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:
Justine Tunney 2021-09-27 22:58:51 -07:00
parent fa7b4f5bd1
commit 39bf41f4eb
806 changed files with 77494 additions and 63859 deletions

View file

@ -1,105 +1,316 @@
/*-*- mode:c;indent-tabs-mode:nil;c-basic-offset:2;tab-width:8;coding:utf-8 -*-│
vi: set net ft=c ts=2 sts=2 sw=2 fenc=utf-8 :vi
/*-*- mode:c;indent-tabs-mode:nil;c-basic-offset:4;tab-width:8;coding:utf-8 -*-│
vi: set net ft=c ts=4 sts=4 sw=4 fenc=utf-8 :vi
This is free and unencumbered software released into the public domain.
Copyright 2021 Justine Alexandra Roberts Tunney
Anyone is free to copy, modify, publish, use, compile, sell, or
distribute this software, either in source code form or as a compiled
binary, for any purpose, commercial or non-commercial, and by any
means.
Permission to use, copy, modify, and/or distribute this software for
any purpose with or without fee is hereby granted, provided that the
above copyright notice and this permission notice appear in all copies.
In jurisdictions that recognize copyright laws, the author or authors
of this software dedicate any and all copyright interest in the
software to the public domain. We make this dedication for the benefit
of the public at large and to the detriment of our heirs and
successors. We intend this dedication to be an overt act of
relinquishment in perpetuity of all present and future rights to this
software under copyright law.
THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND,
EXPRESS OR IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF
MERCHANTABILITY, FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT.
IN NO EVENT SHALL THE AUTHORS BE LIABLE FOR ANY CLAIM, DAMAGES OR
OTHER LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE,
ARISING FROM, OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR
OTHER DEALINGS IN THE SOFTWARE.
THE SOFTWARE IS PROVIDED "AS IS" AND THE AUTHOR DISCLAIMS ALL
WARRANTIES WITH REGARD TO THIS SOFTWARE INCLUDING ALL IMPLIED
WARRANTIES OF MERCHANTABILITY AND FITNESS. IN NO EVENT SHALL THE
AUTHOR BE LIABLE FOR ANY SPECIAL, DIRECT, INDIRECT, OR CONSEQUENTIAL
DAMAGES OR ANY DAMAGES WHATSOEVER RESULTING FROM LOSS OF USE, DATA OR
PROFITS, WHETHER IN AN ACTION OF CONTRACT, NEGLIGENCE OR OTHER
TORTIOUS ACTION, ARISING OUT OF OR IN CONNECTION WITH THE USE OR
PERFORMANCE OF THIS SOFTWARE.
*/
#include "third_party/python/Include/Python-ast.h"
#define PY_SSIZE_T_CLEAN
#include "dsp/scale/cdecimate2xuint8x8.h"
#include "libc/bits/popcnt.h"
#include "libc/dce.h"
#include "libc/macros.internal.h"
#include "libc/math.h"
#include "libc/mem/mem.h"
#include "libc/nexgen32e/crc32.h"
#include "libc/nexgen32e/rdtsc.h"
#include "libc/nexgen32e/rdtscp.h"
#include "libc/runtime/runtime.h"
#include "third_party/python/Include/abstract.h"
#include "third_party/python/Include/boolobject.h"
#include "third_party/python/Include/ceval.h"
#include "third_party/python/Include/code.h"
#include "third_party/python/Include/cosmo.h"
#include "third_party/python/Include/dictobject.h"
#include "third_party/python/Include/errcode.h"
#include "third_party/python/Include/eval.h"
#include "third_party/python/Include/fileutils.h"
#include "third_party/python/Include/frameobject.h"
#include "third_party/python/Include/import.h"
#include "third_party/python/Include/listobject.h"
#include "third_party/python/Include/longobject.h"
#include "third_party/python/Include/marshal.h"
#include "third_party/python/Include/methodobject.h"
#include "third_party/python/Include/modsupport.h"
#include "third_party/python/Include/objimpl.h"
#include "third_party/python/Include/osdefs.h"
#include "third_party/python/Include/pgenheaders.h"
#include "third_party/python/Include/pydebug.h"
#include "third_party/python/Include/moduleobject.h"
#include "third_party/python/Include/pyerrors.h"
#include "third_party/python/Include/pylifecycle.h"
#include "third_party/python/Include/pymacro.h"
#include "third_party/python/Include/pythonrun.h"
#include "third_party/python/Include/sysmodule.h"
#include "third_party/python/Include/traceback.h"
#include "third_party/python/Include/tupleobject.h"
#include "third_party/python/Include/warnings.h"
#include "third_party/python/Include/weakrefobject.h"
#include "third_party/python/Include/yoink.h"
#include "third_party/python/Python/importdl.h"
#include "third_party/xed/x86.h"
/* clang-format off */
PYTHON_PROVIDE("_cosmo");
PYTHON_PROVIDE("cosmo");
static int cosmo_constants(PyObject *m)
PyDoc_STRVAR(cosmo_doc,
"Cosmopolitan Libc Module\n\
\n\
