mirror of
https://github.com/jart/cosmopolitan.git
synced 2025-05-23 22:02:27 +00:00
Make numerous improvements
- Python static hello world now 1.8mb - Python static fully loaded now 10mb - Python HTTPS client now uses MbedTLS - Python REPL now completes import stmts - Increase stack size for Python for now - Begin synthesizing posixpath and ntpath - Restore Python \N{UNICODE NAME} support - Restore Python NFKD symbol normalization - Add optimized code path for Intel SHA-NI - Get more Python unit tests passing faster - Get Python help() pagination working on NT - Python hashlib now supports MbedTLS PBKDF2 - Make memcpy/memmove/memcmp/bcmp/etc. faster - Add Mersenne Twister and Vigna to LIBC_RAND - Provide privileged __printf() for error code - Fix zipos opendir() so that it reports ENOTDIR - Add basic chmod() implementation for Windows NT - Add Cosmo's best functions to Python cosmo module - Pin function trace indent depth to that of caller - Show memory diagram on invalid access in MODE=dbg - Differentiate stack overflow on crash in MODE=dbg - Add stb_truetype and tools for analyzing font files - Upgrade to UNICODE 13 and reduce its binary footprint - COMPILE.COM now logs resource usage of build commands - Start implementing basic poll() support on bare metal - Set getauxval(AT_EXECFN) to GetModuleFileName() on NT - Add descriptions to strerror() in non-TINY build modes - Add COUNTBRANCH() macro to help with micro-optimizations - Make error / backtrace / asan / memory code more unbreakable - Add fast perfect C implementation of μ-Law and a-Law audio codecs - Make strtol() functions consistent with other libc implementations - Improve Linenoise implementation (see also github.com/jart/bestline) - COMPILE.COM now suppresses stdout/stderr of successful build commands
This commit is contained in:
parent
fa7b4f5bd1
commit
39bf41f4eb
806 changed files with 77494 additions and 63859 deletions
357
third_party/python/Python/cosmomodule.c
vendored
357
third_party/python/Python/cosmomodule.c
vendored
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@ -1,105 +1,316 @@
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/*-*- mode:c;indent-tabs-mode:nil;c-basic-offset:2;tab-width:8;coding:utf-8 -*-│
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│vi: set net ft=c ts=2 sts=2 sw=2 fenc=utf-8 :vi│
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/*-*- mode:c;indent-tabs-mode:nil;c-basic-offset:4;tab-width:8;coding:utf-8 -*-│
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│vi: set net ft=c ts=4 sts=4 sw=4 fenc=utf-8 :vi│
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╞══════════════════════════════════════════════════════════════════════════════╡
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│ This is free and unencumbered software released into the public domain. │
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│ Copyright 2021 Justine Alexandra Roberts Tunney │
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│ │
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│ Anyone is free to copy, modify, publish, use, compile, sell, or │
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│ distribute this software, either in source code form or as a compiled │
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│ binary, for any purpose, commercial or non-commercial, and by any │
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│ means. │
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│ Permission to use, copy, modify, and/or distribute this software for │
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│ any purpose with or without fee is hereby granted, provided that the │
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│ above copyright notice and this permission notice appear in all copies. │
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│ │
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│ In jurisdictions that recognize copyright laws, the author or authors │
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│ of this software dedicate any and all copyright interest in the │
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│ software to the public domain. We make this dedication for the benefit │
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│ of the public at large and to the detriment of our heirs and │
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│ successors. We intend this dedication to be an overt act of │
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│ relinquishment in perpetuity of all present and future rights to this │
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│ software under copyright law. │
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│ │
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│ THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, │
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│ EXPRESS OR IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF │
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│ MERCHANTABILITY, FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. │
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│ IN NO EVENT SHALL THE AUTHORS BE LIABLE FOR ANY CLAIM, DAMAGES OR │
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│ OTHER LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, │
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│ ARISING FROM, OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR │
