Troels Emtekær Linnet

Troels Emtekær Linnet PhD student Copenhagen University SBiNLab

Tests

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<include src="https://raw.github.com/Pymol-Scripts/Pymol-script-repo/master/cyspka.py" />

Test2

<include src="http://www.ietf.org/rfc/rfc1945" />

Test DPL imagecontainer=Screenshots

[[%PAGE%|thumb|185px|A random relax screenshot. See Screenshots.]]

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

Test

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