yt-users January 2018

yt-users@python.org

21 participants
23 discussions

by david collins

Hi, Everybody! Does anyone out there have a technique for getting the variance out of a profile object? A profile object is good at getting <X> vs. B, I'd then like to get < (X - <X>)^2 > vs B. Matt and I had spittballed the possibility some time ago, but I was wondering if anyone out there had successfully done it. Thanks, d. -- Sent from my computer.

1 year, 6 months

3-D Mass power spectra

by 梁家豪

Dear yt Can current yt calculate 3-D Mass power spectra? I checked the website but I didn't find any information. I think calculating 3-D Mass power spectra is a very useful for cosmological simulations. So I guess maybe yt supports this function now....? Thanks in advance

2 years, 4 months

Derivatives on a 2D Dataset

by llj16b＠my.fsu.edu

Good morning YT-users, I'm trying to take derivatives on a 2d dataset, below is what I do and the error I get: # - - - - - - A SIMPLE TEST TO TRY GETTING A 2D DERIVATIVE - - - - - - - - - - ... ds_list = [yt.load('%s/DD%04d/data%04d'%(base_directory,n1,n1)) for n1 in frame_list] ds = ds_list[0] g = ds.index.grids[0] ds.periodicity = (True, True, True) ad = ds.all_data() # this is to access the grad operator and the added derived field which are found further below: map(xyz_derived_fields, ds_list) # the following line breaks down print(ad['deriv_vx']) # - - - - - - - - - - - - ANOTHER .PY FILE - - - - - - - - - - ... def grad(data,fieldname,direction): iM2 = slice(None,-2) iP2 = slice(2,None) all = slice(1,-1) all_all=[all]*3 dxi=1./(2*data.dds) out = np.zeros_like(data[fieldname]) Right = [all]*3 Left = [all]*3 print(data.shape) if data.shape[2] == 1: all_all[2]=slice(None) Right[2]=slice(None) Left[2]=slice(None) Right[direction] = iP2 Left[direction] = iM2 out[all_all] = (data[fieldname][Right] - data[fieldname][Left]) * dxi[direction] return out def xyz_derived_fields(target): def deriv_vx(field,data): return grad(data,'velocity_x',0) MyValidators = [yt.ValidateSpatial(1,['velocity_x', 'velocity_y','velocity_z'])] target.add_field('deriv_vx', function=deriv_vx, units='cm/s', validators=MyValidators) # this is the error: - - - - - - - - - - - /home/luzlourdes/yt-conda/lib/python2.7/site-packages/yt/units/yt_array.py:1161: VisibleDeprecationWarning: boolean index did not match indexed array along dimension 2; dimension is 4 but corresponding boolean dimension is 1 ret = super(YTArray, self).__getitem__(item) [ 0. 0. 0. ..., 0. 0. 0.] cm/s # - - - - - - - - - - - - - - - - - - - - - May I use your knowledge and help on knowing what is happening and/or how we could go about solving this? Please let me know if I could provide you with anything further. Thank you, Luz Jimenez Vela Graduate Student at FSU

3 years, 8 months

Projection Plot Image Array

by Julia Rakas

Hello, When I do yt.off_axis_projection(…) I get an array as an output. My question is how I can get an output array for regular projection plots? And does the output array correspond to the actual image that it otherwise would have plotted? Thanks, Julie

