Hypervelocity dust particle impacts observed by the Giotto Magnetometer and Plasma Experiments
This paper describes 13 very short events in the magnetic field of the inner magnetic pile-up region of Comet Halley observed by the Giotto magnetometer experiment together with simultaneous plasma data obtained by the Johnstone plasma analyzer and the ion mass spectrometer experiments. The events a...
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Veröffentlicht in: | Geophysical research letters 1990-10, Vol.17 (11), p.1809-1812 |
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creator | Neubauer, F. M. Glassmeier, K.-H. Coates, A. J. Goldstein, R. Acuña, M. H. Musmann, G. |
description | This paper describes 13 very short events in the magnetic field of the inner magnetic pile-up region of Comet Halley observed by the Giotto magnetometer experiment together with simultaneous plasma data obtained by the Johnstone plasma analyzer and the ion mass spectrometer experiments. The events are due to dust impacts in the milligram range on the spacecraft at the relative velocity between the cometary dust and the spacecraft of 68 km/sec. They are generally consistent with dust impact events derived from spacecraft attitude perturbations by the Giotto camera. Their characteristic shape generally involves a sudden decrease in magnetic-field magnitude, a subsequent overshoot beyond initial field values, and an asymptotic approach to the initial field (somewhat reminiscent of the magnetic-field signature after the AMPTE releases in the solar wind). These observations give a new way of analyzing ultra-fast dust particles incident on a spacecraft. |
doi_str_mv | 10.1029/GL017i011p01809 |
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M. ; Glassmeier, K.-H. ; Coates, A. J. ; Goldstein, R. ; Acuña, M. H. ; Musmann, G.</creator><creatorcontrib>Neubauer, F. M. ; Glassmeier, K.-H. ; Coates, A. J. ; Goldstein, R. ; Acuña, M. H. ; Musmann, G.</creatorcontrib><description>This paper describes 13 very short events in the magnetic field of the inner magnetic pile-up region of Comet Halley observed by the Giotto magnetometer experiment together with simultaneous plasma data obtained by the Johnstone plasma analyzer and the ion mass spectrometer experiments. The events are due to dust impacts in the milligram range on the spacecraft at the relative velocity between the cometary dust and the spacecraft of 68 km/sec. They are generally consistent with dust impact events derived from spacecraft attitude perturbations by the Giotto camera. Their characteristic shape generally involves a sudden decrease in magnetic-field magnitude, a subsequent overshoot beyond initial field values, and an asymptotic approach to the initial field (somewhat reminiscent of the magnetic-field signature after the AMPTE releases in the solar wind). These observations give a new way of analyzing ultra-fast dust particles incident on a spacecraft.</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/GL017i011p01809</identifier><identifier>CODEN: GPRLAJ</identifier><language>eng</language><publisher>Legacy CDMS: Blackwell Publishing Ltd</publisher><subject>640107 - Astrophysics & Cosmology- Planetary Phenomena ; Analyzers ; Astronomy ; Astrophysics ; Asymptotic properties ; Cemeteries ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; COLLISIONS ; COMETS ; COSMIC DUST ; DATA ; DISTRIBUTION ; DISTURBANCES ; Dust ; DUSTS ; Earth, ocean, space ; ENVIRONMENT ; Exact sciences and technology ; HALLEY COMET ; Halley's comet ; INFORMATION ; Interplanetary space ; MAGNETIC FIELDS ; MASS SPECTROMETERS ; MEASURING INSTRUMENTS ; SATELLITES ; SIZE ; Solar system ; Spacecraft ; SPATIAL DISTRIBUTION ; SPECTROMETERS</subject><ispartof>Geophysical research letters, 1990-10, Vol.17 (11), p.1809-1812</ispartof><rights>Copyright 1990 by the American Geophysical Union.