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提供: ComplexRI: Manual
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<div id="Input01"  style="font-size: 150%;">01:The name of output file</div>
 
:This is the name of the output file. You can input freely. The default is set to ‘no-title’.
 
: [[File:2Newtoppage.png|1500px]]
: This is the typical snapshot of the input of ComplexRI.  
: The input of ComplexRI contains two parts. The left part is the information of ATR-IR experimental data. The right part is the control parameters of the complex refractive index fitting procedure. Each part will be explained in the following.
 
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<div id="Input02"  style="font-size: 150%;">02:Input the file</div>
<div id="Information of ATR-IR experiment"  style="font-size: 200%;"> Information of ATR-IR experiment </div>
:You set the result file obtained from the ATR-IR experiment. The format is like below.
 
: [[File:FILE01.png|200px]]
:There are three rules for the format of input file.
:First, the extension of input file must be the .txt.
:Second, the wavenumber and the reflectance or the absorptance are ordered in the columns respectively, and counterparts are in the same line.
:Third, the columns are separated by the space.
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<div id="Input03"  style="font-size: 150%;">03:反射率か吸光度か?</div>
<div id="Input01"  style="font-size: 150%;"> ①ATR-IR File </div>
: 結果のファイルで吸光度と反射率のどちらを読み込ませようとしているかを指定してほしい。
: Please upload the ATR-IR experimental data in this part. The inside should be like the following.
: 選択肢は次の3つである。
: [[File:NewFILE01.png|200px]]
: (1)反射率で単位が(%)である。
: If there are characters at the beginning of the file, they will be ignored. The columns of wavenumber and ATR-IR data should be separated by space or comma.
: (2)反射率で単位が(%)ではない。
: For instance, the csv file exported by ATR-IR can be used.
: (3)吸光度
 
: デフォルトは(1)です。
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<div id="Input04"  style="font-size: 150%;">04:波数範囲</div>
<div id="Input02"  style="font-size: 150%;"> ②The order of data </div>
: 屈折率の分散を解析する波数範囲を指定してほしい。
: Please select the sort order of your data.
<div id="Input05"  style="font-size: 150%;">05:データの列の指定</div>
:: Ascending order: The wavenumbers in the input file are in ascending order (left picture). (Default)
:: Descending order: The wavenumbers in the input file are in descending order (right picture).
:[[File:NewFILE01.png|200px]][[File:NewFILE04.png|220px]]
 
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: Inputファイルのうち解析に用いる列を指定してほしい。
<div id="Input03"  style="font-size: 150%;"> ③Reflectance or Absorbance? </div>
: 波数、反射率(あるいは吸光度)についてそれぞれ指定してほしい。
: Please select the type of your ATR-IR data.
: デフォルトは波数が1行目、反射率(あるいは吸光度)が2行目になっている。
:: Reflectance(%): The Reflectance of ATR-IR spectra in the value of percentage. (Default)
:: Reflectance:    The Reflectance of ATR-IR spectra.
:: Absorbance:    The Absorbance of ATR-IR spectra.
: The relationships between each data are
:: <math> Reflectance(%)=Reflectance*100 </math>
:: <math> Absorbance=-\log_{10}(Reflectance) </math>
 
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<div id="Input06"  style="font-size: 150%;">06:昇順か降順か?</div>
<div id="Input04"  style="font-size: 150%;"> ④The Substrate in ATR-IR </div>
: データの並び方を指定してほしい。これは波数の並び方が昇順か降順かを与えてほしい。
: Please select the substrate you used in the ATR-IR experiment. Here, we prepare the three substrates that often used
: デフォルトは降順になっている。
:: Diamond(Refractive Index = 2.38). (Default)
:: Zinc selenide(Refractive Index = 2.40).
:: Germanium(Refractive Index = 4.0).
: You can also input the refractive index of your substrate by selecting Other in the list.
:[[File:4_other.png|500px]]
 