3 years, 8 months

Error in streamline plotting

by Sushilkumar

Dear yt: I am getting the following error for the script (see below). Could you let me know what is causing it? Thank you in advance Error: yt.utilities.exceptions.YTUnitOperationError: The addition operator for YTArrays with units (km) and (1) is not well defined. Script: import yt import numpy as np import matplotlib.pylab as pl import matplotlib.pyplot as plt import matplotlib.colors as colors from matplotlib.colors import LogNorm from yt.visualization.api import Streamlines from yt.units import km from mpl_toolkits.mplot3d import Axes3D ms = 24000000 vector_max=ms-(ms/3) ms1=ms-vector_max dims = (200,200,200) x = np.genfromtxt("/work/jbi157/MODEL7/UPDATE_B/yo_n_t0.mtx",skip_header=2,usecols=1, dtype="f8") x = x.reshape((8000000, 3), order="F") field1 = x[:,2].reshape(dims, order="F") field2 = x[:,1].reshape(dims, order="F") field3 = x[:,0].reshape(dims, order="F") data = dict(cutting_plane_velocity_x = field1, cutting_plane_velocity_y = field2, cutting_plane_velocity_z = field3) bbox = np.array([[-100, 99], [-100, 99], [-100, 99]]) pf = yt.load_uniform_grid(data, dims, km, bbox=bbox, nprocs=1) L = [0,1,0] # vector normal to cutting plane north_vector = [0,1,1] slc = yt.OffAxisSlicePlot(pf, L, 'cutting_plane_velocity_x', center=[0,0,0], width=(180,'km'), north_vector=north_vector) vel = slc._frb['cutting_plane_velocity_z'] U = slc._frb['cutting_plane_velocity_x'] V = slc._frb['cutting_plane_velocity_y'] extentx = [slc.xlim[i].in_units('km') for i in (0, 1)] extenty = [slc.ylim[i].in_units('km') for i in (0, 1)] extent = extentx + extenty x = np.linspace(extentx[0], extentx[1], vel.shape[0]) y = np.linspace(extenty[1], extenty[0], vel.shape[1]) X, Y = np.meshgrid(x, y) normalize = True if normalize is True: N = np.sqrt(U**2+V**2) U /= N V /= N norm = colors.Normalize(vmin=vel.min(), vmax=vel.max()) factor = 1 #plt.quiver(X[::factor, ::factor], Y[::factor, ::factor], U[::factor, ::factor], V[::factor, ::factor]) plt.streamplot(X,Y,U,V,norm='True') #plt.imshow(vel.d, extent=extent) plt.colorbar() plt.xlabel("x") plt.axis([-100, 99, -100, 99]) plt.savefig('L(1,0,0) N(0,1,1)') #slc.save() On Mon, Jan 29, 2018 at 2:52 PM, <yt-users-request(a)python.org> wrote: > Send yt-users mailing list submissions to > yt-users(a)python.org > > To subscribe or unsubscribe via the World Wide Web, visit > https://mail.python.org/mm3/mailman3/lists/yt-users.python.org/ > or, via email, send a message with subject or body 'help' to > yt-users-request(a)python.org > > You can reach the person managing the list at > yt-users-owner(a)python.org > > When replying, please edit your Subject line so it is more specific > than "Re: Contents of yt-users digest..." > > Today's Topics: > > 1. CLARIFICATION ON FIELD TYPES (Vadlamani Samhitha) > 2. Re: CLARIFICATION ON FIELD TYPES (Nathan Goldbaum) > 3. Re: CLARIFICATION ON FIELD TYPES (Vadlamani Samhitha) > 4. Re: ROTATION CURVE PLOTS IN YT (Vadlamani Samhitha) > > > ---------------------------------------------------------------------- > > Date: Mon, 29 Jan 2018 19:39:25 +0100 > From: Vadlamani Samhitha <vadlamani.samhitha(a)gmail.com> > Subject: [yt-users] CLARIFICATION ON FIELD TYPES > To: Discussion of the yt analysis package <yt-users(a)python.org> > Message-ID: > <CALTqcmXHvS=uX5TYYGQUiGV63uK+eLSzwB0ywo8Hwb4HJDdu7g@mail. > gmail.com> > Content-Type: multipart/alternative; > boundary="001a113a8b64cce13c0563ee9005" > > --001a113a8b64cce13c0563ee9005 > Content-Type: text/plain; charset="UTF-8" > > Hi yt-users, > > I am a newbie in using YT. I read through the documentation of field types > but I still have some confusion in understanding when to use different > field types, as in: > > (1) 'io' vs 'all' (from what I understand, both are used for particles but > I don't get the minute difference) > (2) 'ramses' vs 'index' vs 'gas' (fluids described on the grid, I suppose?) > > It would be really helpful if someone could provide an elaborate > explanation on these. > > --001a113a8b64cce13c0563ee9005 > Content-Type: text/html; charset="UTF-8" > Content-Transfer-Encoding: quoted-printable > > <div dir=3D"ltr">Hi yt-users,=C2=A0<div><br></div><div>I am a newbie in > usi= > ng YT. I read through the documentation of field types but I still have > som= > e confusion=C2=A0in understanding when to use different field types, as > in:= > =C2=A0</div><div><br></div><div>(1) 'io' vs 'all' (from > wha= > t I understand, both are used for particles but I don't get the minute > = > difference)</div><div>(2) 'ramses' vs 'index' vs > 'gas&#= > 39; (fluids described on the grid, I suppose?)</div><div><br></div><div>It > = > would be really helpful if someone could provide an elaborate explanation > o= > n these.=C2=A0 =C2=A0=C2=A0</div></div> > > --001a113a8b64cce13c0563ee9005-- > > ------------------------------ > > Date: Mon, 29 Jan 2018 12:47:09 -0600 > From: Nathan Goldbaum <nathan12343(a)gmail.com> > Subject: [yt-users] Re: CLARIFICATION ON FIELD TYPES > To: Discussion of the yt analysis package <yt-users(a)python.org> > Message-ID: > <CAJXewOkzdX9y7D+-ziBSjZMEFmz86mOep5RsTHiqM_ > 69SK_iHQ(a)mail.gmail.com> > Content-Type: multipart/alternative; > boundary="94eb2c197fcaa201900563eead13" > > --94eb2c197fcaa201900563eead13 > Content-Type: text/plain; charset="UTF-8" > > On Mon, Jan 29, 2018 at 12:39 PM, Vadlamani Samhitha < > vadlamani.samhitha(a)gmail.com> wrote: > > > Hi yt-users, > > > > I am a newbie in using YT. I read through the documentation of field > types > > but I still have some confusion in understanding when to use different > > field types, as in: > > > > (1) 'io' vs 'all' (from what I understand, both are used for particles > but > > I don't get the minute difference) > > > > This distinction only matters if there are multiple types of particles in a > single simulation. For example, Gadget data has 5 different particle types > on disk, 'halo', 'disk', 'stars', 'bulge', and 'gas'. If I load a Gadget > dataset with yt I can access the particles in each of these particle types > separately by prefixing the particle field I want to access with the > particle type I want to access. > > "all" is a particle union (see > http://yt-project.org/docs/dev/analyzing/filtering.html#particle-unions) > that corresponds to the union between all on-disk particle types. If you > access an "all" field, you will get back the field values for the union of > all of the particles in the simulation. Only fields that are defined for > all particle types are defined for the "all" particle union. > > Since ramses only has one particle type, we call that type "io". For RAMSES > (and Enzo and several other formats where all the particles are mixed > together on disk) "io" and "all" are interchangeable. > > > > (2) 'ramses' vs 'index' vs 'gas' (fluids described on the grid, I > suppose?) > > > > The "ramses" field type corresponds to the on-disk fields in the ramses > outputs. Each of these fields has a corresponding "gas" field that it is > aliased to. For example, ('gas', 'density') is an alias to ("ramses", > "Density"). > > When you access a "gas" field, by