Solar Wind In Situ Data Suitable For Machine Learning (python Numpy Structured Arrays): STEREO-A/B, Wind, Parker Solar Probe, Ulysses, Venus Express, MESSENGER - Info and Reading Options
By Christian Moestl, Andreas Weiss, Rachel Bailey, Alexey Isavnin and David Stansby
“Solar Wind In Situ Data Suitable For Machine Learning (python Numpy Structured Arrays): STEREO-A/B, Wind, Parker Solar Probe, Ulysses, Venus Express, MESSENGER” Metadata:
- Title: ➤ Solar Wind In Situ Data Suitable For Machine Learning (python Numpy Structured Arrays): STEREO-A/B, Wind, Parker Solar Probe, Ulysses, Venus Express, MESSENGER
- Authors: Christian MoestlAndreas WeissRachel BaileyAlexey IsavninDavid Stansby
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- Internet Archive ID: figshare.com-12058065-v5
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"Solar Wind In Situ Data Suitable For Machine Learning (python Numpy Structured Arrays): STEREO-A/B, Wind, Parker Solar Probe, Ulysses, Venus Express, MESSENGER" Description:
The Internet Archive:
<div>These are solar wind in situ data arrays in python pickle format suitable for machine learning, i.e. the arrays consist only of numbers, no strings and no datetime objects.<br /></div><div><br /></div><div>See AAREADME_insitu_ML.txt for more explanation.</div><div><br /></div><div>If you use these data for peer reviewed scientific publications, please get in touch concerning usage and possible co-authorship by the authors (C. Möstl, A. J. Weiss, R. L. Bailey, A. Isavnin, D. Stansby): [email protected] or twitter @chrisoutofspace </div><div><br /></div><div>Made with https://github.com/cmoestl/heliocats <br /></div><div><br /></div><div>Load in python with e.g. for Parker Solar Probe data:</div><div><br /></div><div>> import pickle</div><div>> filepsp='psp_2018_2019_sceq_ndarray.p'</div><div>> [psp,hpsp]=pickle.load(open(filepsp, "rb" ) ) </div><div><br /></div><div>plot time vs total field</div><div>> import matplotlib.pyplot as plt</div><div>> plt.plot(psp['time'],psp['bt'])<br /></div><div><br /></div><div>Times psp[:,0 ] or psp['time'] are in matplotlib format.</div><div> </div><div>Variable 'hpsp' contains a header with the variable names and units for each column. Coordinate systems for magnetic field components are RTN (Ulysses), SCEQ (Parker Solar Probe, STEREO-A/B, VEX, MESSENGER), HEEQ (Wind)</div><div><br /></div><div>available parameters:</div><div><br /></div><div>bt = total magnetic field</div><div>bxyz = magnetic field components</div><div>vt = total proton speed</div><div>vxyz = velocity components (only for PSP)</div><div>np = proton density</div><div>tp = proton temperature</div><div>xyz = spacecraft position in HEEQ</div><div>r, lat, lon = spherical coordinates of position in HEEQ</div><div><br /></div><div><br /></div><div><br /></div><div><br /></div>
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- Added Date: 2022-02-19 19:15:08
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