N-S separated 1994–2008 Ulysses data of polar (fast) solar winds for detection of the Sun global Alfven resonance, hourly averaged

Citation Author(s):
Mensur
Omerbashich
Submitted by:
Mensur Omerbashich
Last updated:
Tue, 02/14/2023 - 13:25
DOI:
10.21227/dqkp-3040
Data Format:
*.avi; *.csv; *.txt; *.zip
Link to Paper:
First total recovery of Sun global Alfven resonance reveals solar-type stars act as revolving-field magnetoalternators. arXiv
License:
Creative Commons Attribution
357 Views
Categories:
Astronomy
Keywords:
Time series analysis, least squares, spectral analysis, solar data, astronomy, solar wind, solar vibrations, solar-type stars, Ulysses space mission, WIND space mission, WSO mean solar magnetic field, WSO polar solar magnetic field
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Abstract 

North/South-separated <10nT magnetometer data from the 1994-2008 Ulysses space mission's samplings of polar (fast) solar winds, hourly averaged, non-decimated. The set also includes data from the WIND space mission, the WSO terrestrial observatory (solar Mean Magnetic Field), and the WSO solar Polar magnetic Field, all used in the same research project.

Instructions: 

Data for: Omerbashich, M. (2022) Sun global Alfvén resonance from decade-scale dynamics of N–S separated fast solar wind.

- The data are daily averages, except for Ulysses for which data are hourly averages (not decimated).
- Time series have different (arbitrary) temporal datums per data source (WSO MMF, WSO PF, ULYSSES, WIND).
- NS-combined and respective N- and S-separated time series have a common origin.

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