Loading…
A Test Particle Monte Carlo Investigation of the CH4 Torus around Saturn
The issue of CH4 escape on Titan is still under debate, and a range of escape rates from 1024 to 1027 s−1 has been reported in previous studies. One effective way of solving the CH4 escape dilemma is to investigate the morphology of the CH4 torus around Saturn, which varies with both the total CH4 e...
Saved in:
Published in: | The Astronomical journal 2019-01, Vol.157 (1) |
---|---|
Main Authors: | , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
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 | 1 |
container_start_page | |
container_title | The Astronomical journal |
container_volume | 157 |
creator | Niu, D.-D. Cui, J. Gu, H. Dong, C.-Y. Zhou, L.-Y. Wellbrock, A. Jiang, F.-Y. Xu, X.-J. |
description | The issue of CH4 escape on Titan is still under debate, and a range of escape rates from 1024 to 1027 s−1 has been reported in previous studies. One effective way of solving the CH4 escape dilemma is to investigate the morphology of the CH4 torus around Saturn, which varies with both the total CH4 escape rate on Titan and the CH4 energy distribution near its exobase. Such a torus is modeled via a test particle Monte Carlo approach in this study for a variety of CH4 escaping scenarios characterized by different energy distributions near the exobase. The model calculations indicate that the extension of the CH4 torus depends critically on the population of the high-energy tail of the CH4 energy distribution. The model also predicts several distinctive cavities in CH4 density related to mean motion resonances between Titan and the torus particles. |
doi_str_mv | 10.3847/1538-3881/aaf161 |
format | article |
fullrecord | <record><control><sourceid>proquest_iop_j</sourceid><recordid>TN_cdi_iop_journals_10_3847_1538_3881_aaf161</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365684320</sourcerecordid><originalsourceid>FETCH-LOGICAL-i290t-c16b0fe74b655fd4da63c26073df6e8d53d59979921d2ce573675296c704aedd3</originalsourceid><addsrcrecordid>eNpVkM1LAzEQxYMoWKt3jwGvrp18Z4-laLdQUbCeQ7pJdEvZ1N2sf78pKxYvMzDvx3vDQ-iWwAPTXM2IYLpgWpOZtYFIcoYmf6dzNAEAXkgq5CW66vsdACEa-ARVc7zxfcKvtktNvff4ObbJ44Xt9hGv2u-sNR82NbHFMeD0maWK403shh7bLg6tw282DV17jS6C3ff-5ndP0fvT42ZRFeuX5WoxXxcNLSEVNZFbCF7xrRQiOO6sZDWVoJgL0msnmBNlqcqSEkdrLxSTStBS1gq49c6xKbobfQ9d_Brye2YXc3yONJRJITVnFDJ1P1JNPJwAAubYlTkWY47FmLGrk-k_3O4ymek8zcEF9gMi3mbv</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365684320</pqid></control><display><type>article</type><title>A Test Particle Monte Carlo Investigation of the CH4 Torus around Saturn</title><source>DOAJ Directory of Open Access Journals</source><creator>Niu, D.-D. ; Cui, J. ; Gu, H. ; Dong, C.-Y. ; Zhou, L.-Y. ; Wellbrock, A. ; Jiang, F.-Y. ; Xu, X.-J.</creator><creatorcontrib>Niu, D.-D. ; Cui, J. ; Gu, H. ; Dong, C.-Y. ; Zhou, L.-Y. ; Wellbrock, A. ; Jiang, F.-Y. ; Xu, X.-J.</creatorcontrib><description>The issue of CH4 escape on Titan is still under debate, and a range of escape rates from 1024 to 1027 s−1 has been reported in previous studies. One effective way of solving the CH4 escape dilemma is to investigate the morphology of the CH4 torus around Saturn, which varies with both the total CH4 escape rate on Titan and the CH4 energy distribution near its exobase. Such a torus is modeled via a test particle Monte Carlo approach in this study for a variety of CH4 escaping scenarios characterized by different energy distributions near the exobase. The model calculations indicate that the extension of the CH4 torus depends critically on the population of the high-energy tail of the CH4 energy distribution. The model also predicts several distinctive cavities in CH4 density related to mean motion resonances between Titan and the torus particles.