Changeset 9f51b0e in sasmodels
- Timestamp:
- Mar 21, 2016 5:51:50 AM (9 years ago)
- Branches:
- master, core_shell_microgels, costrafo411, magnetic_model, release_v0.94, release_v0.95, ticket-1257-vesicle-product, ticket_1156, ticket_1265_superball, ticket_822_more_unit_tests
- Children:
- 39cc3be
- Parents:
- c0c3393 (diff), 5cf3c33 (diff)
Note: this is a merge changeset, the changes displayed below correspond to the merge itself.
Use the (diff) links above to see all the changes relative to each parent. - Location:
- sasmodels
- Files:
-
- 2 added
- 3 edited
Legend:
- Unmodified
- Added
- Removed
-
sasmodels/kernel_header.c
r03cac08 r5cf3c33 45 45 } 46 46 #define expm1 cephes_expm1 47 typedef __int32 int32_t 47 48 #else 48 49 #define kernel extern "C" 50 #include <cstdint> 49 51 #endif 50 52 static void SINCOS(double angle, double &svar, double &cvar) { svar=sin(angle); cvar=cos(angle); } 51 53 # else 54 #include <inttypes.h> // C99 guarantees that int32_t types is here 52 55 #include <stdio.h> 53 56 #include <tgmath.h> // C99 type-generic math, so sin(float) => sinf … … 64 67 # define pown(a,b) pow(a,b) 65 68 #else 69 typedef int int32_t; 66 70 # if defined(USE_SINCOS) 67 71 # define SINCOS(angle,svar,cvar) svar=sincos(angle,&cvar) -
sasmodels/kernel_iq.c
r7ff3cf3 r5cf3c33 18 18 19 19 typedef struct { 20 int pd_par[MAX_PD]; // index of the nth polydispersity variable21 int pd_length[MAX_PD]; // length of the nth polydispersity weight vector22 int pd_offset[MAX_PD]; // offset of pd weights in the par & weight vector23 int pd_stride[MAX_PD]; // stride to move to the next index at this level24 int pd_isvol[MAX_PD]; // True if parameter is a volume weighting parameter25 int par_offset[NPARS]; // offset of par values in the par & weight vector26 int par_coord[NPARS]; // polydispersity coordination bitvector27 int fast_coord_index[NPARS]; // index of the fast coordination parameters28 int fast_coord_count; // number of parameters coordinated with pd 129 int theta_var; // id of spherical correction variable30 int fast_theta; // true if spherical correction depends on pd 120 int32_t pd_par[MAX_PD]; // index of the nth polydispersity variable 21 int32_t pd_length[MAX_PD]; // length of the nth polydispersity weight vector 22 int32_t pd_offset[MAX_PD]; // offset of pd weights in the par & weight vector 23 int32_t pd_stride[MAX_PD]; // stride to move to the next index at this level 24 int32_t pd_isvol[MAX_PD]; // True if parameter is a volume weighting parameter 25 int32_t par_offset[NPARS]; // offset of par values in the par & weight vector 26 int32_t par_coord[NPARS]; // polydispersity coordination bitvector 27 int32_t fast_coord_index[NPARS]; // index of the fast coordination parameters 28 int32_t fast_coord_count; // number of parameters coordinated with pd 1 29 int32_t theta_var; // id of spherical correction variable 30 int32_t fast_theta; // true if spherical correction depends on pd 1 31 31 } ProblemDetails; 32 32 … … 39 39 kernel 40 40 void KERNEL_NAME( 41 int nq, // number of q values42 const int pd_start, // where we are in the polydispersity loop43 const int pd_stop, // where we are stopping in the polydispersity loop41 int32_t nq, // number of q values 42 const int32_t pd_start, // where we are in the polydispersity loop 43 const int32_t pd_stop, // where we are stopping in the polydispersity loop 44 44 global const ProblemDetails *problem, 45 45 global const double *weights, -
sasmodels/kernelpy.py
rd5ac45f r31d22de 128 128 129 129 def __call__(self, fixed, pd, cutoff=1e-5): 130 print("fixed",fixed)131 print("pd", pd)130 #print("fixed",fixed) 131 #print("pd", pd) 132 132 args = self.args[:] # grab a copy of the args 133 133 form, form_volume = self.kernel, self.info['form_volume'] … … 187 187 ################################################################ 188 188 189 #TODO: Wojtek's notes190 #TODO: The goal is to restructure polydispersity loop191 #so it allows fitting arbitrary polydispersity parameters192 #and it accepts cases like coupled parameters193 189 weight = np.empty(len(pd), 'd') 194 190 if weight.size > 0: … … 264 260 result = scale * ret / norm + background 265 261 return result 266 267 """268 Python driver for python kernels269 270 Calls the kernel with a vector of $q$ values for a single parameter set.271 Polydispersity is supported by looping over different parameter sets and272 summing the results. The interface to :class:`PyModel` matches those for273 :class:`kernelcl.GpuModel` and :class:`kerneldll.DllModel`.274 """275 import numpy as np276 from numpy import pi, cos277 278 from .generate import F64279 280 class PyModel(object):281 """282 Wrapper for pure python models.283 """284 def __init__(self, model_info):285 self.info = model_info286 287 def __call__(self, q_vectors):288 q_input = PyInput(q_vectors, dtype=F64)289 kernel = self.info['Iqxy'] if q_input.is_2d else self.info['Iq']290 return PyKernel(kernel, self.info, q_input)291 292 def release(self):293 """294 Free resources associated with the model.295 """296 pass297 298 class PyInput(object):299 """300 Make q data available to the gpu.301 302 *q_vectors* is a list of q vectors, which will be *[q]* for 1-D data,303 and *[qx, qy]* for 2-D data. Internally, the vectors will be reallocated304 to get the best performance on OpenCL, which may involve shifting and305 stretching the array to better match the memory architecture. Additional306 points will be evaluated with *q=1e-3*.307 308 *dtype* is the data type for the q vectors. The data type should be309 set to match that of the kernel, which is an attribute of310 :class:`GpuProgram`. Note that not all kernels support double311 precision, so even if the program was created for double precision,312 the *GpuProgram.dtype* may be single precision.313 314 Call :meth:`release` when complete. Even if not called directly, the315 buffer will be released when the data object is freed.316 """317 def __init__(self, q_vectors, dtype):318 self.nq = q_vectors[0].size319 self.dtype = dtype320 self.is_2d = (len(q_vectors) == 2)321 self.q_vectors = [np.ascontiguousarray(q, self.dtype) for q in q_vectors]322 self.q_pointers = [q.ctypes.data for q in self.q_vectors]323 324 def release(self):325 """326 Free resources associated with the model inputs.327 """328 self.q_vectors = []329 330 class PyKernel(object):331 """332 Callable SAS kernel.333 334 *kernel* is the DllKernel object to call.335 336 *model_info* is the module information337 338 *q_input* is the DllInput q vectors at which the kernel should be339 evaluated.340 341 The resulting call method takes the *pars*, a list of values for342 the fixed parameters to the kernel, and *pd_pars*, a list of (value,weight)343 vectors for the polydisperse parameters. *cutoff* determines the344 integration limits: any points with combined weight less than *cutoff*345 will not be calculated.346 347 Call :meth:`release` when done with the kernel instance.348 """349 def __init__(self, kernel, model_info, q_input):350 self.info = model_info351 self.q_input = q_input352 self.res = np.empty(q_input.nq, q_input.dtype)353 dim = '2d' if q_input.is_2d else '1d'354 # Loop over q unless user promises that the kernel is vectorized by355 # taggining it with vectorized=True356 if not getattr(kernel, 'vectorized', False):357 if dim == '2d':358 def vector_kernel(qx, qy, *args):359 """360 Vectorized 2D kernel.361 """362 return np.array([kernel(qxi, qyi, *args)363 for qxi, qyi in zip(qx, qy)])364 else:365 def vector_kernel(q, *args):366 """367 Vectorized 1D kernel.368 """369 return np.array([kernel(qi, *args)370 for qi in q])371 self.kernel = vector_kernel372 else:373 self.kernel = kernel374 fixed_pars = model_info['partype']['fixed-' + dim]375 pd_pars = model_info['partype']['pd-' + dim]376 vol_pars = model_info['partype']['volume']377 378 # First two fixed pars are scale and background379 pars = [p.name for p in model_info['parameters'][2:]]380 offset = len(self.q_input.q_vectors)381 self.args = self.q_input.q_vectors + [None] * len(pars)382 self.fixed_index = np.array([pars.index(p) + offset383 for p in fixed_pars[2:]])384 self.pd_index = np.array([pars.index(p) + offset385 for p in pd_pars])386 self.vol_index = np.array([pars.index(p) + offset387 for p in vol_pars])388 try: self.theta_index = pars.index('theta') + offset389 except ValueError: self.theta_index = -1390 391 # Caller needs fixed_pars and pd_pars392 self.fixed_pars = fixed_pars393 self.pd_pars = pd_pars394 395 def __call__(self, fixed, pd, cutoff=1e-5):396 #print("fixed",fixed)397 #print("pd", pd)398 args = self.args[:] # grab a copy of the args399 form, form_volume = self.kernel, self.info['form_volume']400 # First two fixed401 scale, background = fixed[:2]402 for index, value in zip(self.fixed_index, fixed[2:]):403 args[index] = float(value)404 res = _loops(form, form_volume, cutoff, scale, background, args,405 pd, self.pd_index, self.vol_index, self.theta_index)406 