{ "info": { "author": "Michael Hirsch, Ph.D.", "author_email": "scivision@noreply.users.github.com", "bugtrack_url": null, "classifiers": [ "Development Status :: 4 - Beta", "Intended Audience :: Science/Research", "Programming Language :: Python :: 3.6", "Programming Language :: Python :: 3.7", "Programming Language :: Python :: 3.8", "Topic :: Scientific/Engineering :: Atmospheric Science", "Topic :: Utilities" ], "description": "[![DOI](https://zenodo.org/badge/30336524.svg)](https://zenodo.org/badge/latestdoi/30336524)\n\n[![Build Status](https://travis-ci.com/space-physics/histutils.svg?branch=master)](https://travis-ci.com/space-physics/histutils)\n[![Coverage Status](https://coveralls.io/repos/github/space-physics/histutils/badge.svg?branch=master)](https://coveralls.io/github/space-physics/histutils?branch=master)\n[![pypi versions](https://img.shields.io/pypi/pyversions/histutils.svg)](https://pypi.python.org/pypi/histutils)\n[![PyPi Download stats](http://pepy.tech/badge/histutils)](http://pepy.tech/project/histutils)\n\n\n# HiST Utils\n\nHiST project raw video data reading utilities.\n\n## Install\n\n python -m pip install -e .\n\n## User Programs/Scripts\n\nThese functions are primarily made to be used from the Terminal by a\nhuman, they implement a complete program using the module functions.\n\n### RunSimulPlay\n\nSimultaneous video playback of two or more cameras.\n\n* -i input file list (.h5)\n* -t Time range start/stop\n* -o Output directory for plots (optional, slow)\n\n#### Example\n\n```bash\n$ python RunSimulFrame.py -i ~/data/cmos2013-01-14T1-15.h5 ~/data/ccd2013-01-14T1-15.h5\n```\n\nusing the [data from January 13, 2013\nexperiment](http://heaviside.bu.edu/~mhirsch/dmc/2013-01-13/) during\nactive plasma time.\n\n### ConvertDMC2h5.py\n\nTypically used by our staff internally to convert our binary .DMCdata\nfiles to human- and fast processing- friendly HDF5 files.\n\n#### Example\n\n python ConvertDMC2h5.py -p 512 512 -b 1 1 -k 0.0188679245283019 -o testframes_cam0.h5 ~/data/2013-04-14T07-00-CamSer7196_frames_363000-1-369200.DMCdata -s 2013-04-14T06:59:55Z -t 2013-04-14T08:54:10Z 2013-04-14T08:54:10.05Z\n\n python ConvertDMC2h5.py -p 512 512 -b 1 1 -k 0.0333333333333333 -o testframes_cam1.h5 ~/data/2013-04-14T07-00-CamSer1387_frames_205111-1-208621.DMCdata -s 2013-04-14T07:00:07Z -t 2013-04-14T08:54:10Z 2013-04-14T08:54:10.05Z\n\n### WhenEnd.py\n\nJust predicts the end of a .DMCdata file \"does this file cover the\nauroral event time?\"\n\n## Module Functions\n\nThese functions are typically targeted for calling from other programs,\nhowever, many of these can also be used from the Terminal directly.\n\n## Examples\n\nMany more possibilities exist, the `-h` option on most functions will\ngive some hints as to what the program can do.\n\n## Reference Examples\n\nThese examples are old, now we use HDF5 files. Kept for reference only.\n\n### Read .DMCdata file from within a Python script\n\n from histutils import rawDMCreader\n data = rawDMCreader.goRead('myfile.DMCdata')[0]\n\n### Using rawDMCreader.py from Terminal\n\n cd histutils/histutils\n python3 rawDMCreader.py ~/data/", "description_content_type": "text/markdown", "docs_url": null, "download_url": "", "downloads": { "last_day": -1, "last_month": -1, "last_week": -1 }, "home_page": "https://github.com/space-physics/histutils", "keywords": "aurora", "license": "", "maintainer": "", "maintainer_email": "", "name": "histutils", "package_url": "https://pypi.org/project/histutils/", "platform": "", "project_url": "https://pypi.org/project/histutils/", "project_urls": { "Homepage": "https://github.com/space-physics/histutils" }, "release_url": "https://pypi.org/project/histutils/1.0.1/", "requires_dist": null, "requires_python": ">= 3.6", "summary": "Utilities for reading HiST data, etc.", "version": "1.0.1" }, "last_serial": 5463855, 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