<div dir="ltr">Dear Wannier90 Developers and users,<div><br></div><div>First of all, I've noticed the reason behind the creation of a portion of all of UNK files to plot Wannier functions. That was due to the "Low disk space problem" (for a system with lots of K point and bands UNK files are so huge).</div><div>By decreasing the number of bands and K pint sampling it fixed and all of the UNK files produced.</div><div><br></div><div>I wanted to plot Wannier functions to recognize the orbital character of MLWFs due to the dear Arash's suggestion in " <span style="line-height:100%">Wannier Digest, Vol 105, Issue 7" (</span><span style="line-height:100%">In general you will need to do some further analysis to determine the character of the final MLWFs, e.g., by plotting them.</span><span style="line-height:100%">). Since the Low disk space problem does exist until now, I want to know is there exist another way to recognize the orbital nature of MLWFs without plotting them? </span> </div><div><br></div><div>Would You do a favor by providing me with a detailed answer to my question? It would b a great help and I'll appreciate it.</div><div><br></div><div>Sincerely Yours</div><div>Riemann </div> <div><div><br></div><div><br></div><div><br clear="all"><div><div class="gmail_signature"><div dir="ltr"><div><div dir="ltr"><div><div dir="ltr"><font face="georgia, serif">-- <br>PhD. student of Physics<br>Physics Department of Damghan University <br>Tel : +98 938 903 6759<br>P.O.Box:36716-41167<br>Damghan, Iran</font></div></div></div></div></div></div></div>
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