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提供: ComplexRI: Manual
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: [[File:toppage.png|1000px]]
 
This is the typical snapshot of the input of ComplexRI. Each part will be explained in the following.  
 
: [[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="Input01"  style="font-size: 150%;"> ①Title </div>
<div id="Information of ATR-IR experiment"  style="font-size: 200%;"> Information of ATR-IR experiment </div>
: 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


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<div id="Input02"  style="font-size: 150%;"> ②File </div>
<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.
: 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 two 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.  
: (1). The format of input file must be txt.
: For instance, the csv file exported by ATR-IR can be used.  
: (2). The columns are separated by the space.


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<div id="Input03"  style="font-size: 150%;"> ③The order of data </div>
<div id="Input02"  style="font-size: 150%;"> ②The order of data </div>
: Please select the sort order of your data.
: Please select the sort order of your data.
:: Ascending order: The frequencies in the input file are in ascending order (left picture). (Default)
:: Ascending order: The wavenumbers in the input file are in ascending order (left picture). (Default)
:: Descending order: The frequencies in the input file are in descending order (right picture).  
:: Descending order: The wavenumbers in the input file are in descending order (right picture).  
:[[File:NewFILE01.png|200px]][[File:NewFILE04.png|220px]]
:[[File:NewFILE01.png|200px]][[File:NewFILE04.png|220px]]


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<div id="Input04"  style="font-size: 150%;"> ④Reflectance or Absorptance? </div>
<div id="Input03"  style="font-size: 150%;"> ③Reflectance or Absorbance? </div>
: Please select the type of your ATR-IR data.
: 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 in the value of percentage. (Default)
:: Reflectance:    The Reflectance of ATR-IR spectra.  
:: Reflectance:    The Reflectance of ATR-IR spectra.  
:: Absorptance:    The Absorptance of ATR-IR spectra.
:: Absorbance:    The Absorbance of ATR-IR spectra.
: The relationships between each data are
: The relationships between each data are
:: <math> Reflectance(%)=Reflectance*100 </math>
:: <math> Reflectance(%)=Reflectance*100 </math>
:: <math> Absorptance=-\log_{10}(Reflectance) </math>
:: <math> Absorbance=-\log_{10}(Reflectance) </math>
 
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<div id="Input04"  style="font-size: 150%;"> ④The Substrate in ATR-IR </div>
: 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.
:[[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="Input05"  style="font-size: 150%;"> ⑤Select the column of your data  </div>
<div id="Input06"  style="font-size: 150%;"> ⑥Select the column of your data  </div>
: Please input the column number of the data you want to analyze in your ATR-IR file.  
: 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)
:: 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)
:: ATR-IR data: The column number of ATR-IR data in your input file. (Default: 2)
38行目: 53行目:
: For example, an input file like following can be uploaded and column 1 and column 5 can be selected for analyzing.  
: 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]]
: [[File:manual_input5.png|500px]]
: [[File:6_15.png|300px]]


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<div id="Input06"  style="font-size: 150%;"> ⑥Input the fitting range </div>
 
: Please input the frequency range (in wavenumber) you want to perform the fitting. ComplexRI will fit the data only inside the range you input here.
<div id="Control parameters of ComplexRI fitting"  style="font-size: 200%;">Control parameters of ComplexRI fitting </div>
:: minimum wavenumber: The lower boundary of wavenumber. (Default: 1636)
:: maximum wavenumber: The upper boundary of wavenumber. (Default: 1863)


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<div id="Input07"  style="font-size: 150%;"> ⑦Select the Substrate </div>
<div id="Input07"  style="font-size: 150%;"> ⑦Title of your job </div>
: Please select the substrate you used in the ATR-IR experiment. Here, we prepare the three substrates often used: Diamond(Refractive Index = 2.38), Zinc selenide(Refractive Index = 2.40) and Germanium(Refractive Index = 4.0).
: 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
: You can also input the refractive index of your substrate by selecting Others in the list.
:[[File:manual_input7_other.png|500px]]


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<div id="Input08"  style="font-size: 150%;"> ⑧Incident angle in ATR-IR </div>
<div id="Input08"  style="font-size: 150%;"> ⑧Input the fitting range </div>
: Please input the incident angle in your ATR-IR experiment. (Default=45 degree)
: 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)


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----  
<div id="Input09"  style="font-size: 150%;"> ⑨Refractive index of target sample in non-resnance region </div>
<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 non-resnance region. (Default=1.360)
: Please input the refractive index of the target sample (<math> n_j^0 </math>) in non-resonance region. (Default=1.360)
: The refractive index of target sample in non-resnance region should be determined before the fitting procedure. In the reference paper, we use the refractive index values in the visible regions to fit Cauchy's equation.
: 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>.  
:: <math>n = A + \frac{B}{{\lambda}^2} + \frac{C}{{\lambda}^4}</math>
: The obtained parameters <math>A, B, C</math> were used to evaluate the refractive index at 5000 <math> cm^-1 </math>.


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<div id="Input10"  style="font-size: 150%;"> ⑩The tolerance of fitting ?</div>
<div id="Input10"  style="font-size: 150%;"> ⑩The tolerance of fitting </div>
: Please input the tolerance of fitting procedure. The fitting will be finished when the calculated residual is less than this value.
: Please input the tolerance of the fitting procedure. (default: 0.02)
: The details are written in the<u> [[explanation01|explanation01]] </u>of<u> [[En/ComplexRI#Internal processing |Internal processing]]</u>.
: 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!! Fitting can not finish if this value is too small. </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 functions for fitting of Reflectance spectra as mentioned in the <u>
: Please select whether to set the initial fitting parameters by yourself.
[[explanation01|explanation01]] </u>of<u> [[En/ComplexRI#Internal processing |Internal processing]] </u>. Fitting function is like below.
:: No: Automatically done by the algorithm (Default)
:<math>n_j=n_j^0+\sum_{l=1}^{lmax} \frac{A}{\nu_l-\nu-i\gamma}</math>
:: Yes: Manually set the initial parameters by users.  
:The default is set to “NO” like below.
: In the fitting, we use a set of Lorentz functions to represent the complex refractive index
: [[File:2Newmanual_input11_no.png|500px]]
:: <math>n_j=n_j^0+\sum_{l=1}^{l_{max}} \frac{A_l}{\nu_l-\nu-i\gamma_l}</math>
:In this pattern, the parameters are assigned automatically.
: 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.
:If you select “YES” like below.
: 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>. 
: [[File:manual_input11_yes.png|500px]]
: 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.
:The new input fields are set, and you should give the number of Lorentz functions like below. The maximum of the number is 7.
:: Note:
: [[File:manual_input11_yes_num.png|500px]]
::: 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.  
:Above, the number is set to 1. So, the one set of three parameters of Lorentz function is need to input. init_A1, init_N1 and init_G1 are the amplitude, peak wavenumber, and bandwidth of Lorentz function, respectively.
::: 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