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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.
 
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<div id="Input01"  style="font-size: 150%;"> ①ATR-IR File </div>
: 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="Input02"  style="font-size: 150%;"> ②The order of data </div>
: 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).  
:[[File:NewFILE01.png|200px]][[File:NewFILE04.png|220px]]
 
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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="Input03"  style="font-size: 150%;"> ③Reflectance or Absorbance? </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 type of your ATR-IR data.
:There are two options.  
:: Reflectance(%): The Reflectance of ATR-IR spectra in the value of percentage. (Default)
:First, it is reflectance.
:: Reflectance:    The Reflectance of ATR-IR spectra.  
:Second, it is absorptance.  
:: Absorbance:    The Absorbance of ATR-IR spectra.
:The default is set to the first option.
: The relationships between each data are
:: <math> Reflectance(%)=Reflectance*100 </math>
:: <math> Absorbance=-\log_{10}(Reflectance) </math>
 
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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="Input04"  style="font-size: 150%;"> ④The Substrate in ATR-IR </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 substrate you used in the ATR-IR experiment. Here, we prepare the three substrates that often used
:The default is set to from 1636 to 1863.
:: Diamond(Refractive Index = 2.38). (Default)
<div id="Input05"  style="font-size: 150%;">05:The columns to use for analysis in the Input file</div>
:: 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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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="Input05"  style="font-size: 150%;"> ⑤Incident angle in ATR-IR </div>
:First, it is the wavenumber, and second, it is the representative absorptance or reflectance corresponding the former.
: Please input the incident angle in your ATR-IR experiment. (Default=45 degree)
:For example, there is the input file like below.(You can download this file from Manual Page in ComplexRI. The file name is File03)
: [[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: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>
<div id="Input06"  style="font-size: 150%;"> ⑥Select the column of your data </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.
: Please input the column number of the data that you want to analyze in your ATR-IR file.
:[[File:NewFILE01.png|200px]][[File:NewFILE04.png|220px]]
:: Wavenumber: The column number of wavenumber in your input file. (Default: 1)
:The default is set to the descending order.
:: 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:6_15.png|300px]]


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<div id="Input07"  style="font-size: 150%;">07:The kinds of the substrate used in the ATR-IR experiment</div>
:You should input the refractive index of the substrate you use in the ATR-IR experiment. Here, we prepare the three substrates often used.
:[[File:manual_input7.png|500px]]
:So, if there is the substrate you use, you only have to select the substrate name. It gives the corresponding refractive index. The values are written in the parenthesis next to the substrate name.


:Otherwise, you should select other and, input the refractive index manually.
<div id="Control parameters of ComplexRI fitting"  style="font-size: 200%;">Control parameters of ComplexRI fitting </div>
:[[File:manual_input7_other.png|500px]]
:You can also use this option, when you want to input the refractive index strictly against the three substrates often used.


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<div id="Input08"  style="font-size: 150%;">08:Angle of incidence of IR light</div>
<div id="Input07"  style="font-size: 150%;"> ⑦Title of your job </div>
:You should input the angle of incidence of IR light.
: 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:ATR-IR.png|500px]]
 
:That is <math>{\theta}_i</math>in the above picture.
:The default is set to 45 degree.
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<div id="Input09"  style="font-size: 150%;">09:Refractive index without dispersion</div>
<div id="Input08"  style="font-size: 150%;"> ⑧Input the fitting range </div>
: You should input the refractive index without dispersion. This value is derived from the cauchys equation showed below.
: 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.
:<math>n = A + \frac{B}{{\lambda}^2} + \frac{C}{{\lambda}^4}</math>
:: Minimum wavenumber: The lower boundary of wavenumber. (Default: 1636)
This value usually converges in the IR region. So, you can get this value by substitution of appropriate<math>\lambda</math> and <math>A, B, C</math>parameter corresponding to the substrate for the above equation.
:: Maximum wavenumber: The upper boundary of wavenumber. (Default: 1863)
:The default is set to 1.360.
 
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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%;">10:How strictly you fit the Reflectance Spectra ?</div>
<div id="Input10"  style="font-size: 150%;"> ⑩The tolerance of fitting </div>
:The value input here is used to judge if the fitting of reflectance spectra should finish. The detail is written in the<u> [[explanation01|explanation01]] </u>of<u> [[En/ComplexRI#Internal processing |Internal processing]]</u>.
: Please input the tolerance of the fitting procedure. (default: 0.02)
:The defalut is set to 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>.
:<span style color="red">notice!! If this value is too small, fitting cannot finish.</span>
:: 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:How to set the parameter of the fitting function </div>
<div id="Input11"  style="font-size: 150%;"> ⑪ Manually set the initial parameters </div>
:Here, you can select whether you decide the parameter of fitting functions. We use a set of Lorentz function for fitting of Reflectance spectra as mentioned in the <u>[[explanation01|explanation01]]</u>of<u>[[En/ComplexRI#Internal processing |Internal processing]]</u>. Fitting function is like below.
: Please select whether to set the initial fitting parameters by yourself.
:<math>n_j=n_j^0+\sum_{l=1}^{lmax} \frac{A}{\nu_l-\nu-i\gamma}</math>
:: No: Automatically done by the algorithm (Default)
:The default is set to “NO” like below.
:: Yes: Manually set the initial parameters by users.  
: [[File: manual_input11_no |500px]]
: In the fitting, we use a set of Lorentz functions to represent the complex refractive index
:In this pattern, the parameters are assigned automatically.
:: <math>n_j=n_j^0+\sum_{l=1}^{l_{max}} \frac{A_l}{\nu_l-\nu-i\gamma_l}</math>
:If you select “YES” like below.
: 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.
: [[File: manual_input11_yes|500px]]
: 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>. 
:The new input field is set, and you can give the number of Lorentz function like below
: 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.
: [[File: manual_input11_yes_num |500px]]
:: Note:
:Above, the number is set to 1. So, the three set of parameter of Lorentz function is need to input. init_A1, init_N1 and init_G1 are the amplitude, peak wavenumber, and bandwidth of each Lorentz function, respectively.
::: 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