Connecting solar wind turbulence to plasma parameters at L1 using multi-spacecraft coherence

Pelkum Donahue, K.; Inceoglu, F.

doi:10.1051/0004-6361/202557052

i

Connecting solar wind turbulence to plasma parameters at L1 using multi-spacecraft coherence

2026
By Pelkum Donahue, K. ; Inceoglu, F.

Details

Journal Title:

Astronomy & Astrophysics
Personal Author:

Pelkum Donahue, K. ; Inceoglu, F.
NOAA Program & Office:

NESDIS (National Environmental Satellite, Data, and Information Service) ; OAR (Oceanic and Atmospheric Research) ; CIRES (Cooperative Institute for Research in Environmental Sciences) ; NCEI (National Centers for Environmental Information)
Description:

Solar wind propagation behavior has significant implications for solar wind forecasting and measurements. Variability in coherence and plasma turbulence under different plasma conditions is important for cross-satellite comparisons. Forecasting also depends on whether upstream measurements remain valid at the magnetosphere.
Source:

Astronomy & Astrophysics, 705, A133
DOI:

https://doi.org/10.1051/0004-6361/202557052
ISSN:

0004-6361 ; 1432-0746
Format:

PDF
Publisher:

EDP Sciences
Document Type:

Journal Article
Funding:

Grant no. NA17OAR4320101 ; Grant no. NA22OAR4320151
License:

https://creativecommons.org/licenses/by/4.0/
Rights Information:

CC BY
Compliance:

Submitted
Main Document Checksum:

urn:sha-512:86d2c41afb665ab4b617574877f8b33ddfcfa75119562f67b81e7518f11cd7072d163a7fd8cf09459ddc17615c29ab81e4986a73e9fb818290e4e631fc32fbc7
Download URL:

https://repository.library.noaa.gov/view/noaa/73547/noaa_73547_DS1.pdf
File Type:

[PDF - 3.80 MB ]

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