TY - JOUR
T1 - Origins of Persistence in Energetic Neutral Atom Time Series from IBEX
AU - Sarlis, N. V.
AU - Livadiotis, G.
AU - McComas, D. J.
AU - Alimaganbetov, M.
AU - Schwadron, N. A.
N1 - Publisher Copyright:
© 2025. The Author(s). Published by the American Astronomical Society.
PY - 2025/6/20
Y1 - 2025/6/20
N2 - Recently, we studied the persistence of energetic neutral atom (ENA) fluxes recorded by the Interstellar Boundary Explorer (IBEX) from the north and south polar regions by examining the correct time order for the 14 yr of IBEX data. Here, we further explore the origins of this persistence by comparing the time series of the ENA fluxes obtained from the near-Earth with the time series of the solar wind flow pressure at 1 au. To this end, we employ the detrended fluctuation analysis (DFA), a modern technique for characterizing the persistence of a time series. We show that even when removing all periodic trends from the flux time series, the remaining fluctuations exhibit DFA exponents compatible with those found for the solar wind pressure time series, indicating a causal relation between the two time series. The analysis was performed separately for the north and south poles, characterizing their anisotropy. Finally, we apply the DFA technique to the ENA time series of the polar spectral indices, an exponent related to the thermodynamic kappa and the stationary state of the source protons. This reveals that the plasma proton thermodynamics in both north and south polar regions share the same DFA persistence, despite the hemispheric asymmetry between the generated ENAs.
AB - Recently, we studied the persistence of energetic neutral atom (ENA) fluxes recorded by the Interstellar Boundary Explorer (IBEX) from the north and south polar regions by examining the correct time order for the 14 yr of IBEX data. Here, we further explore the origins of this persistence by comparing the time series of the ENA fluxes obtained from the near-Earth with the time series of the solar wind flow pressure at 1 au. To this end, we employ the detrended fluctuation analysis (DFA), a modern technique for characterizing the persistence of a time series. We show that even when removing all periodic trends from the flux time series, the remaining fluctuations exhibit DFA exponents compatible with those found for the solar wind pressure time series, indicating a causal relation between the two time series. The analysis was performed separately for the north and south poles, characterizing their anisotropy. Finally, we apply the DFA technique to the ENA time series of the polar spectral indices, an exponent related to the thermodynamic kappa and the stationary state of the source protons. This reveals that the plasma proton thermodynamics in both north and south polar regions share the same DFA persistence, despite the hemispheric asymmetry between the generated ENAs.
UR - https://www.scopus.com/pages/publications/105008473800
UR - https://www.scopus.com/pages/publications/105008473800#tab=citedBy
U2 - 10.3847/1538-4357/addb4a
DO - 10.3847/1538-4357/addb4a
M3 - Article
AN - SCOPUS:105008473800
SN - 0004-637X
VL - 986
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 131
ER -