Loading…
Atomic oxygen 3P → 3S0 (λ1304Å) transition revisited : Cross section near threshold
The direct excitation cross section for the atomic oxygen 3P -- > 3S0 transition (1304 A) has been measured at four incident energies between 13.4 and 40 eV. These measurements were made to add sufficient detail to previous direct excitation measurements to allow the near-threshold cross section...
Saved in:
Published in: | Journal of Geophysical Research 2001, Vol.106 (A1), p.203-209 |
---|---|
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 | 209 |
container_issue | A1 |
container_start_page | 203 |
container_title | Journal of Geophysical Research |
container_volume | 106 |
creator | DOERING, J. P YANG, J |
description | The direct excitation cross section for the atomic oxygen 3P -- > 3S0 transition (1304 A) has been measured at four incident energies between 13.4 and 40 eV. These measurements were made to add sufficient detail to previous direct excitation measurements to allow the near-threshold cross section to be determined. Previous optical measurements of the 1304 A emission cross section disagree by up to a factor of two in this important energy region. We have also compared the atomic hydrogen e + H(1s) -- > H(2s + 2p) cross section, used previously as a secondary standard for our direct excitation measurements of atomic oxygen cross sections, to recent measurements of the total e + H -- > Lyman alpha cross section and have found agreement at the +/- 15 percent level, making a revision of our previously reported atomic oxygen cross sections unnecessary. The new direct excitation atomic oxygen cross section results, combined with previous measurements, support the emission cross section measured by Stone and Zipf (1974) and revised by Zipf and Erdman (1985) over the measurement of Wang and McConkey (1992). Except for the region just above threshold at 10-25 eV incident energy, all the cross section measurements now agree to within +/- 20 percent. The 100 eV value of the atomic oxygen 3P -- > 3SO emission cross section from a combination of the emission and direct excitation cross section experiments is 8.6 +/- 11 percent x 10 exp -18 sq cm. (Author) |
format | article |
fullrecord | <record><control><sourceid>proquest_pasca</sourceid><recordid>TN_cdi_proquest_miscellaneous_26998535</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>26998535</sourcerecordid><originalsourceid>FETCH-LOGICAL-p595-e8ac72a4038ed93622d54ba6fb03a2e8171887632f4ecab9fc11d91f1cd106ed3</originalsourceid><addsrcrecordid>eNotj01KAzEcxYMoWGrvEBBEFwP5nsRdKX5BQcGCyyGT_MdGppOaTMUeQA_gdVy69xCexEH7Nu_B-_Hg7aERo1IVjBG2j0aECl0QxspDNMn5iQwSUglCR-hh2sdVcDi-bh-hw_wO_7x_YH5P8On3J-VEfL2d4T7ZLoc-xA4neAlDBI_P8SzFnHEG99d0YBPulwnyMrb-CB00ts0w2fkYLS4vFrPrYn57dTObzou1NLIAbV3JrCBcgzdcMealqK1qasItA01LqnWpOGsEOFubxlHqDW2o85Qo8HyMTv5n1yk-byD31SpkB21rO4ibXDFljJZcDuDxDrTZ2bYZHrmQq3UKK5u2lTZSMcl_AcVuXQw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>26998535</pqid></control><display><type>article</type><title>Atomic oxygen 3P → 3S0 (λ1304Å) transition revisited : Cross section near threshold</title><source>Wiley Online Library AGU Free Content</source><creator>DOERING, J. P ; YANG, J</creator><creatorcontrib>DOERING, J. P ; YANG, J</creatorcontrib><description>The direct excitation cross section for the atomic oxygen 3P -- > 3S0 transition (1304 A) has been measured at four incident energies between 13.4 and 40 eV. These measurements were made to add sufficient detail to previous direct excitation measurements to allow the near-threshold cross section to be determined. Previous optical measurements of the 1304 A emission cross section disagree by up to a factor of two in this important energy region. We have also compared the atomic hydrogen e + H(1s) -- > H(2s + 2p) cross section, used previously as a secondary standard for our direct excitation measurements of atomic oxygen cross sections, to recent measurements of the total e + H -- > Lyman alpha cross section