Jove
Visualize
お問い合わせ
JoVE
x logofacebook logolinkedin logoyoutube logo
JoVEについて
概要リーダーシップブログJoVEヘルプセンター
著者向け
出版プロセス編集委員会範囲と方針査読よくある質問投稿
図書館員向け
推薦の声購読アクセスリソース図書館諮問委員会よくある質問
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experimentsアーカイブ
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教員リソースセンター教員サイト
利用規約
プライバシーポリシー
ポリシー

関連する概念動画

Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview01:02

Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview

Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material,  molecules absorb light depending on the energy required for electronic transitions. As a result...
UV–Vis Spectrometers01:14

UV–Vis Spectrometers

The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell. Samples for...
UV–Vis Spectroscopy: Molecular Electronic Transitions01:16

UV–Vis Spectroscopy: Molecular Electronic Transitions

In Ultraviolet–Visible (UV–Vis) spectroscopy, the absorption of electromagnetic radiation is used to probe the electronic structure of molecules. This technique provides insights into molecular electronic transitions, particularly the movement of electrons between different molecular orbitals. Radiation is absorbed if the energy of the electromagnetic radiation passing through the molecule is precisely equal to the energy difference between the excited and ground states. During this process,...
UV–Vis Spectrum01:30

UV–Vis Spectrum

When light passes through a substance, a portion of the light is absorbed while the remaining light is reflected or transmitted. If the molecule absorbs light between the wavelengths of 180–400 nm range, the UV spectrum is obtained, and if it absorbs light in the 400–780 nm wavelength range, the visible spectrum is obtained.     
The UV–Vis spectrum of a molecule is the plot of its absorbance versus wavelength. The plot is drawn by taking molar absorptivity (ε) or log ε on the y-axis (ordinate)...
UV–Vis Spectroscopy: Beer–Lambert Law01:09

UV–Vis Spectroscopy: Beer–Lambert Law

The Beer-Lambert law describes the relationship between absorbance and concentration, which combines the principles established by scientists Johann Heinrich Lambert and August Beer. Lambert's law states that when light passes through a medium, the loss in intensity is directly proportional to the original intensity and the path length of the light. Beer's law proposed that the transmittance of a solution remains constant if the product of concentration and path length is constant. The modern...
Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...

こちらも読む

関連記事

共著者、ジャーナル、引用グラフによってこの研究に関連する記事。

並び替え
Same author

THE TREATMENT OF DYSENTERY BY RECTAL INJECTIONS.

British medical journal·2010
Same author

Rocket-borne instrument with a high-resolution microchannel plate detector for planetary UV spectroscopy.

Applied optics·2010
Same author

Mariner 6 and 7 ultraviolet spectrometers.

Applied optics·2010
Same author

Planetary ultraviolet spectroscopy.

Applied optics·2010
Same author

Atmospheric scattering of the solar flux in the middle ultraviolet.

Applied optics·2010
Same author

Transcriptional profiling suggests that secondary and primary large B-cell lymphomas of the gastrointestinal (GI) tract are blastic variants of GI marginal zone lymphoma.

The Journal of pathology·2006

関連する実験動画

Updated: Jul 12, 2026

Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna
06:41

Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna

Published on: September 14, 2016

マリナー9号紫外線スペクトロメーター実験:恒星の観測

C F Lillie, R C Bohlin, M R Molnar

    Science (New York, N.Y.)
    |January 21, 1972
    PubMed
    まとめ

    初期のタイプの星の紫外線スペクトルは,主要な元素の線を明らかにします. マリナー9号のデータは,エネルギー分布が以前の観測値より約20%低いことを示しており,恒星の天体物理学研究に影響を与えている.

    科学分野:

    • 天文学と天体物理学について
    • ステラスペクトル顕微鏡 星のスペクトル顕微鏡

    背景:

    • 初期のタイプの星は,恒星の進化と銀河の組成を理解するために重要である.
    • 紫外線 (UV) スペクトロスコピーは,恒星の大気と組成に関するユニークな洞察を提供します.

    研究 の 目的:

    • 1100〜2000アングストームの範囲の初期のタイプの星の光学スペクトルを得るために.
    • 顕著なスペクトル線を特定し,これらの星の絶対エネルギー分布を分析する.

    主な方法:

    • マリナー9号の紫外線スペクトロメーターを利用して,星のスペクトルを捉えました.
    • 1100〜2000アンストームの波長領域に集中しています.

    主要な成果:

    • 水素I (H I),シリコンIV (Si IV),炭素IV (C IV) の共振線を成功裏に特定しました.
    • 炭素II (C II),炭素III (C III),シリコンIII (Si III),鉄II (Fe II),および窒素IV (N IV) から検出されたスペクトル特徴.
    • 抽出した絶対エネルギー分布は,OAO-2で得られたものより約20%低く,1200-2000アングストームの範囲で得られた.

    結論:

    さらに関連する動画

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media
    05:16

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media

    Published on: October 25, 2021

    Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation
    09:53

    Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation

    Published on: October 30, 2012

    関連する実験動画

    Last Updated: Jul 12, 2026

    Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna
    06:41

    Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna

    Published on: September 14, 2016

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media
    05:16

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media

    Published on: October 25, 2021

    Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation
    09:53

    Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation

    Published on: October 30, 2012

  • この研究は,初期のタイプの星に関する貴重な紫外線スペクトルデータを提供します.
  • 過去のミッションと比較してエネルギー分布の不一致は,観測方法と校正のさらなる調査を正当化します.