The Catalogue for Astrophysical Turbulence Simulations (CATS)

Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray propagation. However, data from numerical simulations...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2020-10
Main Authors: Burkhart, B, Appel, S, Bialy, S, Cho, J, Christensen, A J, Collins, D, Federrath, C, Fielding, D, Finkbeiner, D, Hill, A S, Ibanez-Mejia, J C, Krumholz, M R, Lazarian, A, M Li, Mocz, P, -M Mac Low, M, Naiman, J, Portillo, S K N, Shane, B, Slepian, Z, Yuan, Y
Format: Article
Language:English
Subjects:
Astrophysics
Celestial bodies
Computational fluid dynamics
Correlation analysis
Cosmic ray propagation
Cosmic rays
Cubes
Fluid flow
Magnetohydrodynamic turbulence
Power spectra
Simulation
Star & galaxy formation
Star formation
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Burkhart, B
Appel, S
Bialy, S
Cho, J
Christensen, A J
Collins, D
Federrath, C
Fielding, D
Finkbeiner, D
Hill, A S
Ibanez-Mejia, J C
Krumholz, M R
Lazarian, A
M Li
Mocz, P
-M Mac Low, M
Naiman, J
Portillo, S K N
Shane, B
Slepian, Z
Yuan, Y
description Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray propagation. However, data from numerical simulations of astrophysical turbulence are often not made public. We introduce a new simulation-oriented database for the astronomical community: The Catalogue for Astrophysical Turbulence Simulations (CATS), located at www.mhdturbulence.com. CATS includes magnetohydrodynamic (MHD) turbulent box simulation data products generated by the public codes athena++, arepo, enzo, and flash. CATS also includes several synthetic observational data sets, such as turbulent HI data cubes. We also include measured power spectra and 3-point correlation functions from some of these data. We discuss the importance of open source statistical and visualization tools for the analysis of turbulence simulations such as those found in CATS.
doi_str_mv 10.48550/arxiv.2010.11227
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2453833113</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2453833113</sourcerecordid><originalsourceid>FETCH-LOGICAL-a523-29487a5aaa0ae22bb3018c44328fdc92a544a0e31dd876624f0d998759455ab03</originalsourceid><addsrcrecordid>eNotj0FLwzAYhoMgbMz9gN0CXvTQmXzJ16YHD6XoFAYe1vv42qauozYzaUT_vQU9vfAcnoeXsY0UW20QxQP57_5rC2IGUgJkV2wJSsnEaIAFW4dwFkJAmgGiWrLH6mR5SRMN7j1a3jnPizB5dzn9hL6hgVfR13GwY2P5of-IA029GwO_K4vqcH_Drjsagl3_74pVz09V-ZLs33avZbFPCEElkGuTERKRIAtQ10pI02itwHRtkwOh1iSskm1rsjQF3Yk2z02GuUakWqgVu_3TXrz7jDZMx7OLfpyLR9CozHxPKvUL05dINA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2453833113</pqid></control><display><type>article</type><title>The Catalogue for Astrophysical Turbulence Simulations (CATS)</title><source>ProQuest - Publicly Available Content Database</source><creator>Burkhart, B ; Appel, S ; Bialy, S ; Cho, J ; Christensen, A J ; Collins, D ; Federrath, C ; Fielding, D ; Finkbeiner, D ; Hill, A S ; Ibanez-Mejia, J C ; Krumholz, M R ; Lazarian, A ; M Li ; Mocz, P ; -M Mac Low, M ; Naiman, J ; Portillo, S K N ; Shane, B ; Slepian, Z ; Yuan, Y</creator><creatorcontrib>Burkhart, B ; Appel, S ; Bialy, S ; Cho, J ; Christensen, A J ; Collins, D ; Federrath, C ; Fielding, D ; Finkbeiner, D ; Hill, A S ; Ibanez-Mejia, J C ; Krumholz, M R ; Lazarian, A ; M Li ; Mocz, P ; -M Mac Low, M ; Naiman, J ; Portillo, S K N ; Shane, B ; Slepian, Z ; Yuan, Y</creatorcontrib><description>Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray propagation. However, data from numerical simulations of astrophysical turbulence are often not made public. We introduce a new simulation-oriented database for the astronomical community: The Catalogue for Astrophysical Turbulence Simulations (CATS), located at www.mhdturbulence.com. CATS includes magnetohydrodynamic (MHD) turbulent box simulation data products generated by the public codes athena++, arepo, enzo, and flash. CATS also includes several synthetic observational data sets, such as turbulent HI data cubes. We also include measured power spectra and 3-point correlation functions from some of these data. We discuss the importance of open source statistical and visualization tools for the analysis of turbulence simulations such as those found in CATS.