and have found agreement at the +/- 15 percent level, making a revision of our previously reported atomic oxygen cross sections unnecessary. The new direct excitation atomic oxygen cross section results, combined with previous measurements, support the emission cross section measured by Stone and Zipf (1974) and revised by Zipf and Erdman (1985) over the measurement of Wang and McConkey (1992). Except for the region just above threshold at 10-25 eV incident energy, all the cross section measurements now agree to within +/- 20 percent. The 100 eV value of the atomic oxygen 3P -- > 3SO emission cross section from a combination of the emission and direct excitation cross section experiments is 8.6 +/- 11 percent x 10 exp -18 sq cm. (Author)</description><identifier>ISSN: 0148-0227</identifier><identifier>EISSN: 2156-2202</identifier><language>eng</language><publisher>Washington, DC: American Geophysical Union</publisher><subject>Airglow. Aurora ; Earth, ocean, space ; Exact sciences and technology ; External geophysics ; Physics of the high neutral atmosphere</subject><ispartof>Journal of Geophysical Research, 2001, Vol.106 (A1), p.203-209</ispartof><rights>2001 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,4021</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=895625$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>DOERING, J. P</creatorcontrib><creatorcontrib>YANG, J</creatorcontrib><title>Atomic oxygen 3P → 3S0 (λ1304Å) transition revisited : Cross section near threshold</title><title>Journal of Geophysical Research</title><description>The direct excitation cross section for the atomic oxygen 3P -- > 3S0 transition (1304 A) has been measured at four incident energies between 13.4 and 40 eV. These measurements were made to add sufficient detail to previous direct excitation measurements to allow the near-threshold cross section to be determined. Previous optical measurements of the 1304 A emission cross section disagree by up to a factor of two in this important energy region. We have also compared the atomic hydrogen e + H(1s) -- > H(2s + 2p) cross section, used previously as a secondary standard for our direct excitation measurements of atomic oxygen cross sections, to recent measurements of the total e + H -- > Lyman alpha cross section and have found agreement at the +/- 15 percent level, making a revision of our previously reported atomic oxygen cross sections unnecessary. The new direct excitation atomic oxygen cross section results, combined with previous measurements, support the emission cross section measured by Stone and Zipf (1974) and revised by Zipf and Erdman (1985) over the measurement of Wang and McConkey (1992). Except for the region just above threshold at 10-25 eV incident energy, all the cross section measurements now agree to within +/- 20 percent. The 100 eV value of the atomic oxygen 3P -- > 3SO emission cross section from a combination of the emission and direct excitation cross section experiments is 8.6 +/- 11 percent x 10 exp -18 sq cm. (Author)</description><subject>Airglow. Aurora</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Physics of the high neutral atmosphere</subject><issn>0148-0227</issn><issn>2156-2202</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2001</creationdate><recordtype>article</recordtype><recordid>eNotj01KAzEcxYMoWGrvEBBEFwP5nsRdKX5BQcGCyyGT_MdGppOaTMUeQA_gdVy69xCexEH7Nu_B-_Hg7aERo1IVjBG2j0aECl0QxspDNMn5iQwSUglCR-hh2sdVcDi-bh-hw_wO_7x_YH5P8On3J-VEfL2d4T7ZLoc-xA4neAlDBI_P8SzFnHEG99d0YBPulwnyMrb-CB00ts0w2fkYLS4vFrPrYn57dTObzou1NLIAbV3JrCBcgzdcMealqK1qasItA01LqnWpOGsEOFubxlHqDW2o85Qo8HyMTv5n1yk-byD31SpkB21rO4ibXDFljJZcDuDxDrTZ2bYZHrmQq3UKK5u2lTZSMcl_AcVuXQw</recordid><startdate>2001</startdate><enddate>2001</enddate><creator>DOERING, J. P</creator><creator>YANG, J</creator><general>American Geophysical Union</general><scope>IQODW</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>2001</creationdate><title>Atomic oxygen 3P → 3S0 (λ1304Å) transition