default it will be returned in CGS units. > When you access a "ramses" field, by default it will be returned in code > units. > > The 'index' fields are fields that depend on the AMR structure or the > geometry of the data but not the on-disk fields. For example, ('index', > 'x'), ('index', 'grid_level'), etc. > > Hope that helps, > > Nathan > > > > > > It would be really helpful if someone could provide an elaborate > > explanation on these. > > > > _______________________________________________ > > yt-users mailing list -- yt-users(a)python.org > > To unsubscribe send an email to yt-users-leave(a)python.org > > > > > > --94eb2c197fcaa201900563eead13 > Content-Type: text/html; charset="UTF-8" > Content-Transfer-Encoding: quoted-printable > > <div dir=3D"ltr"><br><div class=3D"gmail_extra"><br><div > class=3D"gmail_quo= > te">On Mon, Jan 29, 2018 at 12:39 PM, Vadlamani Samhitha <span > dir=3D"ltr">= > <<a href=3D"mailto:vadlamani.samhitha@gmail.com" > target=3D"_blank">vadla= > mani.samhitha(a)gmail.com</a>></span> wrote:<br><blockquote > class=3D"gmail= > _quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid > rgb(204,204= > ,204);padding-left:1ex"><div dir=3D"ltr">Hi yt-users,=C2=A0<div><br></div> > <= > div>I am a newbie in using YT. I read through the documentation of field > ty= > pes but I still have some confusion=C2=A0in understanding when to use > diffe= > rent field types, as in:=C2=A0</div><div><br></div><div>(1) 'io' > vs= > 'all' (from what I understand, both are used for particles but I > d= > on't get the minute difference)</div></div></ > blockquote><div><br></div>= > <div>This distinction only matters if there are multiple types of > particles= > in a single simulation. For example, Gadget data has 5 different particle > = > types on disk, 'halo', 'disk', 'stars', > 'bulge&= > #39;, and 'gas'. If I load a Gadget dataset with yt I can access > th= > e particles in each of these particle types separately by prefixing the > par= > ticle field I want to access with the particle type I want to > access.<br></= > div><div><br></div><div>"all" is a particle union (see <a > href=3D= > "http://yt-project.org/docs/dev/analyzing/filtering.html#particle-unions > ">h= > ttp://yt-project.org/docs/dev/analyzing/filtering.html#particle-unions > </a>)= > that corresponds to the union between all on-disk particle types. If you > a= > ccess an "all" field, you will get back the field values for the > = > union of all of the particles in the simulation. Only fields that are > defin= > ed for all particle types are defined for the "all" particle > unio= > n.<br></div><div><br></div><div>Since ramses only has one particle type, > we= > call that type "io". For RAMSES (and Enzo and several other > form= > ats where all the particles are mixed together on disk) "io" and > = > "all" are interchangeable.<br></div><div>=C2=A0</div><blockquote > = > class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px > sol= > id rgb(204,204,204);padding-left:1ex"><div dir=3D"ltr"><div>(2) > 'ramses= > ' vs 'index' vs 'gas' (fluids described on the grid, I > = > suppose?)</div></div></blockquote><div><br></div><div>The > "ramses&quot= > ; field type corresponds to the on-disk fields in the ramses outputs. Each > = > of these fields has a corresponding "gas" field that it is > aliase= > d to. For example, ('gas', 'density') is an alias to > (&quot= > ;ramses", "Density").</div><div><br></div><div>When you > acce= > ss a "gas" field, by default it will be returned in CGS units. > Wh= > en you access a "ramses" field, by default it will be returned > in= > code units.</div><div><br></div><div>The 'index' fields are > fields= > that depend on the AMR structure or the geometry of the data but not the > o= > n-disk fields. For example, ('index', 'x'), > ('index&#39= > ;, 'grid_level'), etc.</div><div><br></div><div>Hope that > helps,<br= > ></div><div><br></div><div>Nathan<br></div><div>=C2=A0</div><blockquote > cla= > ss=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid > = > rgb(204,204,204);padding-left:1ex"><div dir=3D"ltr"><div><br></div><div>It > = > would be really helpful if someone could provide an elaborate explanation > o= > n these.=C2=A0 =C2=A0=C2=A0</div></div> > <br>______________________________<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org > ">yt-users@py= > thon.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > ">yt-users-leave(a)python.org</a><br> > <br></blockquote></div><br></div></div> > > --94eb2c197fcaa201900563eead13-- > > ------------------------------ > > Date: Mon, 29 Jan 2018 21:34:03 +0100 > From: Vadlamani Samhitha <vadlamani.samhitha(a)gmail.com> > Subject: [yt-users] Re: CLARIFICATION ON FIELD TYPES > To: Discussion of the yt analysis package <yt-users(a)python.org> > Message-ID: > <CALTqcmWRmaisifABkYFmr_1Vg8aZ6w4uz9bSUPzd9xPh17e1gw@ > mail.gmail.com> > Content-Type: multipart/alternative; > boundary="94eb2c1c1716c1c66a0563f02a60" > > --94eb2c1c1716c1c66a0563f02a60 > Content-Type: text/plain; charset="UTF-8" > > Yes! Thank you > > On Mon, Jan 29, 2018 at 7:47 PM, Nathan Goldbaum <nathan12343(a)gmail.com> > wrote: > > > > > > > On Mon, Jan 29, 2018 at 12:39 PM, Vadlamani Samhitha < > > vadlamani.samhitha(a)gmail.com> wrote: > > > >> Hi yt-users, > >> > >> I am a newbie in using YT. I read through the documentation of field > >> types but I still have some confusion in understanding when to use > >> different field types, as in: > >> > >> (1) 'io' vs 'all' (from what I understand, both are used for particles > >> but I don't get the minute difference) > >> > > > > This distinction only matters if there are multiple types of particles in > > a single simulation. For example, Gadget data has 5 different particle > > types on disk, 'halo', 'disk', 'stars', 'bulge', and 'gas'. If I load a > > Gadget dataset with yt I can access the particles in each of these > particle > > types separately by prefixing the particle field I want to access with > the > > particle type I want to access. > > > > "all" is a particle union (see http://yt-project.org/docs/ > > dev/analyzing/filtering.html#particle-unions) that corresponds to the > > union between all on-disk particle types. If you access an "all" field, > you > > will get back the field values for the union of all of the particles in > the > > simulation. Only fields that are defined for all particle types are > defined > > for the "all" particle union. > > > > Since ramses only has one particle type, we call that type "io". For > > RAMSES (and Enzo and several other formats where all the particles are > > mixed together on disk) "io" and "all" are interchangeable. > > > > > >> (2) 'ramses' vs 'index' vs 'gas' (fluids described on the grid, I > >> suppose?) > >> > > > > The "ramses" field type corresponds to the on-disk fields in the ramses > > outputs. Each of these fields has a corresponding "gas" field that it is > > aliased to. For example, ('gas', 'density') is an alias to ("ramses", > > "Density"). > > > > When you access a "gas" field, by default it will be returned in CGS > > units. When you access a "ramses" field, by default it will