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<div id="Input07"  style="font-size: 150%;">07:実験で用いた基質の種類</div>
<div id="Input05"  style="font-size: 150%;"> ⑤Incident angle in ATR-IR </div>
: 全反射実験で用いた基質の種類をInputしてほしい。これはn1の屈折率を指定することになっている。
: Please input the incident angle in your ATR-IR experiment. (Default=45 degree)
[[File:全反射実験.png|500px]]
 
: 選択肢は次の4つである。
: (1)diamond。屈折率は2.38と設定される。
: (2)zinc selenide。屈折率は2.40と設定される。
: (3)germanium。屈折率は4.0と設定される。
: (4)上記以外。これは屈折率を自由に設定できる。実際の実験で上記3つの基質以外を使った場合を想定している。しかし上記3つの基質のいずれかを使った場合でも、より厳密に屈折率を指定したい場合はこれを用いることも可能である。。
: デフォルトは(1)になっている。
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<div id="Input08"  style="font-size: 150%;">08:入射角</div>
<div id="Input06"  style="font-size: 150%;"> ⑥Select the column of your data  </div>
: 全反射実験の光の入射角を指定してほしい。
: Please input the column number of the data that you want to analyze in your ATR-IR file.
[[File:全反射実験.png|500px]]
:: Wavenumber: The column number of wavenumber in your input file. (Default: 1)
: 上の図でいうところの<math>{\theta}_i</math>である。
:: ATR-IR data: The column number of ATR-IR data in your input file. (Default: 2)
: デフォルトは45°になっている。
 
: For example, an input file like following can be uploaded and column 1 and column 5 can be selected for analyzing.
: [[File:NewFILE03.png|500px]]
: [[File:6_15.png|300px]]
 
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<div id="Input09"  style="font-size: 150%;">09:吸収がないときの屈折率</div>
 
: 吸収がないときの屈折率をInputしてください。
<div id="Control parameters of ComplexRI fitting"  style="font-size: 200%;">Control parameters of ComplexRI fitting </div>
: これはコーシーの方程式<math>n = A + \frac{B}{{\lambda}^2} + \frac{C}{{\lambda}^4}</math>から計算できる。解析したい物質及び波数範囲に合わせて適切なパラメータ及び波長を与え、求めた値をInputしてほしい。
 
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<div id="Input10"  style="font-size: 150%;">10:残差の指定</div>
<div id="Input07"  style="font-size: 150%;"> ⑦Title of your job </div>
: ここでの解析を終了するための指標になる。<u>[[#内部処理|内部処理]]</u>の<u>[[#説明01|説明01:フィッティング方法]]</u>で述べるように最小二乗法を繰り返し行い、残差がここでのInput値より小さいかどうかで解析の終了、続行を判定している。
: Please input the title of your job (alphabet). The output results of ComplexRI will be saved in the excel format with the name @Title.xlsx
: <span style color="red">注意!!小さすぎると終わらないことがある。</span>
 
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<div id="Input11"  style="font-size: 150%;">11:フィッティング関数のパラメータの設定の有無</div>
<div id="Input08"  style="font-size: 150%;"> ⑧Input the fitting range </div>
: フィッティング関数の初期の本数およびパラメータの初期値を手動で与えるか自動で設定するかを選択できる。
: Please input the frequency range (in wavenumber) inside which you want to perform the fitting. ComplexRI will only fit the data inside the range you input here.
: 自動の場合は<u>[[#内部処理|内部処理]]</u><u>[[#説明01|説明01:フィッティング方法]]</u>で述べたように決定している。
:: Minimum wavenumber: The lower boundary of wavenumber. (Default: 1636)
: 手動で決定する場合は、まず、Lor_numにローレンツ関数の本数をInputしてほしい。最大は5となっている。
:: Maximum wavenumber: The upper boundary of wavenumber. (Default: 1863)
: 次に、Lor_numの値に応じて、INIT_A1, INIT_N1, INIT_G1と出てくる。これはローレンツ関数<math>\frac{A}{\nu_l-\nu-i\gamma}</math>のパラメータ<math>A, \nu_l, \gamma</math>に相当している。
 
