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docs/code_usage_guide.ipynb

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"id": "89e9e3bc",
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"# Data conversion\n",
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"## Data conversion\n",
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"\n",
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"We can produce a data file that BiCEP can read internally from the magic format using the `generate_arai_plot_table` function in the `conversion` module. We will specify an output name of `BiCEP_converted.csv`. This gets dumped in the folder with the datafiles. For your convenience, we have included a set of MagIC formatted data to convert to the BiCEP format. This may take a few minutes"
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"# Data processing and analysis\n",
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"## Data processing and analysis\n",
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"### Looking at site and specimen data\n",
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"\n",
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"We can index for our sites and specimens using a key for the site name. Let's look at site \"hw126\" and print out the object to see the specimens. This site is a lava flow erupted in Hawaii in 1935 and originally analyzed by Cromwell et al (2015). Because this eruption occurred in the age of instrumentation, we know that the original field this lava flow was erupted in was approximately 36.4 μT.\n"
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"# Automating, diagnostics and saving fits\n",
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"## Automating, diagnostics and saving fits\n",
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"We can test whether a fit has yielded a successful paleointensity using the `get_sampler_succcess()` function from the `extract` module. Check the docstring to see options - but by default this only accepts things which are an A or a B grade."
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"# Advanced user options - tweaks and accessing raw data\n",
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"## Advanced user options - tweaks and accessing raw data\n",
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"### The \"fit\" object\n",
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"For each site, BiCEP creates a `fit` attribute which contains all the information for the fit to that specimen. This is an `arviz.InferenceData` object"
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