be returned > in > > code units. > > > > The 'index' fields are fields that depend on the AMR structure or the > > geometry of the data but not the on-disk fields. For example, ('index', > > 'x'), ('index', 'grid_level'), etc. > > > > Hope that helps, > > > > Nathan > > > > > >> > >> It would be really helpful if someone could provide an elaborate > >> explanation on these. > >> > >> _______________________________________________ > >> yt-users mailing list -- yt-users(a)python.org > >> To unsubscribe send an email to yt-users-leave(a)python.org > >> > >> > > > > _______________________________________________ > > yt-users mailing list -- yt-users(a)python.org > > To unsubscribe send an email to yt-users-leave(a)python.org > > > > > > --94eb2c1c1716c1c66a0563f02a60 > Content-Type: text/html; charset="UTF-8" > Content-Transfer-Encoding: quoted-printable > > <div dir=3D"ltr">Yes! Thank you</div><div class=3D"gmail_extra"><br><div > cl= > ass=3D"gmail_quote">On Mon, Jan 29, 2018 at 7:47 PM, Nathan Goldbaum <span > = > dir=3D"ltr"><<a href=3D"mailto:nathan12343@gmail.com" > target=3D"_blank">= > nathan12343(a)gmail.com</a>></span> wrote:<br><blockquote > class=3D"gmail_q= > uote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc > solid;padding-left:1e= > x"><div dir=3D"ltr"><br><div class=3D"gmail_extra"><br><div > class=3D"gmail_= > quote"><span class=3D"">On Mon, Jan 29, 2018 at 12:39 PM, Vadlamani > Samhith= > a <span dir=3D"ltr"><<a href=3D"mailto:vadlamani.samhitha@gmail.com" > tar= > get=3D"_blank">vadlamani.samhitha(a)gmail.com</a>></span> > wrote:<br><block= > quote class=3D"gmail_quote" style=3D"margin:0px 0px 0px > 0.8ex;border-left:1= > px solid rgb(204,204,204);padding-left:1ex"><div dir=3D"ltr">Hi yt-users,= > =C2=A0<div><br></div><div>I am a newbie in using YT. I read through the > doc= > umentation of field types but I still have some confusion=C2=A0in > understan= > ding when to use different field types, as in:=C2=A0</div><div><br></div> > <d= > iv>(1) 'io' vs 'all' (from what I understand, both are > used= > for particles but I don't get the minute > difference)</div></div></bloc= > kquote><div><br></div></span><div>This distinction only matters if there > ar= > e multiple types of particles in a single simulation. For example, Gadget > d= > ata has 5 different particle types on disk, 'halo', > 'disk',= > 'stars', 'bulge', and 'gas'. If I load a Gadget > da= > taset with yt I can access the particles in each of these particle types > se= > parately by prefixing the particle field I want to access with the > particle= > type I want to access.<br></div><div><br></div><div>"all" is a > p= > article union (see <a href=3D"http://yt-project.org/ > docs/dev/analyzing/filt= > ering.html#particle-unions" target=3D"_blank">http://yt-project.org/docs/ > <w= > br>dev/analyzing/filtering.html#<wbr>particle-unions</a>) that > corresponds = > to the union between all on-disk particle types. If you access an > "all= > " field, you will get back the field values for the union of all of > th= > e particles in the simulation. Only fields that are defined for all > particl= > e types are defined for the "all" particle > union.<br></div><div><= > br></div><div>Since ramses only has one particle type, we call that type > &q= > uot;io". For RAMSES (and Enzo and several other formats where all the > = > particles are mixed together on disk) "io" and "all" > ar= > e interchangeable.<br></div><span class=3D""><div>=C2=A0</div><blockquote > c= > lass=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px > soli= > d rgb(204,204,204);padding-left:1ex"><div dir=3D"ltr"><div>(2) > 'ramses&= > #39; vs 'index' vs 'gas' (fluids described on the grid, I > s= > uppose?)</div></div></blockquote><div><br></div></span><div>The > "ramse= > s" field type corresponds to the on-disk fields in the ramses > outputs.= > Each of these fields has a corresponding "gas" field that it is > = > aliased to. For example, ('gas', 'density') is an alias to > = > ("ramses", "Density").</div><div><br></div><div>When > yo= > u access a "gas" field, by default it will be returned in CGS > uni= > ts. When you access a "ramses" field, by default it will be > retur= > ned in code units.</div><div><br></div><div>The 'index' fields > are = > fields that depend on the AMR structure or the geometry of the data but > not= > the on-disk fields. For example, ('index', 'x'), > ('ind= > ex', 'grid_level'), etc.</div><div><br></div><div>Hope that > hel= > ps,<br></div><div><br></div><div>Nathan<br></div><div>=C2= > A0</div><blockquo= > te class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px > = > solid rgb(204,204,204);padding-left:1ex"><span class=3D""><div > dir=3D"ltr">= > <div><br></div><div>It would be really helpful if someone could provide an > = > elaborate explanation on these.=C2=A0 =C2=A0=C2=A0</div></div> > <br></span>______________________________<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org" > target=3D"_= > blank">yt-users(a)python.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > " target=3D"_blank">yt-users-leave(a)python.org</a><br> > <br></blockquote></div><br></div></div> > <br>______________________________<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org > ">yt-users@py= > thon.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > ">yt-users-leave(a)python.org</a><br> > <br></blockquote></div><br></div> > > --94eb2c1c1716c1c66a0563f02a60-- > > ------------------------------ > > Date: Mon, 29 Jan 2018 21:52:49 +0100 > From: Vadlamani Samhitha <vadlamani.samhitha(a)gmail.com> > Subject: [yt-users] Re: ROTATION CURVE PLOTS IN YT > To: Discussion of the yt analysis package <yt-users(a)python.org> > Message-ID: > <CALTqcmWGPRTDD3kWaynOOJQ64pMQPAiAN17Q2k326dL_jMvQdg@mail. > gmail.com> > Content-Type: multipart/related; > boundary="089e082788c4e88ead0563f06d0c" > > --089e082788c4e88ead0563f06d0c > Content-Type: multipart/alternative; boundary=" > 089e082788c4e88ea90563f06d0b" > > --089e082788c4e88ea90563f06d0b > Content-Type: text/plain; charset="UTF-8" > Content-Transfer-Encoding: quoted-printable > > Hi again, > > Thanks for all the responses. As Corentin suggested, I tried a ProfilePlot > for just the particles using phi component of the velocity, but I still > don't get a rotational curve atleast close to what is expected. Also, the > velocity seems unreasonably high (10^4 km/s). Any other possible ideas? > " > *filename=3D"SIM001/output_00030/info_00030.txt"* > *ds=3Dyt.load(filename)* > *sp =3D ds.sphere('c', 100*kpc)* > *plot =3D yt.ProfilePlot(sp, "particle_radius", > ["particle_spherical_velocity_phi"], weight_field=3DNone)* > *plot.set_unit("particle_spherical_velocity_phi", "km/s")* > *plot.set_unit("particle_radius", "kpc")* > *plot.save()* > " > [image: Inline image 1] > > On Sun, Jan 28, 2018 at 4:59 PM, Eric Gentry <egentry(a)ucsc.edu> wrote: > > > Remember that v_c generally depends on mass at larger radii too; it's > onl= > y > > a few special cases where you only need to know the mass enclosed in a > > sphere (e.g. spherical mass distribution, or a Mestel disk). This is > > discussed in Binney & Tremaine's