: 最後の数字が同じINIT_A, INIT_N, INIT_G3つが一組となって一つのローレンツ関数のパラメータの初期を与えることになる。それぞれ、INIT_Aは<math>A</math>, INIT_Nは<math>\nu_l</math>, INIT_Gは<math>\gamma</math>に対応している。
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<div id="Input09"  style="font-size: 150%;"> ⑨Refractive index of target sample in non-resonance region (<math> n_j^0 </math>) </div>
: Please input the refractive index of the target sample (<math> n_j^0 </math>) in non-resonance region. (Default=1.360)
: A database of common liquids is prepared for reference. The determination of <math> n_j^0 </math> and some comments about it can be found in <u> [[Theory#Fitting procedure| How to Fit the ATR-IR spectra]] </u>.
 
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<div id="Input10"  style="font-size: 150%;"> ⑩The tolerance of fitting </div>
: Please input the tolerance of the fitting procedure. (default: 0.02)
: The fitting will be finished when the calculated residual is less than this value. The details are described in <u> [[Theory#Fitting procedure| How to Fit the ATR-IR spectra]] </u>.
:: Note: Try to gradually decrease this value if the fitting results are not close to the experiments. This often happens when fit to the weak adsorption bands. Be careful that fitting can not finish if this value is too small.
 
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<div id="Input11"  style="font-size: 150%;"> ⑪ Manually set the initial parameters </div>
: Please select whether to set the initial fitting parameters by yourself.
:: No: Automatically done by the algorithm (Default)
:: Yes: Manually set the initial parameters by users.
: In the fitting, we use a set of Lorentz functions to represent the complex refractive index
:: <math>n_j=n_j^0+\sum_{l=1}^{l_{max}} \frac{A_l}{\nu_l-\nu-i\gamma_l}</math>
: where <math> n_j^0 </math> is input in ⑨. The number of Lorentz functions <math> l_{max} </math>, and the corresponding initial parameters <math> A_l, \nu_l, \gamma_l </math> should be determined.
: By selecting <math> No </math>, it means the initial parameters are automatically guessed by the algorithm explained in <u> [[Theory#Auto Fitting| Automatically determine the initial parameters in fitting procedure]] </u>. 
: By selecting <math> Yes </math>, you can manually set <math> l_{max} </math> and <math> A_l, \nu_l, \gamma_l </math> for each Lorentz function by yourself. The units of <math> A_l, \nu_l, \gamma_l </math> are all wavenumber. <math> l_{max} </math> is up to 5.
:: Note:
::: 1. Automatical mode is recommended when using ComplexRI to fit new data. The results also provide useful information for users to further fitting the data by manual mode.
::: 2. In some cases that users want to fit the vibrational regions with multiple weak adsorption bands, the manual mode might be better to represent the very detailed spectra.
: [[File:11yes.png|500px]]

2022年3月4日 (金) 02:05時点における最新版


2Newtoppage.png
This is the typical snapshot of the input of ComplexRI.
The input of ComplexRI contains two parts. The left part is the information of ATR-IR experimental data. The right part is the control parameters of the complex refractive index fitting procedure. Each part will be explained in the following.

Information of ATR-IR experiment

①ATR-IR File
Please upload the ATR-IR experimental data in this part. The inside should be like the following.
NewFILE01.png
If there are characters at the beginning of the file, they will be ignored. The columns of wavenumber and ATR-IR data should be separated by space or comma.
For instance, the csv file exported by ATR-IR can be used.