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│ OTHER DEALINGS IN THE SOFTWARE. │
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│ THE SOFTWARE IS PROVIDED "AS IS" AND THE AUTHOR DISCLAIMS ALL │
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│ WARRANTIES WITH REGARD TO THIS SOFTWARE INCLUDING ALL IMPLIED │
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│ WARRANTIES OF MERCHANTABILITY AND FITNESS. IN NO EVENT SHALL THE │
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│ AUTHOR BE LIABLE FOR ANY SPECIAL, DIRECT, INDIRECT, OR CONSEQUENTIAL │
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│ DAMAGES OR ANY DAMAGES WHATSOEVER RESULTING FROM LOSS OF USE, DATA OR │
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│ PROFITS, WHETHER IN AN ACTION OF CONTRACT, NEGLIGENCE OR OTHER │
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│ TORTIOUS ACTION, ARISING OUT OF OR IN CONNECTION WITH THE USE OR │
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│ PERFORMANCE OF THIS SOFTWARE. │
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╚─────────────────────────────────────────────────────────────────────────────*/
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#include "third_party/python/Include/Python-ast.h"
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#define PY_SSIZE_T_CLEAN
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#include "dsp/scale/cdecimate2xuint8x8.h"
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#include "libc/bits/popcnt.h"
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#include "libc/dce.h"
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#include "libc/macros.internal.h"
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#include "libc/math.h"
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#include "libc/mem/mem.h"
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#include "libc/nexgen32e/crc32.h"
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#include "libc/nexgen32e/rdtsc.h"
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#include "libc/nexgen32e/rdtscp.h"
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#include "libc/runtime/runtime.h"
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#include "third_party/python/Include/abstract.h"
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#include "third_party/python/Include/boolobject.h"
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#include "third_party/python/Include/ceval.h"
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#include "third_party/python/Include/code.h"
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#include "third_party/python/Include/cosmo.h"
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#include "third_party/python/Include/dictobject.h"
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#include "third_party/python/Include/errcode.h"
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#include "third_party/python/Include/eval.h"
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#include "third_party/python/Include/fileutils.h"
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#include "third_party/python/Include/frameobject.h"
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#include "third_party/python/Include/import.h"
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#include "third_party/python/Include/listobject.h"
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#include "third_party/python/Include/longobject.h"
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#include "third_party/python/Include/marshal.h"
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#include "third_party/python/Include/methodobject.h"
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#include "third_party/python/Include/modsupport.h"
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#include "third_party/python/Include/objimpl.h"
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#include "third_party/python/Include/osdefs.h"
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#include "third_party/python/Include/pgenheaders.h"
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#include "third_party/python/Include/pydebug.h"
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#include "third_party/python/Include/moduleobject.h"
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#include "third_party/python/Include/pyerrors.h"
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#include "third_party/python/Include/pylifecycle.h"
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#include "third_party/python/Include/pymacro.h"
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#include "third_party/python/Include/pythonrun.h"
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#include "third_party/python/Include/sysmodule.h"
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#include "third_party/python/Include/traceback.h"
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#include "third_party/python/Include/tupleobject.h"
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#include "third_party/python/Include/warnings.h"
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#include "third_party/python/Include/weakrefobject.h"
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#include "third_party/python/Include/yoink.h"
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#include "third_party/python/Python/importdl.h"
