dc.contributor.author |
BHATTACHARJEE, DEBESH |
en_US |
dc.contributor.author |
SUBRAMANIAN, PRASAD |
en_US |
dc.contributor.author |
Nieves-Chinchilla, Teresa |
en_US |
dc.contributor.author |
Vourlidas, Angelos |
en_US |
dc.date.accessioned |
2022-11-14T04:05:45Z |
|
dc.date.available |
2022-11-14T04:05:45Z |
|
dc.date.issued |
2023-01 |
en_US |
dc.identifier.citation |
Monthly Notices of the Royal Astronomical Society, 518(1), 1185–1194. |
en_US |
dc.identifier.issn |
1365-2966 |
en_US |
dc.identifier.issn |
0035-8711 |
en_US |
dc.identifier.uri |
https://doi.org/10.1093/mnras/stac3186 |
en_US |
dc.identifier.uri |
http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7451 |
|
dc.description.abstract |
We use in-situ data from the Wind spacecraft to survey the amplitude of turbulent fluctuations in the proton density and total magnetic field inside a large sample of near-Earth magnetic clouds (MCs) associated with coronal mass ejections (CMEs) from the Sun. We find that the most probable value of the modulation index for proton density fluctuations (δnp/np) inside MCs ranges from 0.13 to 0.16, while the most probable values for the modulation index of the total magnetic field fluctuations (δB/B) range from 0.04 to 0.05. We also find that the most probable value of the Mach number fluctuations (δM) inside MCs is ≈0.1. The anomalous resistivity inside near-Earth MCs arising from electron scattering due to turbulent magnetic field fluctuations exceeds the (commonly used) Spitzer resistivity by a factor of ≈500 − 1000. The enhanced Joule heating arising from this anomalous resistivity could impact our understanding of the energetics of CME propagation. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Oxford University Press |
en_US |
dc.subject |
Turbulence, (magnetohydrodynamics) MHD |
en_US |
dc.subject |
Methods: statistical |
en_US |
dc.subject |
Sun: coronal mass ejections (CMEs) |
en_US |
dc.subject |
2022-NOV-WEEK1 |
en_US |
dc.subject |
TOC-NOV-2022 |
en_US |
dc.subject |
2023 |
en_US |
dc.title |
Turbulence and Anomalous Resistivity inside Near-Earth Magnetic Clouds |
en_US |
dc.type |
Article |
en_US |
dc.contributor.department |
Dept. of Physics |
en_US |
dc.identifier.sourcetitle |
Monthly Notices of the Royal Astronomical Society |
en_US |
dc.publication.originofpublisher |
Foreign |
en_US |