</description><identifier>ISSN: 0004-6256</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.3847/1538-3881/aaf161</identifier><language>eng</language><publisher>Madison: The American Astronomical Society</publisher><subject>Astronomy ; Computer simulation ; Energy distribution ; Methane ; Morphology ; Orbital resonances (celestial mechanics) ; planets and satellites: atmospheres ; planets and satellites: individual (Titan) ; Saturn ; Titan ; Toruses</subject><ispartof>The Astronomical journal, 2019-01, Vol.157 (1)</ispartof><rights>2018. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Jan 2019</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0002-4721-8184 ; 0000-0002-9831-0618 ; 0000-0002-5332-0214 ; 0000-0002-2309-0649</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,864,27923,27924</link.rule.ids></links><search><creatorcontrib>Niu, D.-D.</creatorcontrib><creatorcontrib>Cui, J.</creatorcontrib><creatorcontrib>Gu, H.</creatorcontrib><creatorcontrib>Dong, C.-Y.</creatorcontrib><creatorcontrib>Zhou, L.-Y.</creatorcontrib><creatorcontrib>Wellbrock, A.</creatorcontrib><creatorcontrib>Jiang, F.-Y.</creatorcontrib><creatorcontrib>Xu, X.-J.</creatorcontrib><title>A Test Particle Monte Carlo Investigation of the CH4 Torus around Saturn</title><title>The Astronomical journal</title><addtitle>AJ</addtitle><addtitle>Astron. J</addtitle><description>The issue of CH4 escape on Titan is still under debate, and a range of escape rates from 1024 to 1027 s−1 has been reported in previous studies. One effective way of solving the CH4 escape dilemma is to investigate the morphology of the CH4 torus around Saturn, which varies with both the total CH4 escape rate on Titan and the CH4 energy distribution near its exobase. Such a torus is modeled via a test particle Monte Carlo approach in this study for a variety of CH4 escaping scenarios characterized by different energy distributions near the exobase. The model calculations indicate that the extension of the CH4 torus depends critically on the population of the high-energy tail of the CH4 energy distribution. The model also predicts several distinctive cavities in CH4 density related to mean motion resonances between Titan and the torus particles.</description><subject>Astronomy</subject><subject>Computer simulation</subject><subject>Energy distribution</subject><subject>Methane</subject><subject>Morphology</subject><subject>Orbital resonances (celestial mechanics)</subject><subject>planets and satellites: atmospheres</subject><subject>planets and satellites: individual (Titan)</subject><subject>Saturn</subject><subject>Titan</subject><subject>Toruses</subject><issn>0004-6256</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNpVkM1LAzEQxYMoWKt3jwGvrp18Z4-laLdQUbCeQ7pJdEvZ1N2sf78pKxYvMzDvx3vDQ-iWwAPTXM2IYLpgWpOZtYFIcoYmf6dzNAEAXkgq5CW66vsdACEa-ARVc7zxfcKvtktNvff4ObbJ44Xt9hGv2u-sNR82NbHFMeD0maWK403shh7bLg6tw282DV17jS6C3ff-5ndP0fvT42ZRFeuX5WoxXxcNLSEVNZFbCF7xrRQiOO6sZDWVoJgL0msnmBNlqcqSEkdrLxSTStBS1gq49c6xKbobfQ9d_Brye2YXc3yONJRJITVnFDJ1P1JNPJwAAubYlTkWY47FmLGrk-k_3O4ymek8zcEF9gMi3mbv</recordid><startdate>20190101</startdate><enddate>20190101</enddate><creator>Niu, D.-D.</creator><creator>Cui, J.</creator><creator>Gu, H.</creator><creator>Dong, C.-Y.</creator><creator>Zhou, L.-Y.</creator><creator>Wellbrock, A.</creator><creator>Jiang, F.-Y.</creator><creator>Xu, X.-J.</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-4721-8184</orcidid><orcidid>https://orcid.org/0000-0002-9831-0618</orcidid><orcidid>https://orcid.org/0000-0002-5332-0214</orcidid><orcidid>https://orcid.org/0000-0002-2309-0649</orcidid></search><sort><creationdate>20190101</creationdate><title>A Test Particle Monte Carlo Investigation of the CH4 Torus around Saturn</title><author>Niu, D.-D. ; Cui, J. ; Gu, H. ; Dong, C.-Y. ; Zhou, L.-Y. ; Wellbrock, A. ; Jiang, F.-Y. ; Xu, X.