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#include "third_party/xed/x86.h"
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/* clang-format off */
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PYTHON_PROVIDE("_cosmo");
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PYTHON_PROVIDE("cosmo");
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static int cosmo_constants(PyObject *m)
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PyDoc_STRVAR(cosmo_doc,
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"Cosmopolitan Libc Module\n\
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\n\
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This module exposes low-level utilities from the Cosmopolitan library.\n\
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\n\
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Static objects:\n\
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\n\
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MODE -- make build mode, e.g. \"\", \"tiny\", \"opt\", \"rel\", etc.\n\
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IMAGE_BASE_VIRTUAL -- base address of actually portable executable image\n\
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kernel -- o/s platform, e.g. \"linux\", \"xnu\", \"metal\", \"nt\", etc.\n\
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kStartTsc -- the rdtsc() value at process creation.");
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PyDoc_STRVAR(syscount_doc,
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"syscount($module)\n\
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--\n\n\
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Returns number of SYSCALL instructions issued to kernel by C library.\n\
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\n\
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Context switching from userspace to kernelspace is expensive! So it is\n\
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useful to be able to know how many times that's happening in your app.\n\
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\n\
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This value currently isn't meaningful on Windows NT, where it currently\n\
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tracks the number of POSIX calls that were attempted, but have not been\n\
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polyfilled yet.");
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static PyObject *
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cosmo_syscount(PyObject *self, PyObject *noargs)
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{
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if(PyModule_AddStringMacro(m, MODE)) return -1;
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return 0;
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return PyLong_FromSize_t(g_syscount);
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}
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PyDoc_STRVAR(rdtsc_doc,
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"rdtsc($module)\n\
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--\n\n\
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Returns CPU timestamp counter.");
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PyDoc_STRVAR(doc_cosmo,
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"additional information and special functions provided by Cosmopolitan Libc.");
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static PyObject *
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cosmo_rdtsc(PyObject *self, PyObject *noargs)
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{
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return PyLong_FromUnsignedLong(rdtsc());
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}
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PyDoc_STRVAR(getcpucore_doc,
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"getcpucore($module)\n\
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--\n\n\
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Returns 0-indexed CPU core on which process is currently scheduled.");
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static PyObject *
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cosmo_getcpucore(PyObject *self, PyObject *noargs)
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{
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return PyLong_FromUnsignedLong(TSC_AUX_CORE(rdpid()));
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}
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PyDoc_STRVAR(getcpunode_doc,
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"getcpunode($module)\n\
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--\n\n\
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Returns 0-indexed NUMA node on which process is currently scheduled.");
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static PyObject *
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cosmo_getcpunode(PyObject *self, PyObject *noargs)
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{
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return PyLong_FromUnsignedLong(TSC_AUX_NODE(rdpid()));
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}
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PyDoc_STRVAR(ftrace_doc,