book in section 2.6.1. > > > > Unfortunately I don't know a good, general way for calculating v_c off > th= > e > > top of my head. > > > > > > -- > > Eric Gentry > > PhD Candidate > > ISB 159 | ericsgentry.com > > Astronomy and Astrophysics > > University of California, Santa Cruz > > > > > > On Sun, Jan 28, 2018 at 3:58 AM, Vadlamani Samhitha < > > vadlamani.samhitha(a)gmail.com> wrote: > > > >> Hey again, > >> I thought of a simpler way to get the rotational curves, basically using > >> the mass enclosed in a sphere > >> <http://yt-project.org/doc/cookbook/calculating_information.html> to > >> calculate the circular velocity. To be more precise, I do the following: > >> > >> *filename=3D"output_00010/info_00010.txt" * > >> *ds=3Dyt.simulation(filename)* > >> *G=3Dyt.YTArray(4*np.pi**2,'au**3/yr**2/Msun')* > >> *temp=3Dnp.arange(0.5, 40, 0.1)* > >> *x=3Dyt.YTArray(temp,'kpc')* > >> *V_c =3D np.array([])* > >> *for i in x: * > >> * sp =3D ds.sphere("c", (i, "kpc"))* > >> * print(i)* > >> *# This recipe constructs a sphere and then sums the total mass in > >> particles and fluids in the sphere* > >> > >> * baryon_mass, particle_mass =3D sp.quantities.total_quantity([ > "cell_mas= > s", > >> "particle_mass"])* > >> * M_total=3D(baryon_mass+particle_mass).in_units('Msun')* > >> * circular=3Dnp.sqrt(G*M_total/i).in_units('km/s')* > >> * V_c=3Dnp.append(V_c, circular)* > >> *plt.plot(temp,V_c)* > >> *plt.show()* > >> > >> but ended up with a curve attached in the link below. But we expect a > >> flat rotation curve and not keplerian decrease. Is this a valid > approach= > to > >> get the rotation curves in YT? > >> > >> Thanks! > >> > >> On Fri, Jan 26, 2018 at 2:22 PM, Vadlamani Samhitha < > >> vadlamani.samhitha(a)gmail.com> wrote: > >> > >>> Hey thanks, then, are these derived fields computed automatically and > >>> available to access when the data is loaded or does the user have to > >>> manually compute as in > >>> here <http://yt-project.org/doc/developing/creating_derived_ > fields.html= > > > >>> ? > >>> > >>> On Thu, Jan 25, 2018 at 6:06 PM, Contact <contact(a)cphyc.me> wrote: > >>> > >>>> From what I see from your mail, it looks like you're only listing the > >>>> field_list. You can get a much more comprehensive list using > >>>> 'ds.derived_field_list' which include e.g. the angular velocity. These > >>>> fields aren't directly read from your output but are computed (or > deri= > ved) > >>>> quantities, such as the entropy, the dynamical time, =E2=80=A6 and > you= > an use them > >>>> for 1D profiles too. > >>>> > >>>> Corentin Cadiou > >>>> > >>>> On 25 janv. 2018, at 16:16, Vadlamani Samhitha < > >>>> vadlamani.samhitha(a)gmail.com> wrote: > >>>> > >>>> Sorry, I didn't get what you meant. > >>>> > >>>> On Thu, Jan 25, 2018 at 4:04 PM, Nathan Goldbaum < > nathan12343(a)gmail.co= > m > >>>> > wrote: > >>>> > >>>>> You=E2=80=99re looking for the =E2=80=9Cparticle_radius=E2=80=9D > fiel= > d. > >>>>> > >>>>> On Thu, Jan 25, 2018 at 9:01 AM Vadlamani Samhitha < > >>>>> vadlamani.samhitha(a)gmail.com> wrote: > >>>>> > >>>>>> I see, How about obtaining the rotational curves for gas and matter > >>>>>> separately and then adding them up? Would that be simpler (even if > i= > ts an > >>>>>> approximate) instead of considering the potential directly? I > modell= > ed > >>>>>> stars and dark matter under particles and gas as fluid on the mesh > a= > nd I > >>>>>> have the following my fields_list: ( I am dealing with cartesian > >>>>>> coordinates. So, I don't have the spherical coordinates in my > fields= > _list) > >>>>>> > >>>>>> *" ('all', 'particle_extra_field_1')* > >>>>>> *('all', 'particle_extra_field_2')* > >>>>>> *('all', 'particle_extra_field_3')* > >>>>>> *('all', 'particle_extra_field_4')* > >>>>>> *('all', 'particle_extra_field_5')* > >>>>>> *('all', 'particle_identifier')* > >>>>>> *('all', 'particle_mass')* > >>>>>> *('all', 'particle_position_x')* > >>>>>> *('all', 'particle_position_y')* > >>>>>> *('all', 'particle_position_z')* > >>>>>> *('all', 'particle_refinement_level')* > >>>>>> *('all', 'particle_velocity_x')* > >>>>>> *('all', 'particle_velocity_y')* > >>>>>> *('all', 'particle_velocity_z')* > >>>>>> *('io', 'particle_extra_field_1')* > >>>>>> *('io', 'particle_extra_field_2')* > >>>>>> *('io', 'particle_extra_field_3')* > >>>>>> *('io', 'particle_extra_field_4')* > >>>>>> *('io', 'particle_extra_field_5')* > >>>>>> *('io', 'particle_identifier')* > >>>>>> *('io', 'particle_mass')* > >>>>>> *('io', 'particle_position_x')* > >>>>>> *('io', 'particle_position_y')* > >>>>>> *('io', 'particle_position_z')* > >>>>>> *('io', 'particle_refinement_level')* > >>>>>> *('io', 'particle_velocity_x')* > >>>>>> *('io', 'particle_velocity_y')* > >>>>>> *('io', 'particle_velocity_z')* > >>>>>> *('ramses', 'Density')* > >>>>>> *('ramses', 'Metallicity')* > >>>>>> *('ramses', 'Pressure')* > >>>>>> *('ramses', 'var6')* > >>>>>> *('ramses', 'x-velocity')* > >>>>>> *('ramses', 'y-velocity')* > >>>>>> *('ramses', 'z-velocity') "* > >>>>>> > >>>>>> So, I am thinking that the highlighted fields in the type 'all' > coul= > d > >>>>>> be used to compute circular velocity [sqrt(particle_velocity_x^2+ > par= > ticle_velocity_y^2)] > >>>>>> and the radius [sqrt(particle_position_x^2+particle_position_y^2)] > >>>>>> for particles. And for gas, 'ramses' fields could be used. However, > = > I am > >>>>>> not sure how to get the radius for the gas in this case. Would this > = > be a > >>>>>> right approach at all to begin with? > >>>>>> _______________________________________________ > >>>>>> yt-users mailing list -- yt-users(a)python.org > >>>>>> To unsubscribe send an email to yt-users-leave(a)python.org > >>>>>> > >>>>> > >>>>> _______________________________________________ > >>>>> yt-users mailing list -- yt-users(a)python.org > >>>>> To unsubscribe send an email to yt-users-leave(a)python.org > >>>>> > >>>>> > >>>> _______________________________________________ > >>>> yt-users mailing list -- yt-users(a)python.org > >>>> To unsubscribe send an email to yt-users-leave(a)python.org > >>>> > >>>> > >>>> _______________________________________________ > >>>> yt-users mailing list -- yt-users(a)python.org > >>>> To unsubscribe send an email to yt-users-leave(a)python.org > >>>> > >>>> > >>> > >> > >> _______________________________________________ > >> yt-users mailing list -- yt-users(a)python.org > >> To unsubscribe send an email to yt-users-leave(a)python.org > >> > >> > > > > _______________________________________________ > > yt-users mailing list -- yt-users(a)python.org > > To unsubscribe send an email to yt-users-leave(a)python.org > > > > > > --089e082788c4e88ea90563f06d0b > Content-Type: text/html; charset="UTF-8" > Content-Transfer-Encoding: quoted-printable > > <div dir=3D"ltr">Hi again,=C2=A0<div><br></div><div>Thanks for all the > resp= > onses. As Corentin suggested, I tried a ProfilePlot for just the particles > = > using phi component of the velocity, but I still don't get a > rotational= > curve atleast close to what is expected. Also, the velocity seems > unreason= > ably high (10^4 km/s). Any other possible ideas?