-J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-i290t-c16b0fe74b655fd4da63c26073df6e8d53d59979921d2ce573675296c704aedd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Astronomy</topic><topic>Computer simulation</topic><topic>Energy distribution</topic><topic>Methane</topic><topic>Morphology</topic><topic>Orbital resonances (celestial mechanics)</topic><topic>planets and satellites: atmospheres</topic><topic>planets and satellites: individual (Titan)</topic><topic>Saturn</topic><topic>Titan</topic><topic>Toruses</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Niu, D.-D.</creatorcontrib><creatorcontrib>Cui, J.</creatorcontrib><creatorcontrib>Gu, H.</creatorcontrib><creatorcontrib>Dong, C.-Y.</creatorcontrib><creatorcontrib>Zhou, L.-Y.</creatorcontrib><creatorcontrib>Wellbrock, A.</creatorcontrib><creatorcontrib>Jiang, F.-Y.</creatorcontrib><creatorcontrib>Xu, X.-J.</creatorcontrib><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Niu, D.-D.</au><au>Cui, J.</au><au>Gu, H.</au><au>Dong, C.-Y.</au><au>Zhou, L.-Y.</au><au>Wellbrock, A.</au><au>Jiang, F.-Y.</au><au>Xu, X.-J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Test Particle Monte Carlo Investigation of the CH4 Torus around Saturn</atitle><jtitle>The Astronomical journal</jtitle><stitle>AJ</stitle><addtitle>Astron. J</addtitle><date>2019-01-01</date><risdate>2019</risdate><volume>157</volume><issue>1</issue><issn>0004-6256</issn><eissn>1538-3881</eissn><abstract>The issue of CH4 escape on Titan is still under debate, and a range of escape rates from 1024 to 1027 s−1 has been reported in previous studies. One effective way of solving the CH4 escape dilemma is to investigate the morphology of the CH4 torus around Saturn, which varies with both the total CH4 escape rate on Titan and the CH4 energy distribution near its exobase. Such a torus is modeled via a test particle Monte Carlo approach in this study for a variety of CH4 escaping scenarios characterized by different energy distributions near the exobase. The model calculations indicate that the extension of the CH4 torus depends critically on the population of the high-energy tail of the CH4 energy distribution. The model also predicts several distinctive cavities in CH4 density related to mean motion resonances between Titan and the torus particles.</abstract><cop>Madison</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-3881/aaf161</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0002-4721-8184</orcidid><orcidid>https://orcid.org/0000-0002-9831-0618</orcidid><orcidid>https://orcid.org/0000-0002-5332-0214</orcidid><orcidid>https://orcid.org/0000-0002-2309-0649</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6256 |
ispartof | The Astronomical journal, 2019-01, Vol.157 (1) |
issn | 0004-6256 1538-3881 |
language | eng |
recordid | cdi_iop_journals_10_3847_1538_3881_aaf161 |
source | DOAJ Directory of Open Access Journals |
subjects | Astronomy Computer simulation Energy distribution Methane Morphology Orbital resonances (celestial mechanics) planets and satellites: atmospheres planets and satellites: individual (Titan) Saturn Titan Toruses |
title | A Test Particle Monte Carlo Investigation of the CH4 Torus around Saturn |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-08T19%3A16%3A54IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_iop_j&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20Test%20Particle%20Monte%20Carlo%20Investigation%20of%20the%20CH4%20Torus%20around%20Saturn&rft.jtitle=The%20Astronomical%20journal&rft.au=Niu,%20D.-D.&rft.date=2019-01-01&rft.volume=157&rft.issue=1&rft.issn=0004-6256&rft.eissn=1538-3881&rft_id=info:doi/10.3847/1538-3881/aaf161&rft_dat=%3Cproquest_iop_j%3E2365684320%3C/proquest_iop_j%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-i290t-c16b0fe74b655fd4da63c26073df6e8d53d59979921d2ce573675296c704aedd3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2365684320&rft_id=info:pmid/&rfr_iscdi=true |