Inward electrostatic precipitation of interplanetary particles

An inward precipitator collects particles initially dispersed in a gas throughout either a cylindrical or spherical chamber onto a small central planchet. The instrument is effective for particle diameters greater than about 1 μm. One use is the collection of interplanetary dust particles which are...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Review of scientific instruments 1994-06, Vol.65 (6), p.1839-1846
Hauptverfasser: Rulison, Aaron J., Flagan, Richard C., Ahrens, Thomas J.
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 1846
container_issue 6
container_start_page 1839
container_title Review of scientific instruments
container_volume 65
creator Rulison, Aaron J.
Flagan, Richard C.
Ahrens, Thomas J.
description An inward precipitator collects particles initially dispersed in a gas throughout either a cylindrical or spherical chamber onto a small central planchet. The instrument is effective for particle diameters greater than about 1 μm. One use is the collection of interplanetary dust particles which are stopped in a noble gas (xenon) by drag and ablation after perforating the wall of a thin‐walled spacecraft‐mounted chamber. First, the particles are positively charged for several seconds by the corona production of positive xenon ions from inward facing needles placed on the chamber wall. Then an electric field causes the particles to migrate toward the center of the instrument and onto the planchet. The collection time (of the order of hours for a 1 m radius spherical chamber) is greatly reduced by the use of optimally located screens which reapportion the electric field. Some of the electric field lines terminate on the wires of the screens so a fraction of the total number of particles in the chamber is lost. The operation of the instrument is demonstrated by experiments which show the migration of carbon soot particles with radius of approximately 1 μm in a 5‐cm‐diam cylindrical chamber with a single field enhancing screen toward a 3.2 mm central collection rod.
doi_str_mv 10.1063/1.1144832
format Article
fullrecord <record><control><sourceid>scitation_cross</sourceid><recordid>TN_cdi_scitation_primary_10_1063_1_1144832</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>rsi</sourcerecordid><originalsourceid>FETCH-LOGICAL-c294t-e6247109963e5b8375e4764ef0aa7d49246ff84e127678015b2b29449e6ad5413</originalsourceid><addsrcrecordid>eNqdj01LxDAQhoMouK4e_Ae9KnTNJNOkvQiy-LGw4EXPIU0nUKltSILiv7fLFrw7l2HgeYf3Yewa-Aa4knewAUCspThhK-B1U2ol5ClbcS6xVBrrc3aR0gefpwJYsfvd-G1jV9BALscpZZt7V4RIrg_94ZjGYvJFP2aKYbAjZRt_imDjjA2ULtmZt0Oiq2Wv2fvT49v2pdy_Pu-2D_vSiQZzSUqgBt40SlLV1lJXhFoheW6t7rARqLyvkUBopWsOVSvaOYgNKdtVCHLNbo5_3dwxRfImxP5zrmKAm4O4AbOIz-ztkU1uMfgf_DXFP9CEzstfuKBmYw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Inward electrostatic precipitation of interplanetary particles</title><source>AIP Digital Archive</source><creator>Rulison, Aaron J. ; Flagan, Richard C. ; Ahrens, Thomas J.</creator><creatorcontrib>Rulison, Aaron J. ; Flagan, Richard C. ; Ahrens, Thomas J.</creatorcontrib><description>An inward precipitator collects particles initially dispersed in a gas throughout either a cylindrical or spherical chamber onto a small central planchet. The instrument is effective for particle diameters greater than about 1 μm. One use is the collection of interplanetary dust particles which are stopped in a noble gas (xenon) by drag and ablation after perforating the wall of a thin‐walled spacecraft‐mounted chamber. First, the particles are positively charged for several seconds by the corona production of positive xenon ions from inward facing needles placed on the chamber wall. Then an electric field causes the particles to migrate toward the center of the instrument and onto the planchet. The collection time (of the order of hours for a 1 m radius spherical chamber) is greatly reduced by the use of optimally located screens which reapportion the electric field. Some of the electric field lines terminate on the wires of the screens so a fraction of the total number of particles in the chamber is lost. The operation of the instrument is demonstrated by experiments which show the migration of carbon soot particles with radius of approximately 1 μm in a 5‐cm‐diam cylindrical chamber with a single field enhancing screen toward a 3.2 mm central collection rod.</description><identifier>ISSN: 0034-6748</identifier><identifier>EISSN: 1089-7623</identifier><identifier>DOI: 10.1063/1.1144832</identifier><identifier>CODEN: RSINAK</identifier><language>eng</language><ispartof>Review of scientific instruments, 1994-06, Vol.65 (6), p.1839-1846</ispartof><rights>American Institute of Physics</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c294t-e6247109963e5b8375e4764ef0aa7d49246ff84e127678015b2b29449e6ad5413</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/rsi/article-lookup/doi/10.1063/1.1144832$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,780,784,1559,27924,27925,76390</link.rule.ids></links><search><creatorcontrib>Rulison, Aaron J.</creatorcontrib><creatorcontrib>Flagan, Richard C.</creatorcontrib><creatorcontrib>Ahrens, Thomas J.