Trusted, Bureaucrats, Administrators
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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">[[start.png| ]]</div>
<include src="https://raw.github.com/Pymol-Scripts/Pymol-script-repo/master/cyspka.py" />
<include src="http://www.ietf.org/rfc/rfc1945" />
== Test 3 DPL imagecontainer=Screenshots ==
<DPL>
imagecontainer=CoversScreenshots
randomcount=1
escapelinks=false
openreferences=true
listseparators=[[,%PAGE%,|thumb|185px|A Random PyMOL-generated Coverrandom relax screenshot. See [[CoversScreenshots]].]],\n
ordermethod=none
</DPL>
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 pi
from lib import nmr
from lib.physical_constants import return_gyromagnetic_ratio
id = 'test'
H_frq = 900.0e6
B0_tesla = H_frq / return_gyromagnetic_ratio(nucleus='1H') * 2.0 * pi
print "B0 in Tesla:", B0_tesla
isotope = '15N'
yOBS_N15_rad_s = return_gyromagnetic_ratio(nucleus=isotope) * B0_tesla
yOBS_N15_ppm = nmr.frequency_to_ppm_from_rad(frq=yOBS_N15_rad_s, B0=H_frq, isotope=isotope)
print yOBS_N15_ppm
# Convert hz
offset_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 ppm
yCAR_ppm = 118.078
</source>