=C2=A0</div><div>"< > /di= > v><div><b><i>filename=3D"SIM001/output_00030/info_ > 00030.txt"</i><= > /b></div><div><b><i>ds=3Dyt.load(filename)</i></b></div><div><b><i>sp =3D > d= > s.sphere('c', 100*kpc)</i></b><br></div><div><b><i>plot =3D > yt.Prof= > ilePlot(sp, "particle_radius", ["particle_spherical_ > velocity= > _phi"], weight_field=3DNone)</i></b></div><div><b><i>plot.set_unit(& > qu= > ot;particle_spherical_velocity_phi", "km/s")</i></b></ > div><d= > iv><b><i>plot.set_unit("particle_radius", > "kpc")</i></b= > ></div><div><b><i>plot.save()</i></b></div><div>"</div><div><img src= > =3D"cid:ii_16143af40e0751ec" alt=3D"Inline image 1" width=3D"412" > height=3D= > "330"><br></div></div><div class=3D"gmail_extra"><br><div > class=3D"gmail_qu= > ote">On Sun, Jan 28, 2018 at 4:59 PM, Eric Gentry <span dir=3D"ltr"><<a > = > href=3D"mailto:egentry@ucsc.edu" target=3D"_blank">egentry(a)ucsc.edu > </a>>= > </span> wrote:<br><blockquote class=3D"gmail_quote" style=3D"margin:0 0 0 > .= > 8ex;border-left:1px #ccc solid;padding-left:1ex"><div dir=3D"ltr">Remember > = > that v_c generally depends on mass at larger radii too; it's only a > few= > special cases where you only need to know the mass enclosed in a sphere > (e= > .g. spherical mass distribution, or a Mestel disk).=C2=A0 This is > discussed= > in Binney & Tremaine's book in section > 2.6.1.<div><br></div><div>U= > nfortunately I don't know a good, general way for calculating v_c off > t= > he top of my head.</div></div><div class=3D"gmail_extra"><br > clear=3D"all">= > <div><div class=3D"m_-2580383644780269033gmail_signature" > data-smartmail=3D= > "gmail_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div > dir=3D"l= > tr"><div><font color=3D"#888888"><br></font></div><font > color=3D"#888888">-= > -<br>Eric Gentry</font><div><font color=3D"#888888">PhD > Candidate<br></font= > ><div><font color=3D"#888888">ISB 159 | <a href=3D"http://ericsgentry.com" > = > target=3D"_blank">ericsgentry.com</a><br></font><div><font > color=3D"#888888= > ">Astronomy and Astrophysics<br>University of California, Santa > Cruz</font>= > </div></div><div><br></div></div></div></div></div></div></ > div></div></div>= > <div><div class=3D"h5"> > <br><div class=3D"gmail_quote">On Sun, Jan 28, 2018 at 3:58 AM, Vadlamani > S= > amhitha <span dir=3D"ltr"><<a href=3D"mailto:vadlamani. > samhitha(a)gmail.co= > m" target=3D"_blank">vadlamani.samhitha(a)gmail.com</a>></span> > wrote:<br>= > <blockquote class=3D"gmail_quote" style=3D"margin:0 0 0 > .8ex;border-left:1p= > x #ccc solid;padding-left:1ex"><div dir=3D"ltr">Hey again,=C2=A0<div>I > thou= > ght of a simpler way to get the rotational curves, basically using the=C2= > =A0<a href=3D"http://yt-project.org/doc/cookbook/calculating_ > information.ht= > ml" target=3D"_blank">mass enclosed in a sphere</a>=C2=A0to calculate the > c= > ircular velocity. To be more precise, I do the > following:</div><div><br></d= > iv><div><div><b><i>filename=3D"output_00010/info_00< > wbr>010.txt"= > =C2=A0</i></b></div><div><b><i>ds=3Dyt.simulation(filename) > </i></b></div><d= > iv><b><i>G=3Dyt.YTArray(4*np.pi**2,'au**3<wbr>/yr**2/ > Msun')</i></b>= > </div><div><b><i>temp=3Dnp.arange(0.5, 40, 0.1)</i></b></div><div><b><i>x= > =3Dyt.YTArray(temp,'kpc')</i></b></div><div><b><i>V_c =3D > np.array(= > [])</i></b></div><div><b><i>for i in x:=C2=A0</i></b></div><div><b> > <i><span= > style=3D"white-space:pre-wrap"> </span>sp =3D > ds.sphere("c", (i,= > "kpc"))</i></b></div><div><b><i><span > style=3D"white-space:pre-w= > rap"> </span>print(i)</i></b></div><div><b><i># This recipe constructs > a sp= > here and then sums the total mass in particles and fluids in the > sphere</i>= > </b></div><div><b><i><br></i></b></div><div><b><i><span > style=3D"white-spac= > e:pre-wrap"> </span>baryon_mass, particle_mass =3D > sp.quantities.total_quan= > tity([<wbr>"cell_mass", "particle_mass"])</ > i></b></div>= > <div><b><i><span style=3D"white-space:pre-wrap"> > </span>M_total=3D(baryon_m= > ass+particle_<wbr>mass).in_units('Msun')</i></b>< > /div><div><b><i><s= > pan style=3D"white-space:pre-wrap"> </span>circular=3Dnp.sqrt(G*M_ > total/i).= > <wbr>in_units('km/s')</i></b></div><div><b><i><span > style=3D"white-= > space:pre-wrap"> </span>V_c=3Dnp.append(V_c, > circular)</i></b></div><div><b= > ><i>plt.plot(temp,V_c)</i></b></div><div><b><i>plt.show()</ > i></b></div></di= > v><div><br></div><div>but ended up with a curve attached in the link > below.= > But we expect a flat rotation curve and not keplerian=C2=A0decrease. Is > th= > is a valid approach to get the rotation curves in > YT?</div><div><br></div><= > div>Thanks!</div></div><div class=3D"gmail_extra"><br><div > class=3D"gmail_q= > uote">On Fri, Jan 26, 2018 at 2:22 PM, Vadlamani Samhitha <span > dir=3D"ltr"= > ><<a href=3D"mailto:vadlamani.samhitha@gmail.com" > target=3D"_blank">vadl= > amani.samhitha(a)gmail.com</a>></span> wrote:<br><blockquote > class=3D"gmai= > l_quote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc > solid;padding-left= > :1ex"><div dir=3D"ltr">Hey thanks, then, are these derived fields computed > = > automatically and available to access when the data is loaded or does the > u= > ser have to manually compute as in=C2=A0<div><a href=3D" > http://yt-project.o= > rg/doc/developing/creating_derived_fields.html" > target=3D"_blank">here</a>?= > <br></div></div><div class=3D"m_-2580383644780269033m_- > 8722327220951420101H= > OEnZb"><div class=3D"m_-2580383644780269033m_-8722327220951420101h5"><div > c= > lass=3D"gmail_extra"><br><div class=3D"gmail_quote">On Thu, Jan 25, 2018 > at= > 6:06 PM, Contact <span dir=3D"ltr"><<a href=3D"mailto:contact@cphyc.me > "= > target=3D"_blank">contact(a)cphyc.me</a>></span> wrote:<br><blockquote > cl= > ass=3D"gmail_quote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc > solid;p= > adding-left:1ex"><div dir=3D"auto"><div>From what I see from your mail, it > = > looks like you're only listing the field_list. You can get a much more > = > comprehensive list using 'ds.derived_field_list' which include > e.g.= > the angular velocity. These fields aren't directly read from your > outp= > ut but are computed (or derived) quantities, such as the entropy, the > dynam= > ical time, =E2=80=A6 and you an use them for 1D profiles > too.</div><div><br= > ></div><div>Corentin Cadiou</div><div><div class=3D"m_- > 2580383644780269033m= > _-8722327220951420101m_6573092944491014774h5"><div><br>On 25 janv. 2018, > at= > 16:16, Vadlamani Samhitha <<a href=3D"mailto:vadlamani. > samhitha(a)gmail.c= > om" target=3D"_blank">vadlamani.samhitha(a)gmail.com</a>> > wrote:<br><br></= > div><blockquote type=3D"cite"><div><div dir=3D"ltr">Sorry, I didn't > get= > what you meant.</div><div class=3D"gmail_extra"><br><div > class=3D"gmail_qu= > ote">On Thu, Jan 25, 2018 at 4:04 PM, Nathan Goldbaum <span > dir=3D"ltr">&lt= > ;<a href=3D"mailto:nathan12343@gmail.com" target=3D"_blank">nathan12343@ > gma= > il.com</a>></span> wrote:<br><blockquote class=3D"gmail_quote" > style=3D"= > margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex"><div><div > di= > r=3D"auto">You=E2=80=99re looking for the =E2=80=9Cparticle_radius=E2= > 80=9D= > field.