 au during the first parker solar probe-solar orbiter radial alignment
T2  - Letters of the Astrophysical Journal
UR  - http://dx.doi.org/10.3847/2041-8213/abf7d1
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000648772000001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - https://iopscience.iop.org/article/10.3847/2041-8213/abf7d1
UR  - http://hdl.handle.net/10044/1/89346
VL  - 912
ER  - 

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