Solar flare soft X-ray spectra from Diogeness observations

Diogeness was an uncollimated scanning flat crystal spectrometer observing solar flare X-ray spectra in four narrow wavelength bands in the vicinity of Ca xix, S xv and Si xiii He-like line ‘triplets’ around 3.18 Å, 5.04 Å and 6.65 Å. In two of the spectral channels, emission lines around the Ca xix...

Full description

Saved in:
Bibliographic Details
Published in:Proceedings of the International Astronomical Union 2015-08, Vol.11 (S320), p.109-111
Main Authors: Stȩślicki, Marek, Sylwester, Janusz, Sylwester, Barbara, Szaforz, Żaneta, Kordylewski, Zbigniew, Płocieniak, Stefan, Siarkowski, Marek, Phillips, Kenneth J. H.
Format: Article
Language:English
Subjects:
Analysis
Channels
Contributed Papers
Corona
Flares
Gamma rays
Solar flares
Spectra
Spectral emissivity
Spectral lines
Spectrometers
Spectrum analysis
Studies
Tachometers
X-rays
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page 111
container_issue S320
container_start_page 109
container_title Proceedings of the International Astronomical Union
container_volume 11
creator Stȩślicki, Marek
Sylwester, Janusz
Sylwester, Barbara
Szaforz, Żaneta
Kordylewski, Zbigniew
Płocieniak, Stefan
Siarkowski, Marek
Phillips, Kenneth J. H.
description Diogeness was an uncollimated scanning flat crystal spectrometer observing solar flare X-ray spectra in four narrow wavelength bands in the vicinity of Ca xix, S xv and Si xiii He-like line ‘triplets’ around 3.18 Å, 5.04 Å and 6.65 Å. In two of the spectral channels, emission lines around the Ca xix 3.178 Å resonance line were scanned in opposite directions, being diffracted from precisely adjusted identical Quartz crystals mounted on a common shaft in a so-called Dopplerometer (tachometer) configuration. Observations of solar X-ray spectra made by Diogeness provide a direct diagnostic information on plasma characteristics during the impulsive flare energy release. We present a sample of events which occurred during the Diogeness operation time from August 16, 2001 to September 17, 2001.
doi_str_mv 10.1017/S1743921316000314
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1880008087</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cupid>10_1017_S1743921316000314</cupid><sourcerecordid>1859481342</sourcerecordid><originalsourceid>FETCH-LOGICAL-c378t-de96247aeedc3bec69ca061412e130bc65b3a44b88595c76c9d0390d4f3037283</originalsourceid><addsrcrecordid>eNqNkE9Lw0AQxRdRsFY_gLeAFy_RnZ1Ndteb1L8geKiCt7DZTEpKmq27qdBvb0qLiCJ4mRmG33vwHmOnwC-Ag7qcgpJoBCDknHMEucdGm1dqhID9rxvwkB3FOOdc5hqzEbua-taGpB4GJdHXffKWBrtO4pJcH2xSB79Ibho_o45iTHwZKXzYvvFdPGYHtW0jnez2mL3e3b5MHtKn5_vHyfVT6lDpPq3I5EIqS1Q5LMnlxlmegwRBgLx0eVailbLUOjOZU7kzFUfDK1kjRyU0jtn51ncZ_PuKYl8smuiobW1HfhUL0HqIrLlW_0AzIzWgFAN69gOd-1XohiAbKhMGlckGCraUCz7GQHWxDM3ChnUBvNgUX_wqftDgTmMXZWiqGX2z_lP1CXqkgkU</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1855293795</pqid></control><display><type>article</type><title>Solar flare soft X-ray spectra from Diogeness observations</title><source>Cambridge University Press</source><creator>Stȩślicki, Marek ; Sylwester, Janusz ; Sylwester, Barbara ; Szaforz, Żaneta ; Kordylewski, Zbigniew ; Płocieniak, Stefan ; Siarkowski, Marek ; Phillips, Kenneth J. H.</creator><creatorcontrib>Stȩślicki, Marek ; Sylwester, Janusz ; Sylwester, Barbara ; Szaforz, Żaneta ; Kordylewski, Zbigniew ; Płocieniak, Stefan ; Siarkowski, Marek ; Phillips, Kenneth J. H.</creatorcontrib><description>Diogeness was an uncollimated scanning flat crystal spectrometer observing solar flare X-ray spectra in four narrow wavelength bands in the vicinity of Ca xix, S xv and Si xiii He-like line ‘triplets’ around 3.18 Å, 5.04 Å and 6.65 Å. In two of the spectral channels, emission lines around the Ca xix 3.178 Å resonance line were scanned in opposite directions, being diffracted from precisely adjusted identical Quartz crystals mounted on a common shaft in a so-called Dopplerometer (tachometer) configuration. Observations of solar X-ray spectra made by Diogeness provide a direct diagnostic information on plasma characteristics during the impulsive flare energy release. We present a sample of events which occurred during the Diogeness operation time from August 16, 2001 to September 17, 2001.