</div><br><div class=3D"gmail_quote"><div><div > class=3D"m_-258038364= > 4780269033m_-8722327220951420101m_6573092944491014774m_- > 5999361843722410537= > h5"><div>On Thu, Jan 25, 2018 at 9:01 AM Vadlamani Samhitha <<a > href=3D"= > mailto:vadlamani.samhitha@gmail.com" target=3D"_blank">vadlamani. > samhitha@g= > mail.com</a>> wrote:<br></div></div></div><blockquote > class=3D"gmail_quo= > te" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc > solid;padding-left:1ex"= > ><div><div class=3D"m_-2580383644780269033m_-8722327220951420101m_ > 657309294= > 4491014774m_-5999361843722410537h5"><div>I see, How about obtaining the > rot= > ational curves for gas and matter separately and then adding them up? > Would= > that be simpler (even if its an approximate) instead of considering the > po= > tential directly? I modelled stars and dark matter under particles and gas > = > as fluid on the mesh and I have the following my fields_list: ( I am > dealin= > g with cartesian coordinates. So, I don't have the spherical > coordinate= > s in my fields_list)<div><br></div><div><i>" ('all', > 'part= > icle_extra_field_1')</i><div><i>('all', > 'particle_extra_fie= > ld_2')</i></div><div><i>('all', 'particle_extra_field_3&# > 39= > ;)</i></div><div><i>('all', 'particle_extra_field_4&# > 39;)</i></= > div><div><i>('all', 'particle_extra_field_5&# > 39;)</i></div><div= > ><i>('all', 'particle_identifier') > </i></div><div><i>('a= > ll', 'particle_mass')</i></div><div><i><b>('all', > '= > particle_position_x')</b></i></div><div><i><b>('all', > 'part= > icle_position_y')</b></i></div><div><i>('all', > 'particle_po= > sition_z')</i></div><div><i>('all', > 'particle_refinement_le= > vel')</i></div><div><i><b>('all', > 'particle_velocity_x'= > )</b></i></div><div><i><b>('all', 'particle_velocity_y') > </b= > ></i></div><div><i>('all', 'particle_velocity_z') > </i></div>= > <div><i>('io', 'particle_extra_field_1&# > 39;)</i></div><div><i>(= > 'io', 'particle_extra_field_2')</i></div><div><i>(' > io&#= > 39;, 'particle_extra_field_3')</i></div><div><i>('io', > &#39= > ;particle_extra_field_4')</i></div><div><i>('io', > 'particle= > _extra_field_5')</i></div><div><i>('io', > 'particle_identifi= > er')</i></div><div><i>('io', 'particle_mass')</i></ > div>= > <div><i>('io', 'particle_position_x') > </i></div><div><i>(&#3= > 9;io', 'particle_position_y')</i></div><div><i>('io', > &= > #39;particle_position_z')</i></div><div><i>('io', > 'particle= > _refinement_level')</i></div><div><i>('io', > 'particle_veloc= > ity_x')</i></div><div><i>('io', 'particle_velocity_y') > <= > /i></div><div><i>('io', 'particle_velocity_z') > </i></div><di= > v><i>('ramses', 'Density')</i></div>< > div><i>('ramses&#3= > 9;, 'Metallicity')</i></div><div><i>('ramses', > 'Pressur= > e')</i></div><div><i>('ramses', 'var6')</i></div><div> > <= > i><b>('ramses', 'x-velocity')</b></i>< > /div><div><i><b>(&#39= > ;ramses', 'y-velocity')</b></i></div><div><i>('ramses' > ,= > 'z-velocity') "</i></div><div><br></div><div>So, I am > thinkin= > g that the highlighted fields in the type 'all' could be used to > co= > mpute circular velocity [sqrt(particle_velocity_x^2+ > pa<wbr>rticle_velocity_= > y^2)] and the radius [sqrt(particle_position_x^2+ > pa<wbr>rticle_position_y^2= > )] for particles. And for gas, 'ramses' fields could be used. > Howev= > er, I am not sure how to get the radius for the gas in this case. Would > thi= > s be a right approach at all to begin with?</div></div></div></div>< > /div><s= > pan> > ______________________________<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org" > target=3D"_= > blank">yt-users(a)python.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > " target=3D"_blank">yt-users-leave(a)python.org</a><br> > </span></blockquote></div></div> > <br>______________________________<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org" > target=3D"_= > blank">yt-users(a)python.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > " target=3D"_blank">yt-users-leave(a)python.org</a><br> > <br></blockquote></div><br></div> > </div></blockquote><blockquote type=3D"cite"><div><span>_____ > ______________= > ___________<wbr>_________________</span><br><span>yt-users mailing list > -- = > <a href=3D"mailto:yt-users@python.org" target=3D"_blank">yt-users@ > python.or= > g</a></span><br><span>To unsubscribe send an email to <a href=3D"mailto: > yt-= > users-leave(a)python.org" target=3D"_blank">yt-users-leave(a)python.org > </a></sp= > an><br></div></blockquote></div></div></div><br>__________ > _________________= > ___<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org" > target=3D"_= > blank">yt-users(a)python.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > " target=3D"_blank">yt-users-leave(a)python.org</a><br> > <br></blockquote></div><br></div> > </div></div></blockquote></div><br></div> > <br>______________________________<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org" > target=3D"_= > blank">yt-users(a)python.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > " target=3D"_blank">yt-users-leave(a)python.org</a><br> > <br></blockquote></div><br></div></div></div> > <br>______________________________<wbr>_________________<br> > yt-users mailing list -- <a href=3D"mailto:yt-users@python.org > ">yt-users@py= > thon.org</a><br> > To unsubscribe send an email to <a href=3D"mailto:yt-users-leave@ > python.org= > ">yt-users-leave(a)python.org</a><br> > <br></blockquote></div><br></div> > > --089e082788c4e88ea90563f06d0b-- > > --089e082788c4e88ead0563f06d0c > Content-Type: image/png; > name="info_00030_1d-Profile_particle_radius_particle_ > spherical_velocity_phi.png" > Content-Disposition: inline; > filename="info_00030_1d-Profile_particle_radius_ > particle_spherical_velocity_phi.png" > Content-Transfer-Encoding: base64 > Content-ID: <ii_16143af40e0751ec> > X-Attachment-Id: ii_16143af40e0751ec > > iVBORw0KGgoAAAANSUhEUgAAA+gAAAMgCAYAAACwGEg9AAAABHNCSVQI > CAgIfAhkiAAAAAlwSFlz > AAAPYQAAD2EBqD+naQAAADl0RVh0U29mdHdhcmUAbWF0c > 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w4YN06efflrlVnoAgKaDgA4AAELS/v37deedd+q1117z3MbOjg4cOKDrrrtO06ZN49pz > AGjiCOgA > AAAWWrZsmdq3b6/zzjvP6lIAABYjoAMAAAAAYAMMEgcAA > AAAgA0Q0AEAAAAAsAECOgAAAAAANkBA > BwAAAADABgjoAAAAAADYAAEdAAAAAAAbIKADAAAAAGADBHQAAAAAAGyAgA4A > AAAAgA0Q0AEAAAAA > sAECOgAAAAAANkBABwAAAADABgjoAAAAAADYAAEdAAAAAAAbIKADAAAAAGAD > /w+05pgXhp4FIQAA > AABJRU5ErkJggg== > --089e082788c4e88ead0563f06d0c-- > > ------------------------------ > > Subject: Digest Footer > > _______________________________________________ > yt-users mailing list -- yt-users(a)python.org > To unsubscribe send an email to yt-users-leave(a)python.org > > > ------------------------------ > > End of yt-users Digest, Vol 119, Issue 41 > ***************************************** > -- *SK2* *"**Claiming that something can move faster than light is a good conversation-stopper in physics. People edge away from you in cocktail parties; friends never return phone calls. You just don’t mess with Albert Einstein.**"*