revisited : Cross section near threshold</title><author>DOERING, J. P ; YANG, J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p595-e8ac72a4038ed93622d54ba6fb03a2e8171887632f4ecab9fc11d91f1cd106ed3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2001</creationdate><topic>Airglow. Aurora</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>External geophysics</topic><topic>Physics of the high neutral atmosphere</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>DOERING, J. P</creatorcontrib><creatorcontrib>YANG, J</creatorcontrib><collection>Pascal-Francis</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of Geophysical Research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>DOERING, J. P</au><au>YANG, J</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Atomic oxygen 3P → 3S0 (λ1304Å) transition revisited : Cross section near threshold</atitle><jtitle>Journal of Geophysical Research</jtitle><date>2001</date><risdate>2001</risdate><volume>106</volume><issue>A1</issue><spage>203</spage><epage>209</epage><pages>203-209</pages><issn>0148-0227</issn><eissn>2156-2202</eissn><abstract>The direct excitation cross section for the atomic oxygen 3P -- > 3S0 transition (1304 A) has been measured at four incident energies between 13.4 and 40 eV. These measurements were made to add sufficient detail to previous direct excitation measurements to allow the near-threshold cross section to be determined. Previous optical measurements of the 1304 A emission cross section disagree by up to a factor of two in this important energy region. We have also compared the atomic hydrogen e + H(1s) -- > H(2s + 2p) cross section, used previously as a secondary standard for our direct excitation measurements of atomic oxygen cross sections, to recent measurements of the total e + H -- > Lyman alpha cross section and have found agreement at the +/- 15 percent level, making a revision of our previously reported atomic oxygen cross sections unnecessary. The new direct excitation atomic oxygen cross section results, combined with previous measurements, support the emission cross section measured by Stone and Zipf (1974) and revised by Zipf and Erdman (1985) over the measurement of Wang and McConkey (1992). Except for the region just above threshold at 10-25 eV incident energy, all the cross section measurements now agree to within +/- 20 percent. The 100 eV value of the atomic oxygen 3P -- > 3SO emission cross section from a combination of the emission and direct excitation cross section experiments is 8.6 +/- 11 percent x 10 exp -18 sq cm. (Author)</abstract><cop>Washington, DC</cop><pub>American Geophysical Union</pub><tpages>7</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0148-0227 |
ispartof | Journal of Geophysical Research, 2001, Vol.106 (A1), p.203-209 |
issn | 0148-0227 2156-2202 |
language | eng |
recordid | cdi_proquest_miscellaneous_26998535 |
source | Wiley Online Library AGU Free Content |
subjects | Airglow. Aurora Earth, ocean, space Exact sciences and technology External geophysics Physics of the high neutral atmosphere |
title | Atomic oxygen 3P → 3S0 (λ1304Å) transition revisited : Cross section near threshold |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-14T15%3A03%3A12IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_pasca&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Atomic%20oxygen%203P%20%E2%86%92%203S0%20(%CE%BB1304%C3%85)%20transition%20revisited%20:%20Cross%20section%20near%20threshold&rft.jtitle=Journal%20of%20Geophysical%20Research&rft.au=DOERING,%20J.%20P&rft.date=2001&rft.volume=106&rft.issue=A1&rft.spage=203&rft.epage=209&rft.pages=203-209&rft.issn=0148-0227&rft.eissn=2156-2202&rft_id=info:doi/&rft_dat=%3Cproquest_pasca%3E26998535%3C/proquest_pasca%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-p595-e8ac72a4038ed93622d54ba6fb03a2e8171887632f4ecab9fc11d91f1cd106ed3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=26998535&rft_id=info:pmid/&rfr_iscdi=true |