Trusted, Bureaucrats, Administrators
1,660
edits
Changes
Jump to navigation
Jump to search
Troels Emtekær Linnet
PhD student
Copenhagen University
SBiNLab
== Tests ==
[[File:Example.jpg|80px|link=http://www.wikipedia.org]]
[[File:Example.jpg|80px|link=MediaWiki]]
<div class="imagelink_screenshots_small">[[Filestart.png| ]]</div> <include src="https://raw.github.com/Pymol-Scripts/Pymol-script-repo/master/cyspka.py" /> == Test2 == <include src="http:Wiki_test//www.ietf.org/rfc/rfc1945" /> == Test DPL imagecontainer=Screenshots ==<DPL>imagecontainer=Screenshotsrandomcount=1escapelinks=falseopenreferences=truelistseparators=[[,%PAGE%,|thumb|185px|A random relax screenshot. See [[Screenshots]].png]] ,\nordermethod=none</DPL> == SeriesTab == ls -v -d -1 */*.ft2 > allplanes.list cd analysis_FT/int_corr_ft_method_all_awk/coMDD seriesTab -in peaks.dat seriesTab -in ../../peaks.dat -out allplanes_coMDD_ser.ser -list allplanes_coMDD.list == Test randomimagebycategor ==<randomimagebycategory width="200" categories="Screenshots"/> == Test ==<source lang="python">from math import pifrom lib import nmrfrom lib.physical_constants import return_gyromagnetic_ratio id = 'test'H_frq = 900.0e6B0_tesla = H_frq / return_gyromagnetic_ratio(nucleus='1H') * 2.0 * piprint "B0 in Tesla:", B0_teslaisotope = '15N' yOBS_N15_rad_s = return_gyromagnetic_ratio(nucleus=isotope) * B0_teslayOBS_N15_ppm = nmr.frequency_to_ppm_from_rad(frq=yOBS_N15_rad_s, B0=H_frq, isotope=isotope) print yOBS_N15_ppm # Convert hzoffset_hz = 2100.offset_ppm = nmr.frequency_to_ppm(frq=offset_hz, B0=H_frq, isotope=isotope)print offset_ppm #yOBS_rad_s = return_gyromagnetic_ratio(nucleus=isotope) * B0_tesla#print yOBS_rad_s#yOBS_ppm = nmr.frequency_to_ppm_from_rad(frq=yOBS_rad_s, B0=H_frq, isotope=isotope)#print yOBS_ppm # Center carriage In ppmyCAR_ppm = 118.078<br/source>