3 years, 8 months

ROTATION CURVE PLOTS IN YT

by Vadlamani Samhitha

Hi everyone, I have recently started using YT to analyze my simulation data from RAMSES. I would like to plot rotational curves for my simulated galaxy but am not quite sure how to do it. Is there a specific function in YT to do so? Any help is greatly appreciated.

3 years, 8 months

CLARIFICATION ON FIELD TYPES

by Vadlamani Samhitha

Hi yt-users, I am a newbie in using YT. I read through the documentation of field types but I still have some confusion in understanding when to use different field types, as in: (1) 'io' vs 'all' (from what I understand, both are used for particles but I don't get the minute difference) (2) 'ramses' vs 'index' vs 'gas' (fluids described on the grid, I suppose?) It would be really helpful if someone could provide an elaborate explanation on these.

3 years, 8 months

Key error using gradient fields with Enzo

by Sam Patrick

Hello all, I am rather new to yt and have recently tried using the gradient fields functionality. I'm attempting to write a script which involves basic calculations with the gradient of the velocity field, however I keep coming across the same error when assigning the gradient field to a variable. My current version of yt is 3.3.1 and my version of Python is 2.7.12. The data dumps I'm reading from were produced by an Enzo cosmology simulation (version 2.5). The following code is a simplified version of the script which runs successfully and outputs a slice plot of the velocity gradient: import yt from yt import derived_field yt.enable_parallelism() ds = yt.load("DD0045/output_0045") val, loc = ds.find_max('density') ds.periodicity = (True, True, True) ds.add_gradient_fields(('gas', 'velocity_x')) #grad_x = ds['velocity_x_gradient_x'] plt = yt.SlicePlot(ds, 'z', 'velocity_x_gradient_x', center= loc, width= (6.0, 'pc') plt.save("plot.png") However, when I try to assign this gradient field to a variable by removing the comment and adding the line "grad_x = ds['velocity_x_gradient_x']" and plotting this instead I come across the following error: File "/opt/apps/yt/3.3.1/yt-conda/lib/python2.7/site-packages/yt/data_objects/static_output.py", line 352, in __getitem__ return self.parameters[key] P015 yt : [ERROR ] 2018-01-25 10:49:00,443 KeyError: 'velocity_x_gradient_x' I am unsure what I am doing wrong here. Any help will be very much appreciated. Thanks, Sam Patrick

3 years, 8 months

BLANK TEMPERATURE PROJECTION PLOT

by Vadlamani Samhitha

Hi, I'm trying to obtain a projection plot of temperature for RAMSES data using: *plot = yt.ProjectionPlot(ds, "z", "temperature", weight_field=None)* However, I get a blank plot as attached in the picture below. Could someone help me figure out what could have gone wrong?

3 years, 8 months

Unable to locate the YT 2.6(Legacy (2.x)) installation script

by Reju Sam John

Dear all, The link http://hg.yt-project.org/yt/raw/stable/doc/install_script.sh for installing yt 2.6 on the page http://yt-project.org/docs/2.6/installing.html is not working. Could you please provide the likeinstall_script.sh of the yt 2.6(Legacy (2.x)) -- Reju Sam John

3 years, 9 months

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yt-users January 2018