407 return res408 409 def release(self):410 """411 Free resources associated with the kernel.412 """413 self.q_input = None414 415 def _loops(form, form_volume, cutoff, scale, background,416 args, pd, pd_index, vol_index, theta_index):417 """418 *form* is the name of the form function, which should be vectorized over419 q, but otherwise have an interface like the opencl kernels, with the420 q parameters first followed by the individual parameters in the order421 given in model.parameters (see :mod:`sasmodels.generate`).422 423 *form_volume* calculates the volume of the shape. *vol_index* gives424 the list of volume parameters425 426 *cutoff* ignores the corners of the dispersion hypercube427 428 *scale*, *background* multiplies the resulting form and adds an offset429 430 *args* is the prepopulated set of arguments to the form function, starting431 with the q vectors, and including slots for all the parameters. The432 values for the parameters will be substituted with values from the433 dispersion functions.434 435 *pd* is the list of dispersion parameters436 437 *pd_index* are the indices of the dispersion parameters in *args*438 439 *vol_index* are the indices of the volume parameters in *args*440 441 *theta_index* is the index of the theta parameter for the sasview442 spherical correction, or -1 if there is no angular dispersion443 """444 445 ################################################################446 # #447 # !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! #448 # !! !! #449 # !! KEEP THIS CODE CONSISTENT WITH KERNEL_TEMPLATE.C !! #450 # !! !! #451 # !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! #452 # #453 ################################################################454 455 weight = np.empty(len(pd), 'd')456 if weight.size > 0:457 # weight vector, to be populated by polydispersity loops458 459 # identify which pd parameters are volume parameters460 vol_weight_index = np.array([(index in vol_index) for index in pd_index])461 462 # Sort parameters in decreasing order of pd length463 Npd = np.array([len(pdi[0]) for pdi in pd], 'i')464 order = np.argsort(Npd)[::-1]465 stride = np.cumprod(Npd[order])466 pd = [pd[index] for index in order]467 pd_index = pd_index[order]468 vol_weight_index = vol_weight_index[order]469 470 fast_value = pd[0][0]471 fast_weight = pd[0][1]472 else:473 stride = np.array([1])474 vol_weight_index = slice(None, None)475 # keep lint happy476 fast_value = [None]477 fast_weight = [None]478 479 ret = np.zeros_like(args[0])480 norm = np.zeros_like(ret)481 vol = np.zeros_like(ret)482 vol_norm = np.zeros_like(ret)483 for k in range(stride[-1]):484 # update polydispersity parameter values485 fast_index = k % stride[0]486 if fast_index == 0: # bottom loop complete ... check all other loops487 if weight.size > 0:488 for i, index, in enumerate(k % stride):489 args[pd_index[i]] = pd[i][0][index]490 weight[i] = pd[i][1][index]491 else:492 args[pd_index[0]] = fast_value[fast_index]493 weight[0] = fast_weight[fast_index]494 495 # Computes the weight, and if it is not sufficient then ignore this496 # parameter set.497 # Note: could precompute w1*...*wn so we only need to multiply by w0498 w = np.prod(weight)499 if w > cutoff:500 # Note: can precompute spherical correction if theta_index is not501 # the fast index. Correction factor for spherical integration502 #spherical_correction = abs(cos(pi*args[phi_index])) if phi_index>=0 else 1.0503 spherical_correction = (abs(cos(pi * args[theta_index])) * pi / 2504 if theta_index >= 0 else 1.0)505 #spherical_correction = 1.0506 507 # Call the scattering function and adds it to the total.508 I = form(*args)509 if np.isnan(I).any(): continue510 ret += w * I * spherical_correction511 norm += w512 513 # Volume normalization.514 # If there are "volume" polydispersity parameters, then these515 # will be used to call the form_volume function from the user516 # supplied kernel, and accumulate a normalized weight.517 # Note: can precompute volume norm if fast index is not a volume518 if form_volume:519 vol_args = [args[index] for index in vol_index]520 vol_weight = np.prod(weight[vol_weight_index])521 vol += vol_weight * form_volume(*vol_args)522 vol_norm += vol_weight523 524 positive = (vol * vol_norm != 0.0)525 ret[positive] *= vol_norm[positive] / vol[positive]526 result = scale * ret / norm + background527 return result
Note: See TracChangeset
for help on using the changeset viewer.