Ex 04: Query by TimeΒΆ
This is an example of converting Voyager 1 PWS waveform data to power spectral density in client code.
For long time durations it’s more efficent to read dynamic spectra directly from the server, for example this data source: tag:das2.org,2012:site:/uiowa/voyager/1/pws/uncalibrated/highrate_spectrogram, however dust hit processing must be preformed on the time-series data directly.
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 | # das2 module example 4
# Using the low-level server specific query interface to download Voyager
# PWS waveforms and plotting spectra generated from reference and offset
# time values
import numpy
import das2
# Read a data source definition given a catalog ID. The returned item will
# vary based on the contents of catalog file. This ID below corresponds to
# a data source collection.
sId = 'site:/uiowa/voyager/1/pws/uncalibrated/waveform'
col = das2.get_source(sId)
# Show the available query parameters for the primary data interface. Other
# ancillary interfaces can be defined such as coverage, psd, histogram etc.
dIface = col.interface('primary')
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