Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap

We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clea...
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Autor*in:	Hiroyuki A. Sakaue [verfasserIn] Daiji Kato [verfasserIn] Norimasa Yamamoto [verfasserIn] Izumi Murakami [verfasserIn] Hirohisa Hara [verfasserIn] Nobuyuki Nakamura [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Solar transition region Solar corona Solar flares Solar ultraviolet emission Solar atmosphere Stellar atmospheres

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 943(2023), 1, p 14
Übergeordnetes Werk:	volume:943 ; year:2023 ; number:1, p 14

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/aca895

Katalog-ID:	DOAJ089166566

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520			\|a We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition.
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allfields	10.3847/1538-4357/aca895 doi (DE-627)DOAJ089166566 (DE-599)DOAJ69b2bb7f0d78434eb22d14458f46d86e DE-627 ger DE-627 rakwb eng QB460-466 Hiroyuki A. Sakaue verfasserin aut Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition. Solar transition region Solar corona Solar flares Solar ultraviolet emission Solar atmosphere Stellar atmospheres Astrophysics Daiji Kato verfasserin aut Norimasa Yamamoto verfasserin aut Izumi Murakami verfasserin aut Hirohisa Hara verfasserin aut Nobuyuki Nakamura verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 1, p 14 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:1, p 14 https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/article/69b2bb7f0d78434eb22d14458f46d86e kostenfrei https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 1, p 14
spelling	10.3847/1538-4357/aca895 doi (DE-627)DOAJ089166566 (DE-599)DOAJ69b2bb7f0d78434eb22d14458f46d86e DE-627 ger DE-627 rakwb eng QB460-466 Hiroyuki A. Sakaue verfasserin aut Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition. Solar transition region Solar corona Solar flares Solar ultraviolet emission Solar atmosphere Stellar atmospheres Astrophysics Daiji Kato verfasserin aut Norimasa Yamamoto verfasserin aut Izumi Murakami verfasserin aut Hirohisa Hara verfasserin aut Nobuyuki Nakamura verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 1, p 14 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:1, p 14 https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/article/69b2bb7f0d78434eb22d14458f46d86e kostenfrei https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 1, p 14
allfields_unstemmed	10.3847/1538-4357/aca895 doi (DE-627)DOAJ089166566 (DE-599)DOAJ69b2bb7f0d78434eb22d14458f46d86e DE-627 ger DE-627 rakwb eng QB460-466 Hiroyuki A. Sakaue verfasserin aut Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition. Solar transition region Solar corona Solar flares Solar ultraviolet emission Solar atmosphere Stellar atmospheres Astrophysics Daiji Kato verfasserin aut Norimasa Yamamoto verfasserin aut Izumi Murakami verfasserin aut Hirohisa Hara verfasserin aut Nobuyuki Nakamura verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 1, p 14 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:1, p 14 https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/article/69b2bb7f0d78434eb22d14458f46d86e kostenfrei https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 1, p 14
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allfieldsSound	10.3847/1538-4357/aca895 doi (DE-627)DOAJ089166566 (DE-599)DOAJ69b2bb7f0d78434eb22d14458f46d86e DE-627 ger DE-627 rakwb eng QB460-466 Hiroyuki A. Sakaue verfasserin aut Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition. Solar transition region Solar corona Solar flares Solar ultraviolet emission Solar atmosphere Stellar atmospheres Astrophysics Daiji Kato verfasserin aut Norimasa Yamamoto verfasserin aut Izumi Murakami verfasserin aut Hirohisa Hara verfasserin aut Nobuyuki Nakamura verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 1, p 14 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:1, p 14 https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/article/69b2bb7f0d78434eb22d14458f46d86e kostenfrei https://doi.org/10.3847/1538-4357/aca895 kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 1, p 14
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source	In The Astrophysical Journal 943(2023), 1, p 14 volume:943 year:2023 number:1, p 14
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authorswithroles_txt_mv	Hiroyuki A. Sakaue @@aut@@ Daiji Kato @@aut@@ Norimasa Yamamoto @@aut@@ Izumi Murakami @@aut@@ Hirohisa Hara @@aut@@ Nobuyuki Nakamura @@aut@@
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callnumber-first	Q - Science
author	Hiroyuki A. Sakaue
spellingShingle	Hiroyuki A. Sakaue misc QB460-466 misc Solar transition region misc Solar corona misc Solar flares misc Solar ultraviolet emission misc Solar atmosphere misc Stellar atmospheres misc Astrophysics Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap
authorStr	Hiroyuki A. Sakaue
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topic_title	QB460-466 Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap Solar transition region Solar corona Solar flares Solar ultraviolet emission Solar atmosphere Stellar atmospheres
topic	misc QB460-466 misc Solar transition region misc Solar corona misc Solar flares misc Solar ultraviolet emission misc Solar atmosphere misc Stellar atmospheres misc Astrophysics
topic_unstemmed	misc QB460-466 misc Solar transition region misc Solar corona misc Solar flares misc Solar ultraviolet emission misc Solar atmosphere misc Stellar atmospheres misc Astrophysics
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title	Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap
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title_full	Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap
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title_sort	energy dependence of the line ratio i(233.9 å)/i(243.8 å) in fe xv observed with an electron beam ion trap
callnumber	QB460-466
title_auth	Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap
abstract	We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition.
abstractGer	We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition.
abstract_unstemmed	We present the energy dependence of the intensity ratio between the 3 s 3 p ^3 P _2 —3 s 3 d ^3 D _3 transition at 233.9 Å and the 3 s 3 p ^1 P _1 —3 s 3 d ^1 D _2 transition at 243.8 Å in Fe xv studied with an electron beam ion trap over an energy range that spans resonance excitation regions. Clear resonance structures are observed in the electron energy range of 400–600 eV. The energy dependence obtained in the experiment is compared with a collisional-radiative model calculation, including resonance excitations, and overall agreement is found. It is shown that the ratio strongly reflects the population of the 3 s 3 p ^3 P _2 metastable state, which is the lower state of the 233.9 Å transition.
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title_short	Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap
url	https://doi.org/10.3847/1538-4357/aca895 https://doaj.org/article/69b2bb7f0d78434eb22d14458f46d86e https://doaj.org/toc/1538-4357
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Energy Dependence of the Line Ratio I(233.9 Å)/I(243.8 Å) in Fe xv Observed with an Electron Beam Ion Trap

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