</creatorcontrib><title>Inward electrostatic precipitation of interplanetary particles</title><title>Review of scientific instruments</title><description>An inward precipitator collects particles initially dispersed in a gas throughout either a cylindrical or spherical chamber onto a small central planchet. The instrument is effective for particle diameters greater than about 1 μm. One use is the collection of interplanetary dust particles which are stopped in a noble gas (xenon) by drag and ablation after perforating the wall of a thin‐walled spacecraft‐mounted chamber. First, the particles are positively charged for several seconds by the corona production of positive xenon ions from inward facing needles placed on the chamber wall. Then an electric field causes the particles to migrate toward the center of the instrument and onto the planchet. The collection time (of the order of hours for a 1 m radius spherical chamber) is greatly reduced by the use of optimally located screens which reapportion the electric field. Some of the electric field lines terminate on the wires of the screens so a fraction of the total number of particles in the chamber is lost. The operation of the instrument is demonstrated by experiments which show the migration of carbon soot particles with radius of approximately 1 μm in a 5‐cm‐diam cylindrical chamber with a single field enhancing screen toward a 3.2 mm central collection rod.</description><issn>0034-6748</issn><issn>1089-7623</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1994</creationdate><recordtype>article</recordtype><recordid>eNqdj01LxDAQhoMouK4e_Ae9KnTNJNOkvQiy-LGw4EXPIU0nUKltSILiv7fLFrw7l2HgeYf3Yewa-Aa4knewAUCspThhK-B1U2ol5ClbcS6xVBrrc3aR0gefpwJYsfvd-G1jV9BALscpZZt7V4RIrg_94ZjGYvJFP2aKYbAjZRt_imDjjA2ULtmZt0Oiq2Wv2fvT49v2pdy_Pu-2D_vSiQZzSUqgBt40SlLV1lJXhFoheW6t7rARqLyvkUBopWsOVSvaOYgNKdtVCHLNbo5_3dwxRfImxP5zrmKAm4O4AbOIz-ztkU1uMfgf_DXFP9CEzstfuKBmYw</recordid><startdate>19940601</startdate><enddate>19940601</enddate><creator>Rulison, Aaron J.</creator><creator>Flagan, Richard C.</creator><creator>Ahrens, Thomas J.</creator><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19940601</creationdate><title>Inward electrostatic precipitation of interplanetary particles</title><author>Rulison, Aaron J. ; Flagan, Richard C. ; Ahrens, Thomas J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c294t-e6247109963e5b8375e4764ef0aa7d49246ff84e127678015b2b29449e6ad5413</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1994</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rulison, Aaron J.</creatorcontrib><creatorcontrib>Flagan, Richard C.</creatorcontrib><creatorcontrib>Ahrens, Thomas J.</creatorcontrib><collection>CrossRef</collection><jtitle>Review of scientific instruments</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Rulison, Aaron J.</au><au>Flagan, Richard C.</au><au>Ahrens, Thomas J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Inward electrostatic precipitation of interplanetary particles</atitle><jtitle>Review of scientific instruments</jtitle><date>1994-06-01</date><risdate>1994</risdate><volume>65</volume><issue>6</issue><spage>1839</spage><epage>1846</epage><pages>1839-1846</pages><issn>0034-6748</issn><eissn>1089-7623</eissn><coden>RSINAK</coden><abstract>An inward precipitator collects particles initially dispersed in a gas throughout either a cylindrical or spherical chamber onto a small central planchet. The instrument is effective for particle diameters greater than about 1 μm. One use is the collection of interplanetary dust particles which are stopped in a noble gas (xenon) by drag and ablation after perforating the wall of a thin‐walled spacecraft‐mounted chamber. First, the particles are positively charged for several seconds by the corona production of positive xenon ions from inward facing needles placed on the chamber wall. Then an electric field causes the particles to migrate toward the center of the instrument and onto the planchet. The collection time (of the order of hours for a 1 m radius spherical chamber) is greatly reduced by the use of optimally located screens which reapportion the electric field. Some of the electric field lines terminate on the wires of the screens so a fraction of the total number of particles in the chamber is lost. The operation of the instrument is demonstrated by experiments which show the migration of carbon soot particles with radius of approximately 1 μm in a 5‐cm‐diam cylindrical chamber with a single field enhancing screen toward a 3.2 mm central collection rod.</abstract><doi>10.1063/1.1144832</doi><tpages>8</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0034-6748
ispartof Review of scientific instruments, 1994-06, Vol.65 (6), p.1839-1846
issn 0034-6748
1089-7623
language eng
recordid cdi_scitation_primary_10_1063_1_1144832
source AIP Digital Archive
title Inward electrostatic precipitation of interplanetary particles
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T12%3A54%3A22IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-scitation_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Inward%20electrostatic%20precipitation%20of%20interplanetary%20particles&rft.jtitle=Review%20of%20scientific%20instruments&rft.au=Rulison,%20Aaron%20J.&rft.date=1994-06-01&rft.volume=65&rft.issue=6&rft.spage=1839&rft.epage=1846&rft.pages=1839-1846&rft.issn=0034-6748&rft.eissn=1089-7623&rft.coden=RSINAK&rft_id=info:doi/10.1063/1.1144832&rft_dat=%3Cscitation_cross%3Ersi%3C/scitation_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true