</description><identifier>ISSN: 1743-9213</identifier><identifier>EISSN: 1743-9221</identifier><identifier>DOI: 10.1017/S1743921316000314</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Analysis ; Channels ; Contributed Papers ; Corona ; Flares ; Gamma rays ; Solar flares ; Spectra ; Spectral emissivity ; Spectral lines ; Spectrometers ; Spectrum analysis ; Studies ; Tachometers ; X-rays</subject><ispartof>Proceedings of the International Astronomical Union, 2015-08, Vol.11 (S320), p.109-111</ispartof><rights>Copyright © International Astronomical Union 2016</rights><lds50>peer_reviewed</lds50><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.cambridge.org/core/product/identifier/S1743921316000314/type/journal_article$$EHTML$$P50$$Gcambridge$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,72960</link.rule.ids></links><search><creatorcontrib>Stȩślicki, Marek</creatorcontrib><creatorcontrib>Sylwester, Janusz</creatorcontrib><creatorcontrib>Sylwester, Barbara</creatorcontrib><creatorcontrib>Szaforz, Żaneta</creatorcontrib><creatorcontrib>Kordylewski, Zbigniew</creatorcontrib><creatorcontrib>Płocieniak, Stefan</creatorcontrib><creatorcontrib>Siarkowski, Marek</creatorcontrib><creatorcontrib>Phillips, Kenneth J. H.</creatorcontrib><title>Solar flare soft X-ray spectra from Diogeness observations</title><title>Proceedings of the International Astronomical Union</title><addtitle>Proc. IAU</addtitle><description>Diogeness was an uncollimated scanning flat crystal spectrometer observing solar flare X-ray spectra in four narrow wavelength bands in the vicinity of Ca xix, S xv and Si xiii He-like line ‘triplets’ around 3.18 Å, 5.04 Å and 6.65 Å. In two of the spectral channels, emission lines around the Ca xix 3.178 Å resonance line were scanned in opposite directions, being diffracted from precisely adjusted identical Quartz crystals mounted on a common shaft in a so-called Dopplerometer (tachometer) configuration. Observations of solar X-ray spectra made by Diogeness provide a direct diagnostic information on plasma characteristics during the impulsive flare energy release. We present a sample of events which occurred during the Diogeness operation time from August 16, 2001 to September 17, 2001.</description><subject>Analysis</subject><subject>Channels</subject><subject>Contributed Papers</subject><subject>Corona</subject><subject>Flares</subject><subject>Gamma rays</subject><subject>Solar flares</subject><subject>Spectra</subject><subject>Spectral emissivity</subject><subject>Spectral lines</subject><subject>Spectrometers</subject><subject>Spectrum analysis</subject><subject>Studies</subject><subject>Tachometers</subject><subject>X-rays</subject><issn>1743-9213</issn><issn>1743-9221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqNkE9Lw0AQxRdRsFY_gLeAFy_RnZ1Ndteb1L8geKiCt7DZTEpKmq27qdBvb0qLiCJ4mRmG33vwHmOnwC-Ag7qcgpJoBCDknHMEucdGm1dqhID9rxvwkB3FOOdc5hqzEbua-taGpB4GJdHXffKWBrtO4pJcH2xSB79Ibho_o45iTHwZKXzYvvFdPGYHtW0jnez2mL3e3b5MHtKn5_vHyfVT6lDpPq3I5EIqS1Q5LMnlxlmegwRBgLx0eVailbLUOjOZU7kzFUfDK1kjRyU0jtn51ncZ_PuKYl8smuiobW1HfhUL0HqIrLlW_0AzIzWgFAN69gOd-1XohiAbKhMGlckGCraUCz7GQHWxDM3ChnUBvNgUX_wqftDgTmMXZWiqGX2z_lP1CXqkgkU</recordid><startdate>20150801</startdate><enddate>20150801</enddate><creator>Stȩślicki, Marek</creator><creator>Sylwester, Janusz</creator><creator>Sylwester, Barbara</creator><creator>Szaforz, Żaneta</creator><creator>Kordylewski, Zbigniew</creator><creator>Płocieniak, Stefan</creator><creator>Siarkowski, Marek</creator><creator>Phillips, Kenneth J. H.</creator><general>Cambridge University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20150801</creationdate><title>Solar flare soft X-ray spectra from Diogeness observations</title><author>Stȩślicki, Marek ; Sylwester, Janusz ; Sylwester, Barbara ; Szaforz, Żaneta ; Kordylewski, Zbigniew ; Płocieniak, Stefan ; Siarkowski, Marek ; Phillips, Kenneth J. H.