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GUSTO Ground Data System

GUSTO is a suborbital NASA Explorers Mission of Opportunity launched from McMurdo Station (Antarctica) on a long duration stratospheric balloon on 31 December 2023, flying for a record 57+ days before landing on Mac Robsertson Land near the Antarctic coast between Davis and Mawson stations (AUS). This repository serves the development of the data system to process the downlinked science data and telemetry into deliverable science products.

GUSTO mission and science

GUSTO deployed a 0.9-meter telescope coupled to a 150 liter liquid helium hybrid cryostat which served to keep its suite of three 8-pixel heterodyne mixer arrays cooled to 4-6K over a 50-80 day mission. Each heterodyne pixel delivers a high resolution spectrum, and the telescope served a mission of drift-scanning the Milky Way and LMC to amass a spectroscopic survey in the far-infrared light of the ionized carbon at 157.7 microns (1900 GHz) and ionized nitrogen at 205 microns (1461 GHz).

Data System Documentation

An overview slide sketching the highest-level data flow of the pipeline is shown here: pipeline-convergence-9_9_2024

Data Level Definitions

Raw Level 0 lag files

Level 0 data is pulled from the autocorrelation spectrometers as raw lags coupled with a minimal spectrometer header, with instrument telemetry captured into a standalone Influx database.

Level 0.5-0.9 spectral bandpasses

At level 0.5, the lag files are converted to power spectra and incorporated into an SDFITS container by GUSTO scan ID. At level 0.7, the instrument telemetry is concatenated into the FITS header. At level 0.8, the data are despurred and channel flags updated. At level 0.9, the bandpasses are normalized by calibration frames and a second round of despurring is performed.

Level 0.95-1 calibrated spectra

At level 0.95, the data have residual baseline structure removed and the per-pixel pointing updated in the final level 1 products.

Level 2 maps

Based on the spectral quality factors assigned before level 1, the level 2 processor assigns weights to each spectrum, and remaps the "random" sampling of the on-the-fly (drift scanning) observations into a regularly sampled grid. The product of the level 2 processor are 3D FITS cubes with a tile size of the order of 1-2 square degrees.

Further reading

The GUSTO Science Data Management Plan is available here.

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