Terrestrial (WSO) & L1 space (WIND) MAG data for detection of Sun's 2002 global shutdown-superflaring response to failed star Jupiter's 1996 switch to a recurrent pulsar phase

Citation Author(s):
Mensur
Omerbashich
Geophysics Online
Submitted by:
Mensur Omerbashich
Last updated:
Sat, 12/07/2024 - 17:50
DOI:
10.21227/cv28-8929
Data Format:
.txt
Research Article Link:
Sun superflaring mechanism from decade-scale magnetic entanglement with Jupiter
License:
Creative Commons Attribution
111 Views
Categories:
Astronomy
Keywords:
Time series analysis, least squares, spectral analysis, solar data, astronomy, Astrophysics, solar wind, solar wind macroscopic dynamics, solar superflaring, solar-type stars, WIND space mission, WSO mean solar magnetic field, planetary pulsars
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Abstract 

The WSO (Wilcox Solar Observatory at Stanford University) terrestrial observatory data, spanning 47 years of solar Mean Magnetic Field (MMF) values. The set also includes data from the WIND space mission's magnetometer (MAG), collected at the L1 Lagrangian point over the time interval of 27 years. The least-squares spectral analysis scientific software LSSA, based on the rigorous method by Vanicek (1969: https://doi.org/10.1007/BF00651344, 1971: https://doi.org/10.1007/BF00656134), was used to compute spectra. LSSA v.5 is available as an open-source version from http://www2.unb.ca/gge/Research/GRL/LSSA/sourceCode.html.

Instructions: 

Data for: Omerbashich, M. (2024) Sun superflaring mechanism from decade-scale magnetic entanglement with Jupiter.

- The WSO data are diurnal averages in microT, source: http://wso.stanford.edu/#MeanField
- The WIND data are hourly averages in nT, Source: https://cdaweb.gsfc.nasa.gov/pub/data/wind/mfi/ascii
- Time series have arbitrary temporal datums.

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