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  1. 原著論文

Effect of number of views on cross-sectional Compton imaging: A fundamental study with backprojection

https://repo.qst.go.jp/records/49337
https://repo.qst.go.jp/records/49337
c016710a-413e-46ea-8c77-7029e52f5e5f
Item type 学術雑誌論文 / Journal Article(1)
公開日 2018-12-18
タイトル
タイトル Effect of number of views on cross-sectional Compton imaging: A fundamental study with backprojection
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
アクセス権
アクセス権 metadata only access
アクセス権URI http://purl.org/coar/access_right/c_14cb
著者 Sakai, Makoto

× Sakai, Makoto

WEKO 497975

Sakai, Makoto

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Raj, kumar Parajuli

× Raj, kumar Parajuli

WEKO 497976

Raj, kumar Parajuli

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Kikuchi, Mikiko

× Kikuchi, Mikiko

WEKO 497977

Kikuchi, Mikiko

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Yamaguchi, Mitsutaka

× Yamaguchi, Mitsutaka

WEKO 497978

Yamaguchi, Mitsutaka

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Nagao, Yuto

× Nagao, Yuto

WEKO 497979

Nagao, Yuto

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Kawachi, Naoki

× Kawachi, Naoki

WEKO 497980

Kawachi, Naoki

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Arakawa, Kazuo

× Arakawa, Kazuo

WEKO 497981

Arakawa, Kazuo

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Nakano, (Gunma Univ.) Takashi

× Nakano, (Gunma Univ.) Takashi

WEKO 497982

Nakano, (Gunma Univ.) Takashi

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酒井 真理

× 酒井 真理

WEKO 497983

en 酒井 真理

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ラジュ クマル パラジュリ

× ラジュ クマル パラジュリ

WEKO 497984

en ラジュ クマル パラジュリ

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菊地 美貴子

× 菊地 美貴子

WEKO 497985

en 菊地 美貴子

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山口 充孝

× 山口 充孝

WEKO 497986

en 山口 充孝

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長尾 悠人

× 長尾 悠人

WEKO 497987

en 長尾 悠人

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河地 有木

× 河地 有木

WEKO 497988

en 河地 有木

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荒川 和夫

× 荒川 和夫

WEKO 497989

en 荒川 和夫

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抄録
内容記述タイプ Abstract
内容記述 Introduction: We have been developing a medical imaging technique using a Compton camera, which is expected to reconstruct three-dimensional images. If the number of views is not sufficient, star-shaped artifacts (streak artifacts) could arise in cross-sectional images. Therefore, we estimated the point spread function (PSF) of cross-sectional Compton images and the effect of the number of views by Monte Carlo simulations and experimental studies.
Materials and Methods: A cross-sectional Compton image was reconstructed using a dataset comprising 719 view directions and PSF was analyzed using a radial distribution. The peak height, full width at half maximum (FWHM), background (BG), and residual sum of squares (RSS) were calculated from the obtained PSF. In addition, RSSs were plotted against the number of views to estimate the required number to suppress star-shaped artifacts.
Results: There was no correlation found between the number of views and both FWHM (16 mm) and peak/BG ratio (~1×10^4). RSSs were reduced with the number of views and approached the minimum asymptotically. Correlation was observed between the required number of views and the number of Compton events used for image reconstruction.
Conclusion: We determined the PSF of cross-sectional Compton images and the effect of the number of views on the images. The required number of views to suppress the star-shaped artifact is related to the square root of the number of Compton events used to reconstruct the image. From this study, we concluded that 21 or more views are required for clinical purposes.
書誌情報 Physica Medica

巻 56, p. 1-9, 発行日 2018-11
出版者
出版者 Elsevier
ISSN
収録物識別子タイプ ISSN
収録物識別子 1120-1797
DOI
識別子タイプ DOI
関連識別子 10.1016/j.ejmp.2018.11.006
関連サイト
識別子タイプ DOI
関連識別子 https://doi.org/10.1016/j.ejmp.2018.11.006
関連名称 https://doi.org/10.1016/j.ejmp.2018.11.006
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