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2010.11227</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Astrophysics ; Celestial bodies ; Computational fluid dynamics ; Correlation analysis ; Cosmic ray propagation ; Cosmic rays ; Cubes ; Fluid flow ; Magnetohydrodynamic turbulence ; Power spectra ; Simulation ; Star &amp; galaxy formation ; Star formation</subject><ispartof>arXiv.org, 2020-10</ispartof><rights>2020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2453833113?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25753,27925,37012,44590</link.rule.ids></links><search><creatorcontrib>Burkhart, B</creatorcontrib><creatorcontrib>Appel, S</creatorcontrib><creatorcontrib>Bialy, S</creatorcontrib><creatorcontrib>Cho, J</creatorcontrib><creatorcontrib>Christensen, A J</creatorcontrib><creatorcontrib>Collins, D</creatorcontrib><creatorcontrib>Federrath, C</creatorcontrib><creatorcontrib>Fielding, D</creatorcontrib><creatorcontrib>Finkbeiner, D</creatorcontrib><creatorcontrib>Hill, A S</creatorcontrib><creatorcontrib>Ibanez-Mejia, J C</creatorcontrib><creatorcontrib>Krumholz, M R</creatorcontrib><creatorcontrib>Lazarian, A</creatorcontrib><creatorcontrib>M Li</creatorcontrib><creatorcontrib>Mocz, P</creatorcontrib><creatorcontrib>-M Mac Low, M</creatorcontrib><creatorcontrib>Naiman, J</creatorcontrib><creatorcontrib>Portillo, S K N</creatorcontrib><creatorcontrib>Shane, B</creatorcontrib><creatorcontrib>Slepian, Z</creatorcontrib><creatorcontrib>Yuan, Y</creatorcontrib><title>The Catalogue for Astrophysical Turbulence Simulations (CATS)</title><title>arXiv.org</title><description>Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray propagation. However, data from numerical simulations of astrophysical turbulence are often not made public. We introduce a new simulation-oriented database for the astronomical community: The Catalogue for Astrophysical Turbulence Simulations (CATS), located at www.mhdturbulence.com. CATS includes magnetohydrodynamic (MHD) turbulent box simulation data products generated by the public codes athena++, arepo, enzo, and flash. CATS also includes several synthetic observational data sets, such as turbulent HI data cubes. We also include measured power spectra and 3-point correlation functions from some of these data. We discuss the importance of open source statistical and visualization tools for the analysis of turbulence simulations such as those found in CATS.</description><subject>Astrophysics</subject><subject>Celestial bodies</subject><subject>Computational fluid dynamics</subject><subject>Correlation analysis</subject><subject>Cosmic ray propagation</subject><subject>Cosmic rays</subject><subject>Cubes</subject><subject>Fluid flow</subject><subject>Magnetohydrodynamic turbulence</subject><subject>Power spectra</subject><subject>Simulation</subject><subject>Star &amp; galaxy formation</subject><subject>Star formation</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotj0FLwzAYhoMgbMz9gN0CXvTQmXzJ16YHD6XoFAYe1vv42qauozYzaUT_vQU9vfAcnoeXsY0UW20QxQP57_5rC2IGUgJkV2wJSsnEaIAFW4dwFkJAmgGiWrLH6mR5SRMN7j1a3jnPizB5dzn9hL6hgVfR13GwY2P5of-IA029GwO_K4vqcH_Drjsagl3_74pVz09V-ZLs33avZbFPCEElkGuTERKRIAtQ10pI02itwHRtkwOh1iSskm1rsjQF3Yk2z02GuUakWqgVu_3TXrz7jDZMx7OLfpyLR9CozHxPKvUL05dINA</recordid><startdate>20201021</startdate><enddate>20201021</enddate><creator>Burkhart, B</creator><creator>Appel, S</creator><creator>Bialy, S</creator><creator>Cho, J</creator><creator>Christensen, A J</creator><creator>Collins, D</creator><creator>Federrath, C</creator><creator>Fielding, D</creator><creator>Finkbeiner, D</creator><creator>Hill, A S</creator><creator>Ibanez-Mejia, J C</creator><creator>Krumholz, M R</creator><creator>Lazarian, A</creator><creator>M Li</creator><creator>Mocz, P</creator><creator>-M Mac Low, M</creator><creator>Naiman, J</creator><creator>Portillo, S K N</creator><creator>Shane, B</creator><creator>Slepian, Z</creator><creator>Yuan, Y</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20201021</creationdate><title>The Catalogue for Astrophysical Turbulence Simulations (CATS)</title><author>Burkhart, B ; Appel, S ; Bialy, S ; Cho, J ; Christensen, A J ; Collins, D ; Federrath, C ; Fielding, D ; Finkbeiner, D ; Hill, A S ; Ibanez-Mejia, J C ; Krumholz, M R ; Lazarian, A ; M Li ; Mocz, P ; -M Mac Low, M ; Naiman, J ; Portillo, S K N ; Shane, B ; Slepian, Z ; Yuan, Y</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a523-29487a5aaa0ae22bb3018c44328fdc92a544a0e31dd876624f0d998759455ab03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Astrophysics</topic><topic>Celestial bodies</topic><topic>Computational fluid dynamics</topic><topic>Correlation analysis</topic><topic>Cosmic ray propagation</topic><topic>Cosmic rays</topic><topic>Cubes</topic><topic>Fluid flow</topic><topic>Magnetohydrodynamic turbulence</topic><topic>Power spectra</topic><topic>Simulation</topic><topic>Star &amp; galaxy formation</topic><topic>Star formation</topic><toplevel>online_resources</toplevel><creatorcontrib>Burkhart, B</creatorcontrib><creatorcontrib>Appel, S</creatorcontrib><creatorcontrib>Bialy, S</creatorcontrib><creatorcontrib>Cho, J</creatorcontrib><creatorcontrib>Christensen, A J</creatorcontrib><creatorcontrib>Collins, D</creatorcontrib><creatorcontrib>Federrath, C</creatorcontrib><creatorcontrib>Fielding, D</creatorcontrib><creatorcontrib>Finkbeiner, D</creatorcontrib><creatorcontrib>Hill, A S</creatorcontrib><creatorcontrib>Ibanez-Mejia, J C</creatorcontrib><creatorcontrib>Krumholz, M R</creatorcontrib><creatorcontrib>Lazarian, A</creatorcontrib><creatorcontrib>M Li</creatorcontrib><creatorcontrib>Mocz, P</creatorcontrib><creatorcontrib>-M Mac Low, M</creatorcontrib><creatorcontrib>Naiman, J</creatorcontrib><creatorcontrib>Portillo, S K N</creatorcontrib><creatorcontrib>Shane, B</creatorcontrib><creatorcontrib>Slepian, Z</creatorcontrib><creatorcontrib>Yuan, Y</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>ProQuest - Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Burkhart, B</au><au>Appel, S</au><au>Bialy, S</au><au>Cho, J</au><au>Christensen, A J</au><au>Collins, D</au><au>Federrath, C</au><au>Fielding, D</au><au>Finkbeiner, D</au><au>Hill, A S</au><au>Ibanez-Mejia, J C</au><au>Krumholz, M R</au><au>Lazarian, A</au><au>M Li</au><au>Mocz, P</au><au>-M Mac Low, M</au><au>Naiman, J</au><au>Portillo, S K N</au><au>Shane, B</au><au>Slepian, Z</au><au>Yuan, Y</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Catalogue for Astrophysical Turbulence Simulations (CATS)</atitle><jtitle>arXiv.org</jtitle><date>2020-10-21</date><risdate>2020</risdate><eissn>2331-8422</eissn><abstract>Turbulence is a key process in many fields of astrophysics. Advances in numerical simulations of fluids over the last several decades have revolutionized our understanding of turbulence and related processes such as star formation and cosmic ray propagation. However, data from numerical simulations of astrophysical turbulence are often not made public. We introduce a new simulation-oriented database for the astronomical community: The Catalogue for Astrophysical Turbulence Simulations (CATS), located at www.mhdturbulence.com. CATS includes magnetohydrodynamic (MHD) turbulent box simulation data products generated by the public codes athena++, arepo, enzo, and flash. CATS also includes several synthetic observational data sets, such as turbulent HI data cubes. We also include measured power spectra and 3-point correlation functions from some of these data. We discuss the importance of open source statistical and visualization tools for the analysis of turbulence simulations such as those found in CATS.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2010.11227</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2020-10
issn 2331-8422
language eng
recordid cdi_proquest_journals_2453833113
source ProQuest - Publicly Available Content Database
subjects Astrophysics
Celestial bodies
Computational fluid dynamics
Correlation analysis
Cosmic ray propagation
Cosmic rays
Cubes
Fluid flow
Magnetohydrodynamic turbulence
Power spectra
Simulation
Star & galaxy formation
Star formation
title The Catalogue for Astrophysical Turbulence Simulations (CATS)
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-06T06%3A50%3A51IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Catalogue%20for%20Astrophysical%20Turbulence%20Simulations%20(CATS)&rft.jtitle=arXiv.org&rft.au=Burkhart,%20B&rft.date=2020-10-21&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2010.11227&rft_dat=%3Cproquest%3E2453833113%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a523-29487a5aaa0ae22bb3018c44328fdc92a544a0e31dd876624f0d998759455ab03%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2453833113&rft_id=info:pmid/&rfr_iscdi=true