</rights><rights>1991 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c5408-7b045c4430e6fc31a8bf171b8f6eb9dfc46a91e4fc9e85e522a17e547be8a5643</citedby><cites>FETCH-LOGICAL-c5408-7b045c4430e6fc31a8bf171b8f6eb9dfc46a91e4fc9e85e522a17e547be8a5643</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2FGL017i011p01809$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2FGL017i011p01809$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>230,314,776,780,881,1411,27901,27902,45550,45551</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=19406971$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/5392414$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Neubauer, F. M.</creatorcontrib><creatorcontrib>Glassmeier, K.-H.</creatorcontrib><creatorcontrib>Coates, A. J.</creatorcontrib><creatorcontrib>Goldstein, R.</creatorcontrib><creatorcontrib>Acuña, M. H.</creatorcontrib><creatorcontrib>Musmann, G.</creatorcontrib><title>Hypervelocity dust particle impacts observed by the Giotto Magnetometer and Plasma Experiments</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>This paper describes 13 very short events in the magnetic field of the inner magnetic pile-up region of Comet Halley observed by the Giotto magnetometer experiment together with simultaneous plasma data obtained by the Johnstone plasma analyzer and the ion mass spectrometer experiments. The events are due to dust impacts in the milligram range on the spacecraft at the relative velocity between the cometary dust and the spacecraft of 68 km/sec. They are generally consistent with dust impact events derived from spacecraft attitude perturbations by the Giotto camera. Their characteristic shape generally involves a sudden decrease in magnetic-field magnitude, a subsequent overshoot beyond initial field values, and an asymptotic approach to the initial field (somewhat reminiscent of the magnetic-field signature after the AMPTE releases in the solar wind). These observations give a new way of analyzing ultra-fast dust particles incident on a spacecraft.</description><subject>640107 - Astrophysics & Cosmology- Planetary Phenomena</subject><subject>Analyzers</subject><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Asymptotic properties</subject><subject>Cemeteries</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>COLLISIONS</subject><subject>COMETS</subject><subject>COSMIC DUST</subject><subject>DATA</subject><subject>DISTRIBUTION</subject><subject>DISTURBANCES</subject><subject>Dust</subject><subject>DUSTS</subject><subject>Earth, ocean, space</subject><subject>ENVIRONMENT</subject><subject>Exact sciences and technology</subject><subject>HALLEY COMET</subject><subject>Halley's comet</subject><subject>INFORMATION</subject><subject>Interplanetary space</subject><subject>MAGNETIC FIELDS</subject><subject>MASS SPECTROMETERS</subject><subject>MEASURING INSTRUMENTS</subject><subject>SATELLITES</subject><subject>SIZE</subject><subject>Solar system</subject><subject>Spacecraft</subject><subject>SPATIAL DISTRIBUTION</subject><subject>SPECTROMETERS</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1990</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNqFkEtv1DAURiMEEkNhzYaFhYTEJvQ6sWN7iUpJC8NDVYEdluO5oYbEDranNP-ejFKBxIaVr-TznfsoiscUXlCo1HG7BSocUDoBlaDuFBuqGCslgLhbbADUUleiuV88SOk7ANRQ003x9WyeMF7jEKzLM9ntUyaTidnZAYkbJ2NzIqFLB2ZHupnkKyStCzkH8s5885jDiBkjMX5HPg4mjYac3ixKN6LP6WFxrzdDwke371Hx6fXp5clZuf3Qnp-83JaWM5Cl6IBxy1gN2PS2pkZ2PRW0k32Dndr1ljVGUWS9VSg58qoyVCBnokNpeMPqo-Lp6g0pO52WXdBe2eA92qx5rSpGD9DzFZpi-LnHlPXoksVhMB7DPmnKK6UqKRlf0OMVtTGkFLHX07KRibOmoA_n1v-ce0k8u5WbZM3QR-OtS39jikGjBF04tnK_3IDz_7S6vdhyYHKJPVlj3iSjfY7LuEpRgKph1aF7uX67lPHmj9XEH7oRteD6y_tWX8q3r95cQKs_178BSlenqw</recordid><startdate>199010</startdate><enddate>199010</enddate><creator>Neubauer, F. M.</creator><creator>Glassmeier, K.-H.</creator><creator>Coates, A. J.</creator><creator>Goldstein, R.</creator><creator>Acuña, M. H.</creator><creator>Musmann, G.</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><scope>BSCLL</scope><scope>CYE</scope><scope>CYI</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>KR7</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>199010</creationdate><title>Hypervelocity dust particle impacts observed by the Giotto Magnetometer and Plasma Experiments</title><author>Neubauer, F. M. ; Glassmeier, K.