Data for paper "Resonant Drag Instabilities in Polydisperse Dust: II. The streaming and settling instability"
doi:10.4121/810f163a-b786-4366-ad9b-5794d71c4ede.v1
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doi: 10.4121/810f163a-b786-4366-ad9b-5794d71c4ede
doi: 10.4121/810f163a-b786-4366-ad9b-5794d71c4ede
Datacite citation style:
Paardekooper, Sijme-Jan; Aly, Hossam (2024): Data for paper "Resonant Drag Instabilities in Polydisperse Dust: II. The streaming and settling instability". Version 1. 4TU.ResearchData. dataset. https://doi.org/10.4121/810f163a-b786-4366-ad9b-5794d71c4ede.v1
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Dataset
categories
licence
CC0
Numerically calculated growth rates for the streaming and settling instability, as published in "Resonant Drag Instabilities in Polydisperse Dust: II. The streaming and settling instability" by Paardekooper & Aly. These multiphase hydrodynamic instabilities are thought to be important in planet formation, since they can concentrate solid particles into clouds of high enough density so that they can collapse gravitationally. Calculations were done using the publicly available package PSITOOLS.
history
- 2024-12-18 first online, published, posted
publisher
4TU.ResearchData
format
Numpy savez
funding
- DUSTSPEC (grant code 101054502) ERC
organizations
TU Delft, Faculty of Aerospace Engineering, Department of Space Engineering
DATA
files (16)
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fig_dsi_contour_growth.npz - 167,038 bytesMD5:
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fig_dsi_convergence.npz - 322,608 bytesMD5:
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fig_dsi_convergence_max.npz - 446,280 bytesMD5:
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fig_dsi_double_growth.npz - 5,127,642 bytesMD5:
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fig_dsi_monoresonance.npz - 12,170 bytesMD5:
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fig_dsi_poly_kx.npz - 1,604,618 bytesMD5:
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fig_dsi_visc.npz - 11,178 bytesMD5:
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fig_si_cont.npz - 7,414 bytesMD5:
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fig_si_delta.npz - 322,842 bytesMD5:
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fig_si_monoresonance.npz - 322,842 bytesMD5:
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fig_si_resonance.npz - 2,592 bytesMD5:
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paper.mplstyle - 17,235 bytesMD5:
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paper_figures.py - 203 bytesMD5:
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requirements.txt -
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