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c378t-de96247aeedc3bec69ca061412e130bc65b3a44b88595c76c9d0390d4f3037283</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Analysis</topic><topic>Channels</topic><topic>Contributed Papers</topic><topic>Corona</topic><topic>Flares</topic><topic>Gamma rays</topic><topic>Solar flares</topic><topic>Spectra</topic><topic>Spectral emissivity</topic><topic>Spectral lines</topic><topic>Spectrometers</topic><topic>Spectrum analysis</topic><topic>Studies</topic><topic>Tachometers</topic><topic>X-rays</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Stȩślicki, Marek</creatorcontrib><creatorcontrib>Sylwester, Janusz</creatorcontrib><creatorcontrib>Sylwester, Barbara</creatorcontrib><creatorcontrib>Szaforz, Żaneta</creatorcontrib><creatorcontrib>Kordylewski, Zbigniew</creatorcontrib><creatorcontrib>Płocieniak, Stefan</creatorcontrib><creatorcontrib>Siarkowski, Marek</creatorcontrib><creatorcontrib>Phillips, Kenneth J. H.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies &amp; Aerospace Database‎ (1962 - current)</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</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</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>ProQuest Central Basic</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><jtitle>Proceedings of the International Astronomical Union</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Stȩślicki, Marek</au><au>Sylwester, Janusz</au><au>Sylwester, Barbara</au><au>Szaforz, Żaneta</au><au>Kordylewski, Zbigniew</au><au>Płocieniak, Stefan</au><au>Siarkowski, Marek</au><au>Phillips, Kenneth J. H.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Solar flare soft X-ray spectra from Diogeness observations</atitle><jtitle>Proceedings of the International Astronomical Union</jtitle><addtitle>Proc. IAU</addtitle><date>2015-08-01</date><risdate>2015</risdate><volume>11</volume><issue>S320</issue><spage>109</spage><epage>111</epage><pages>109-111</pages><issn>1743-9213</issn><eissn>1743-9221</eissn><abstract>Diogeness was an uncollimated scanning flat crystal spectrometer observing solar flare X-ray spectra in four narrow wavelength bands in the vicinity of Ca xix, S xv and Si xiii He-like line ‘triplets’ around 3.18 Å, 5.04 Å and 6.65 Å. In two of the spectral channels, emission lines around the Ca xix 3.178 Å resonance line were scanned in opposite directions, being diffracted from precisely adjusted identical Quartz crystals mounted on a common shaft in a so-called Dopplerometer (tachometer) configuration. Observations of solar X-ray spectra made by Diogeness provide a direct diagnostic information on plasma characteristics during the impulsive flare energy release. We present a sample of events which occurred during the Diogeness operation time from August 16, 2001 to September 17, 2001.</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/S1743921316000314</doi><tpages>3</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1743-9213
ispartof Proceedings of the International Astronomical Union, 2015-08, Vol.11 (S320), p.109-111
issn 1743-9213
1743-9221
language eng
recordid cdi_proquest_miscellaneous_1880008087
source Cambridge University Press
subjects Analysis
Channels
Contributed Papers
Corona
Flares
Gamma rays
Solar flares
Spectra
Spectral emissivity
Spectral lines
Spectrometers
Spectrum analysis
Studies
Tachometers
X-rays
title Solar flare soft X-ray spectra from Diogeness observations
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T20%3A11%3A00IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Solar%20flare%20soft%20X-ray%20spectra%20from%20Diogeness%20observations&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.au=St%C8%A9%C5%9Blicki,%20Marek&rft.date=2015-08-01&rft.volume=11&rft.issue=S320&rft.spage=109&rft.epage=111&rft.pages=109-111&rft.issn=1743-9213&rft.eissn=1743-9221&rft_id=info:doi/10.1017/S1743921316000314&rft_dat=%3Cproquest_cross%3E1859481342%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c378t-de96247aeedc3bec69ca061412e130bc65b3a44b88595c76c9d0390d4f3037283%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1855293795&rft_id=info:pmid/&rft_cupid=10_1017_S1743921316000314&rfr_iscdi=true