-H. ; Coates, A. J. ; Goldstein, R. ; Acuña, M. H. ; Musmann, G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c5408-7b045c4430e6fc31a8bf171b8f6eb9dfc46a91e4fc9e85e522a17e547be8a5643</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1990</creationdate><topic>640107 - Astrophysics & Cosmology- Planetary Phenomena</topic><topic>Analyzers</topic><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Asymptotic properties</topic><topic>Cemeteries</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>COLLISIONS</topic><topic>COMETS</topic><topic>COSMIC DUST</topic><topic>DATA</topic><topic>DISTRIBUTION</topic><topic>DISTURBANCES</topic><topic>Dust</topic><topic>DUSTS</topic><topic>Earth, ocean, space</topic><topic>ENVIRONMENT</topic><topic>Exact sciences and technology</topic><topic>HALLEY COMET</topic><topic>Halley's comet</topic><topic>INFORMATION</topic><topic>Interplanetary space</topic><topic>MAGNETIC FIELDS</topic><topic>MASS SPECTROMETERS</topic><topic>MEASURING INSTRUMENTS</topic><topic>SATELLITES</topic><topic>SIZE</topic><topic>Solar system</topic><topic>Spacecraft</topic><topic>SPATIAL DISTRIBUTION</topic><topic>SPECTROMETERS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Neubauer, F. M.</creatorcontrib><creatorcontrib>Glassmeier, K.-H.</creatorcontrib><creatorcontrib>Coates, A. J.</creatorcontrib><creatorcontrib>Goldstein, R.</creatorcontrib><creatorcontrib>Acuña, M. H.</creatorcontrib><creatorcontrib>Musmann, G.</creatorcontrib><collection>Istex</collection><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Civil Engineering Abstracts</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Neubauer, F. M.</au><au>Glassmeier, K.-H.</au><au>Coates, A. J.</au><au>Goldstein, R.</au><au>Acuña, M. H.</au><au>Musmann, G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Hypervelocity dust particle impacts observed by the Giotto Magnetometer and Plasma Experiments</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>1990-10</date><risdate>1990</risdate><volume>17</volume><issue>11</issue><spage>1809</spage><epage>1812</epage><pages>1809-1812</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>This paper describes 13 very short events in the magnetic field of the inner magnetic pile-up region of Comet Halley observed by the Giotto magnetometer experiment together with simultaneous plasma data obtained by the Johnstone plasma analyzer and the ion mass spectrometer experiments. The events are due to dust impacts in the milligram range on the spacecraft at the relative velocity between the cometary dust and the spacecraft of 68 km/sec. They are generally consistent with dust impact events derived from spacecraft attitude perturbations by the Giotto camera. Their characteristic shape generally involves a sudden decrease in magnetic-field magnitude, a subsequent overshoot beyond initial field values, and an asymptotic approach to the initial field (somewhat reminiscent of the magnetic-field signature after the AMPTE releases in the solar wind). These observations give a new way of analyzing ultra-fast dust particles incident on a spacecraft.</abstract><cop>Legacy CDMS</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/GL017i011p01809</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record> |
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subjects | 640107 - Astrophysics & Cosmology- Planetary Phenomena Analyzers Astronomy Astrophysics Asymptotic properties Cemeteries CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COLLISIONS COMETS COSMIC DUST DATA DISTRIBUTION DISTURBANCES Dust DUSTS Earth, ocean, space ENVIRONMENT Exact sciences and technology HALLEY COMET Halley's comet INFORMATION Interplanetary space MAGNETIC FIELDS MASS SPECTROMETERS MEASURING INSTRUMENTS SATELLITES SIZE Solar system Spacecraft SPATIAL DISTRIBUTION SPECTROMETERS |
title | Hypervelocity dust particle impacts observed by the Giotto Magnetometer and Plasma Experiments |
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