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"ftrace($module)\n\
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--\n\n\
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Enables logging of C function calls to stderr, e.g.\n\
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\n\
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cosmo.ftrace()\n\
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WeirdFunction()\n\
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os._exit(1)\n\
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\n\
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Please be warned this prints massive amount of text. In order for it\n\
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to work, the concomitant .com.dbg binary needs to be present.");
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static PyObject *
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cosmo_ftrace(PyObject *self, PyObject *noargs)
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{
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ftrace_install();
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return Py_None;
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}
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PyDoc_STRVAR(crc32c_doc,
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"crc32c($module, bytes, init=0)\n\
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--\n\n\
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Computes 32-bit Castagnoli Cyclic Redundancy Check.\n\
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\n\
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Used by ISCSI, TensorFlow, etc.\n\
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Similar to zlib.crc32().");
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static PyObject *
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cosmo_crc32c(PyObject *self, PyObject *args)
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{
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Py_ssize_t n;
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Py_buffer data;
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unsigned crc, init = 0;
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if (!PyArg_ParseTuple(args, "y*|I:crc32c", &data, &init)) return 0;
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crc = crc32c(init, data.buf, data.len);
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PyBuffer_Release(&data);
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return PyLong_FromUnsignedLong(crc);
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}
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PyDoc_STRVAR(decimate_doc,
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"decimate($module, bytes)\n\
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--\n\n\
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Shrinks byte buffer in half using John Costella's magic kernel.\n\
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\n\
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This downscales data 2x using an eight-tap convolution, e.g.\n\
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\n\
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>>> cosmo.decimate(b'\\xff\\xff\\x00\\x00\\xff\\xff\\x00\\x00\\xff\\xff\\x00\\x00')\n\
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b'\\xff\\x00\\xff\\x00\\xff\\x00'\n\
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\n\
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This is very fast if SSSE3 is available (Intel 2004+ / AMD 2011+).");
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static PyObject *
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cosmo_decimate(PyObject *self, PyObject *args)
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{
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Py_ssize_t n;
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PyObject *buf;
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Py_buffer data;
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if (!PyArg_ParseTuple(args, "y*:decimate", &data)) return 0;
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if ((buf = PyBytes_FromStringAndSize(0, (n = ROUNDUP(data.len, 16))))) {
|
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memcpy(PyBytes_AS_STRING(buf), data.buf, data.len);
|
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memset(PyBytes_AS_STRING(buf) + data.len, 0, n - data.len);
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cDecimate2xUint8x8(n, (void *)PyBytes_AS_STRING(buf),
|
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(signed char[8]){-1, -3, 3, 17, 17, 3, -3, -1});
|
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_PyBytes_Resize(&buf, (data.len + 1) >> 1);
|
||||
}
|
||||
PyBuffer_Release(&data);
|
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return buf;
|
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}
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PyDoc_STRVAR(ild_doc,
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"ild($module, bytes)\n\
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--\n\n\
|
||||
Decodes byte-length of first machine instruction in byte sequence.\n\
|
||||
\n\
|
||||
This function makes it possible to tokenize raw x86 binary instructions.\n\
|
||||
Return value is negative on error, where -1 is defined as buffer being\n\
|