This module exposes low-level utilities from the Cosmopolitan library.\n\
\n\
Static objects:\n\
\n\
MODE -- make build mode, e.g. \"\", \"tiny\", \"opt\", \"rel\", etc.\n\
IMAGE_BASE_VIRTUAL -- base address of actually portable executable image\n\
kernel -- o/s platform, e.g. \"linux\", \"xnu\", \"metal\", \"nt\", etc.\n\
kStartTsc -- the rdtsc() value at process creation.");
PyDoc_STRVAR(syscount_doc,
"syscount($module)\n\
--\n\n\
Returns number of SYSCALL instructions issued to kernel by C library.\n\
\n\
Context switching from userspace to kernelspace is expensive! So it is\n\
useful to be able to know how many times that's happening in your app.\n\
\n\
This value currently isn't meaningful on Windows NT, where it currently\n\
tracks the number of POSIX calls that were attempted, but have not been\n\
polyfilled yet.");
static PyObject *
cosmo_syscount(PyObject *self, PyObject *noargs)
{
if(PyModule_AddStringMacro(m, MODE)) return -1;
return 0;
return PyLong_FromSize_t(g_syscount);
}
PyDoc_STRVAR(rdtsc_doc,
"rdtsc($module)\n\
--\n\n\
Returns CPU timestamp counter.");
PyDoc_STRVAR(doc_cosmo,
"additional information and special functions provided by Cosmopolitan Libc.");
static PyObject *
cosmo_rdtsc(PyObject *self, PyObject *noargs)
{
return PyLong_FromUnsignedLong(rdtsc());
}
PyDoc_STRVAR(getcpucore_doc,
"getcpucore($module)\n\
--\n\n\
Returns 0-indexed CPU core on which process is currently scheduled.");
static PyObject *
cosmo_getcpucore(PyObject *self, PyObject *noargs)
{
return PyLong_FromUnsignedLong(TSC_AUX_CORE(rdpid()));
}
PyDoc_STRVAR(getcpunode_doc,
"getcpunode($module)\n\
--\n\n\
Returns 0-indexed NUMA node on which process is currently scheduled.");
static PyObject *
cosmo_getcpunode(PyObject *self, PyObject *noargs)
{
return PyLong_FromUnsignedLong(TSC_AUX_NODE(rdpid()));
}
PyDoc_STRVAR(ftrace_doc,
"ftrace($module)\n\
--\n\n\
Enables logging of C function calls to stderr, e.g.\n\
\n\
cosmo.ftrace()\n\
WeirdFunction()\n\
os._exit(1)\n\
\n\
Please be warned this prints massive amount of text. In order for it\n\
to work, the concomitant .com.dbg binary needs to be present.");
static PyObject *
cosmo_ftrace(PyObject *self, PyObject *noargs)
{
ftrace_install();
return Py_None;
}
PyDoc_STRVAR(crc32c_doc,
"crc32c($module, bytes, init=0)\n\
--\n\n\
Computes 32-bit Castagnoli Cyclic Redundancy Check.\n\
\n\
Used by ISCSI, TensorFlow, etc.\n\
Similar to zlib.crc32().");
static PyObject *
cosmo_crc32c(PyObject *self, PyObject *args)
{
Py_ssize_t n;
Py_buffer data;
unsigned crc, init = 0;
if (!PyArg_ParseTuple(args, "y*|I:crc32c", &data, &init)) return 0;
crc = crc32c(init, data.buf, data.len);
PyBuffer_Release(&data);
return PyLong_FromUnsignedLong(crc);
}
PyDoc_STRVAR(decimate_doc,
"decimate($module, bytes)\n\
--\n\n\
Shrinks byte buffer in half using John Costella's magic kernel.\n\
\n\
This downscales data 2x using an eight-tap convolution, e.g.\n\
\n\
>>> cosmo.decimate(b'\\xff\\xff\\x00\\x00\\xff\\xff\\x00\\x00\\xff\\xff\\x00\\x00')\n\
b'\\xff\\x00\\xff\\x00\\xff\\x00'\n\
\n\
This is very fast if SSSE3 is available (Intel 2004+ / AMD 2011+).");
static PyObject *
cosmo_decimate(PyObject *self, PyObject *args)
{
Py_ssize_t n;
PyObject *buf;
Py_buffer data;
if (!PyArg_ParseTuple(args, "y*:decimate", &data)) return 0;
if ((buf = PyBytes_FromStringAndSize(0, (n = ROUNDUP(data.len, 16))))) {
memcpy(PyBytes_AS_STRING(buf), data.buf, data.len);
memset(PyBytes_AS_STRING(buf) + data.len, 0, n - data.len);
cDecimate2xUint8x8(n, (void *)PyBytes_AS_STRING(buf),
(signed char[8]){-1, -3, 3, 17, 17, 3, -3, -1});
_PyBytes_Resize(&buf, (data.len + 1) >> 1);
}
PyBuffer_Release(&data);
return buf;
}
PyDoc_STRVAR(ild_doc,
"ild($module, bytes)\n\
--\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.");
static PyObject *
cosmo_ild(PyObject *self, PyObject *args)
{
Py_ssize_t n;
const char *p;
enum XedError e;
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,
"popcount($module, bytes)\n\
--\n\n\
Returns population count of byte sequence, e.g.\n\
\n\
>>> cosmo.popcount(b'\\xff\\x00\\xff')\n\
16\n\
\n\
The population count is the number of bits that are set to one.\n\
It does the same thing as `Long.bit_count()` but for data buffers.\n\
This goes 30gbps on Nehalem (Intel 2008+) so it's quite fast.");
static PyObject *
cosmo_popcount(PyObject *self, PyObject *args)
{
Py_ssize_t n;
const char *p;
if (!PyArg_ParseTuple(args, "y#:popcount", &p, &n)) return 0;
return PyLong_FromSize_t(_countbits(p, n));
}
PyDoc_STRVAR(rgb2xterm256_doc,
"rgb2xterm256($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,
};