②The order of data
Please select the sort order of your data.
Ascending order: The wavenumbers in the input file are in ascending order (left picture). (Default)
Descending order: The wavenumbers in the input file are in descending order (right picture).
NewFILE01.pngNewFILE04.png

③Reflectance or Absorbance?
Please select the type of your ATR-IR data.
Reflectance(%): The Reflectance of ATR-IR spectra in the value of percentage. (Default)
Reflectance: The Reflectance of ATR-IR spectra.
Absorbance: The Absorbance of ATR-IR spectra.
The relationships between each data are
構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle Reflectance(%)=Reflectance*100 }
構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle Absorbance=-\log_{10}(Reflectance) }

④The Substrate in ATR-IR
Please select the substrate you used in the ATR-IR experiment. Here, we prepare the three substrates that often used
Diamond(Refractive Index = 2.38). (Default)
Zinc selenide(Refractive Index = 2.40).
Germanium(Refractive Index = 4.0).
You can also input the refractive index of your substrate by selecting Other in the list.
4 other.png

⑤Incident angle in ATR-IR
Please input the incident angle in your ATR-IR experiment. (Default=45 degree)

⑥Select the column of your data
Please input the column number of the data that you want to analyze in your ATR-IR file.
Wavenumber: The column number of wavenumber in your input file. (Default: 1)
ATR-IR data: The column number of ATR-IR data in your input file. (Default: 2)
For example, an input file like following can be uploaded and column 1 and column 5 can be selected for analyzing.
NewFILE03.png
6 15.png

Control parameters of ComplexRI fitting

⑦Title of your job
Please input the title of your job (alphabet). The output results of ComplexRI will be saved in the excel format with the name @Title.xlsx

⑧Input the fitting range
Please input the frequency range (in wavenumber) inside which you want to perform the fitting. ComplexRI will only fit the data inside the range you input here.
Minimum wavenumber: The lower boundary of wavenumber. (Default: 1636)
Maximum wavenumber: The upper boundary of wavenumber. (Default: 1863)

⑨Refractive index of target sample in non-resonance region (構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle n_j^0 } )
Please input the refractive index of the target sample (構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle n_j^0 } ) in non-resonance region. (Default=1.360)
A database of common liquids is prepared for reference. The determination of 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle n_j^0 } and some comments about it can be found in How to Fit the ATR-IR spectra .

⑩The tolerance of fitting
Please input the tolerance of the fitting procedure. (default: 0.02)
The fitting will be finished when the calculated residual is less than this value. The details are described in How to Fit the ATR-IR spectra .
Note: Try to gradually decrease this value if the fitting results are not close to the experiments. This often happens when fit to the weak adsorption bands. Be careful that fitting can not finish if this value is too small.

⑪ Manually set the initial parameters
Please select whether to set the initial fitting parameters by yourself.
No: Automatically done by the algorithm (Default)
Yes: Manually set the initial parameters by users.
In the fitting, we use a set of Lorentz functions to represent the complex refractive index
構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle n_j=n_j^0+\sum_{l=1}^{l_{max}} \frac{A_l}{\nu_l-\nu-i\gamma_l}}
where 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle n_j^0 } is input in ⑨. The number of Lorentz functions 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle l_{max} } , and the corresponding initial parameters 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle A_l, \nu_l, \gamma_l } should be determined.
By selecting 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle No } , it means the initial parameters are automatically guessed by the algorithm explained in Automatically determine the initial parameters in fitting procedure .
By selecting 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle Yes } , you can manually set 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle l_{max} } and 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle A_l, \nu_l, \gamma_l } for each Lorentz function by yourself. The units of 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle A_l, \nu_l, \gamma_l } are all wavenumber. 構文解析に失敗 (MathML、ただし動作しない場合はSVGかPNGで代替(最新ブラウザーや補助ツールに推奨): サーバー「https://wikimedia.org/api/rest_v1/」から無効な応答 ("Math extension cannot connect to Restbase."):): {\displaystyle l_{max} } is up to 5.
Note:
1. Automatical mode is recommended when using ComplexRI to fit new data. The results also provide useful information for users to further fitting the data by manual mode.
2. In some cases that users want to fit the vibrational regions with multiple weak adsorption bands, the manual mode might be better to represent the very detailed spectra.
11yes.png