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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="Information of ATR-IR experiment"  style="font-size: 200%;"> Information of ATR-IR experiment </div>
 
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<div id="Input02"  style="font-size: 150%;">02:Input the file</div>
<div id="Input01"  style="font-size: 150%;"> ①ATR-IR File </div>
:You set the result file obtained from the ATR-IR experiment. The format is like below.
: Please upload the ATR-IR experimental data in this part. The inside should be like the following.
: [[File:NewFILE01.png|200px]]
: [[File:NewFILE01.png|200px]]
:There are three rules for the format of input file.
: 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.  
:First, the extension of input file must be the .txt.
: For instance, the csv file exported by ATR-IR can be used.  
:Second, the wavenumber and the corresponding 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:Which kinds of data is written in the Input file, absorptance or reflectance?</div>
<div id="Input02"  style="font-size: 150%;"> ②The order of data </div>
:In the input file, there should be the wavenumber and the corresponding absorptance or reflectance. Please, input which data is written in your input file.
: Please select the sort order of your data.
:There are two options.  
:: Ascending order: The wavenumbers in the input file are in ascending order (left picture). (Default)
:First, it is reflectance.
:: Descending order: The wavenumbers in the input file are in descending order (right picture).  
:Second, it is absorptance.  
:[[File:NewFILE01.png|200px]][[File:NewFILE04.png|220px]]
:The default is set to the first option.
 
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<div id="Input04"  style="font-size: 150%;">04:The range of the wavenumber to fit the Reflectance Spectra</div>
<div id="Input03"  style="font-size: 150%;"> ③Reflectance or Absorbance? </div>
:In the input file, there may be all range of the wavenumber and corresponding data obtained from the ATR-IR experiment. Here, you input the range of the wavenumber to fit the reflectance spectra. ComplexRI execute the fitting only in the range you input here.
: Please select the type of your ATR-IR data.
:The default is set to from 1636 to 1863.
:: Reflectance(%): The Reflectance of ATR-IR spectra in the value of percentage. (Default)
<div id="Input05"  style="font-size: 150%;">05:The columns to use for analysis in the Input file</div>
:: 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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In the input file, there may be some columns of the wavenumber and corresponding data obtained from the ATR-IR experiment, but the columns necessary for the fitting is only two.
<div id="Input04"  style="font-size: 150%;"> ④The Substrate in ATR-IR </div>
:First, it is the wavenumber, and second, it is the representative absorptance or reflectance corresponding the former.
: Please select the substrate you used in the ATR-IR experiment. Here, we prepare the three substrates that often used
:For example, there is the input file like below.(You can download this file from Manual Page in ComplexRI. The file name is File03)
:: 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="Input05"  style="font-size: 150%;"> ⑤Incident angle in ATR-IR </div>
: Please input the incident angle in your ATR-IR experiment. (Default=45 degree)
 
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<div id="Input06"  style="font-size: 150%;"> ⑥Select the column of your data  </div>
: 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.  
: [[File:NewFILE03.png|500px]]
: [[File:NewFILE03.png|500px]]
: There are five columns. The first is the wavenumber, the others are all reflectance. The fifth is average of the second, the third and the forth. In this situation, when you input like below, you can get the better fitting result.
: [[File:6_15.png|300px]]
: [[File:manual_input5.png|500px]]
:The default is set to the wavenumber to the first column and the reflectance or the absorptance to second column respectively.


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<div id="Input06"  style="font-size: 150%;">06:The order of data in the input file, ascending order or descending order?</div>
 
:You should input how the data is ordered in the input file. There are two patterns, ascending order or descending order. They are like below. The left is ascending, and the right is descending.
<div id="Control parameters of ComplexRI fitting"  style="font-size: 200%;">Control parameters of ComplexRI fitting </div>
:[[File:NewFILE01.png|200px]][[File:NewFILE04.png|210px]]
:The default is set to the descending order.


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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="Input07"  style="font-size: 150%;"> ⑦Title of your job </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 title of your job (alphabet). The output results of ComplexRI will be saved in the excel format with the name @Title.xlsx
[[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="Input08"  style="font-size: 150%;"> ⑧Input the fitting range </div>
: 全反射実験の光の入射角を指定してほしい。
: 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.
[[File:全反射実験.png|500px]]
:: Minimum wavenumber: The lower boundary of wavenumber. (Default: 1636)
: 上の図でいうところの<math>{\theta}_i</math>である。
:: Maximum wavenumber: The upper boundary of wavenumber. (Default: 1863)
: デフォルトは45°になっている。
 
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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="Input09"  style="font-size: 150%;">09:吸収がないときの屈折率</div>
<div id="Input10"  style="font-size: 150%;"> ⑩The tolerance of fitting </div>
: 吸収がないときの屈折率をInputしてください。
: Please input the tolerance of the fitting procedure. (default: 0.02)
: 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。
: 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>.
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:: 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.
<div id="Input10"  style="font-size: 150%;">10:残差の指定</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。
: <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="Input11"  style="font-size: 150%;"> ⑪ Manually set the initial parameters </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 select whether to set the initial fitting parameters by yourself.
: 自動の場合は<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>で述べたように決定している。
:: No: Automatically done by the algorithm (Default)
: 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。
:: Yes: Manually set the initial parameters by users.
: 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。
: In the fitting, we use a set of Lorentz functions to represent the complex refractive index
: 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。
:: <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