Skip to content
Snippets Groups Projects
Commit 17a12778 authored by Frielinghaus, Henrich's avatar Frielinghaus, Henrich
Browse files

README.md and paper.md changed

parent af9815cf
No related branches found
No related tags found
No related merge requests found
...@@ -39,9 +39,9 @@ particles. However, a small angle spectrum contains the information in reciproca ...@@ -39,9 +39,9 @@ particles. However, a small angle spectrum contains the information in reciproca
space, i.e. the information has been Fourier transformed. This is the reason space, i.e. the information has been Fourier transformed. This is the reason
why experimentalists need to be educated well for the data interpretation. why experimentalists need to be educated well for the data interpretation.
The target group of this program is the small angle scattering community The target group of this program is the small angle scattering community
using neutrons and x-rays. Typical wavelengths for neutrons are 5 to 10\AA\ using neutrons and x-rays. Typical wavelengths for neutrons are 5 to 10$\mathrm{\AA}$
with detector distances ranging from 1 to 40m. For x-rays, the typical wavelength with detector distances ranging from 1 to 40m. For x-rays, the typical wavelength
ranges from 0.7 to 1.54\AA with detector distances from 20cm to 10m. ranges from 0.7 to 1.54$\mathrm{\AA}$ with detector distances from 20cm to 10m.
For applying the program ``MuScatt´´ the absolute calibration including For applying the program ``MuScatt´´ the absolute calibration including
a transmission measurement is mandatory. If the sample is scattering strongly a transmission measurement is mandatory. If the sample is scattering strongly
the transmission is usually low, lets say below 30\%. Then, the corrections due the transmission is usually low, lets say below 30\%. Then, the corrections due
......
...@@ -39,9 +39,9 @@ particles. However, a small angle spectrum contains the information in reciproca ...@@ -39,9 +39,9 @@ particles. However, a small angle spectrum contains the information in reciproca
space, i.e. the information has been Fourier transformed. This is the reason space, i.e. the information has been Fourier transformed. This is the reason
why experimentalists need to be educated well for the data interpretation. why experimentalists need to be educated well for the data interpretation.
The target group of this program is the small angle scattering community The target group of this program is the small angle scattering community
using neutrons and x-rays. Typical wavelengths for neutrons are 5 to 10\AA\ using neutrons and x-rays. Typical wavelengths for neutrons are 5 to 10$\mathrm{\AA}$
with detector distances ranging from 1 to 40m. For x-rays, the typical wavelength with detector distances ranging from 1 to 40m. For x-rays, the typical wavelength
ranges from 0.7 to 1.54\AA with detector distances from 20cm to 10m. ranges from 0.7 to 1.54$\mathrm{\AA}$ with detector distances from 20cm to 10m.
For applying the program ``MuScatt´´ the absolute calibration including For applying the program ``MuScatt´´ the absolute calibration including
a transmission measurement is mandatory. If the sample is scattering strongly a transmission measurement is mandatory. If the sample is scattering strongly
the transmission is usually low, lets say below 30\%. Then, the corrections due the transmission is usually low, lets say below 30\%. Then, the corrections due
......
0% Loading or .
You are about to add 0 people to the discussion. Proceed with caution.
Finish editing this message first!
Please register or to comment