||||
too short, and lower numbers represent other errors.");
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static PyObject *
|
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cosmo_ild(PyObject *self, PyObject *args)
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{
|
||||
Py_ssize_t n;
|
||||
const char *p;
|
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enum XedError e;
|
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struct XedDecodedInst xedd;
|
||||
if (!PyArg_ParseTuple(args, "y#:ild", &p, &n)) return 0;
|
||||
xed_decoded_inst_zero_set_mode(&xedd, XED_MACHINE_MODE_LONG_64);
|
||||
e = xed_instruction_length_decode(&xedd, p, n);
|
||||
return PyLong_FromUnsignedLong(e ? -e : xedd.length);
|
||||
}
|
||||
|
||||
PyDoc_STRVAR(popcount_doc,
|
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"popcount($module, bytes)\n\
|
||||
--\n\n\
|
||||
Returns population count of byte sequence, e.g.\n\
|
||||
\n\
|
||||
>>> cosmo.popcount(b'\\xff\\x00\\xff')\n\
|
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16\n\
|
||||
\n\
|
||||
The population count is the number of bits that are set to one.\n\
|
||||
It does the same thing as `Long.bit_count()` but for data buffers.\n\
|
||||
This goes 30gbps on Nehalem (Intel 2008+) so it's quite fast.");
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||||
|
||||
static PyObject *
|
||||
cosmo_popcount(PyObject *self, PyObject *args)
|
||||
{
|
||||
Py_ssize_t n;
|
||||
const char *p;
|
||||
if (!PyArg_ParseTuple(args, "y#:popcount", &p, &n)) return 0;
|
||||
return PyLong_FromSize_t(_countbits(p, n));
|
||||
}
|
||||
|
||||
PyDoc_STRVAR(rgb2xterm256_doc,
|
||||
"rgb2xterm256($module, r, g, b)\n\
|
||||
--\n\n\
|
||||
Quantizes RGB to color to XTERM256 ANSI terminal code.\n\
|
||||
\n\
|
||||
This helps you print colors in the terminal faster. For example:\n\
|
||||
\n\
|
||||
print(\"\\x1b[38;5;%dmhello\\x1b[0m\" % (cosmo.rgb2xterm256(255,0,0)))\n\
|
||||
\n\
|
||||
Will print red text to the terminal.");
|
||||
|
||||
static PyObject *
|
||||
cosmo_rgb2xterm256(PyObject *self, PyObject *args)
|
||||
{
|
||||
unsigned char r, g, b;
|
||||
int res, cerr, gerr, ir, ig, ib, gray, grai, cr, cg, cb, gv;
|
||||
const unsigned char kXtermCube[6] = {0, 0137, 0207, 0257, 0327, 0377};
|
||||
if (!PyArg_ParseTuple(args, "BBB:rgb2xterm256", &r, &g, &b)) return 0;
|
||||
gray = round(r * .299 + g * .587 + b * .114);
|
||||
grai = gray > 238 ? 23 : (gray - 3) / 10;
|
||||
ir = r < 48 ? 0 : r < 115 ? 1 : (r - 35) / 40;
|
||||
ig = g < 48 ? 0 : g < 115 ? 1 : (g - 35) / 40;
|
||||
ib = b < 48 ? 0 : b < 115 ? 1 : (b - 35) / 40;
|
||||
cr = kXtermCube[ir];
|
||||
cg = kXtermCube[ig];
|
||||
cb = kXtermCube[ib];
|
||||
gv = 8 + 10 * grai;
|
||||
cerr = (cr-r)*(cr-r) + (cg-g)*(cg-g) + (cb-b)*(cb-b);
|
||||
gerr = (gv-r)*(gv-r) + (gv-g)*(gv-g) + (gv-b)*(gv-b);
|
||||
if (cerr <= gerr) {
|
||||
res = 16 + 36 * ir + 6 * ig + ib;
|
||||
} else {
|
||||
res = 232 + grai;
|
||||
}
|
||||
return PyLong_FromUnsignedLong(res);
|
||||
}
|
||||
|
||||
static PyMethodDef cosmo_methods[] = {
|
||||
{NULL, NULL} /* sentinel */
|
||||
{"ild", cosmo_ild, METH_VARARGS, ild_doc},
|
||||
{"rdtsc", cosmo_rdtsc, METH_NOARGS, rdtsc_doc},
|
||||
{"crc32c", cosmo_crc32c, METH_VARARGS, crc32c_doc},
|
||||
{"syscount", cosmo_syscount, METH_NOARGS, syscount_doc},
|
||||
{"popcount", cosmo_popcount, METH_VARARGS, popcount_doc},
|
||||
{"decimate", cosmo_decimate, METH_VARARGS, decimate_doc},
|
||||
{"getcpucore", cosmo_getcpucore, METH_NOARGS, getcpucore_doc},
|
||||
{"getcpunode", cosmo_getcpunode, METH_NOARGS, getcpunode_doc},
|
||||
{"rgb2xterm256", cosmo_rgb2xterm256, METH_VARARGS, rgb2xterm256_doc},
|
||||
#ifdef __PG__
|
||||
{"ftrace", cosmo_ftrace, METH_NOARGS, ftrace_doc},
|
||||
#endif
|
||||
{0},
|
||||
};
|
||||
|
||||
|
||||
static struct PyModuleDef cosmomodule = {
|
||||
PyModuleDef_HEAD_INIT,
|
||||
"_cosmo",
|
||||
doc_cosmo,
|
||||
"cosmo",
|
||||
cosmo_doc,
|
||||
-1,
|
||||
cosmo_methods,
|
||||
NULL,
|
||||
NULL,
|
||||
NULL,
|
||||
NULL
|
||||
};
|
||||
|
||||
static const char *
|
||||
GetKernelName(void) {
|
||||
if (IsLinux()) {
|
||||
return "linux";
|
||||
} else if (IsXnu()) {
|
||||
return "xnu";
|
||||
} else if (IsMetal()) {
|
||||
return "metal";
|
||||
} else if (IsWindows()) {
|
||||
return "nt";
|
||||
} else if (IsFreebsd()) {
|
||||
return "freebsd";
|
||||
} else if (IsOpenbsd()) {
|
||||
return "openbsd";
|
||||
} else if (IsNetbsd()) {
|
||||
return "netbsd";
|
||||
} else {
|
||||
return "wut";
|
||||
}
|
||||
}
|
||||
|
||||
PyMODINIT_FUNC
|
||||
PyInit_cosmo(void)
|
||||
{
|
||||
PyObject *m, *d;
|
||||
|
||||
m = PyModule_Create(&cosmomodule);
|
||||
if (m == NULL)
|
||||
goto failure;
|
||||
|
||||
if(cosmo_constants(m))
|
||||
goto failure;
|
||||
|
||||
return m;
|
||||
failure:
|
||||
Py_XDECREF(m);
|
||||
return NULL;
|
||||
PyObject *m;
|
||||
if (!(m = PyModule_Create(&cosmomodule))) return 0;
|
||||
PyModule_AddStringConstant(m, "MODE", MODE);
|
||||
PyModule_AddIntConstant(m, "IMAGE_BASE_VIRTUAL", IMAGE_BASE_VIRTUAL);
|
||||
PyModule_AddStringConstant(m, "kernel", GetKernelName());
|
||||
PyModule_AddIntConstant(m, "kStartTsc", kStartTsc);
|
||||
return !PyErr_Occurred() ? m : 0;
|
||||
}
|
||||
|
||||
_Section(".rodata.pytab.1") const struct _inittab _PyImport_Inittab_cosmo = {
|
||||
"cosmo",
|
||||
PyInit_cosmo,
|
||||
};
|
||||
|
|
Loading…
Add table
Add a link
Reference in a new issue