Last Update 28-Jan-2024, Kim Tolbert (kim.tolbert at nasa.gov)
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) recorded X-ray data between 3 keV and 17 MeV from the Sun between February 2012 and April 2018. Please see the RHESSI web site at https://hesperia.gsfc.nasa.gov/rhessi for a complete description of the mission, the instrument, and the software needed to analyze the data.
These directories contain the primary RHESSI data archive of raw data and various quicklook products. There are additional archived RHESSI data products here (please read the aa_readme_rhessi_extras file there for descriptions of those files).
These directories are organized as follows:
Year directories | Raw Level-0 packed telemetry data for the full mission in FITS files, usually each covering one 90-minute orbit. These files contain the energy and time of arrival for every HXR photon detected. The RHESSI software in SSW is required to unpack the telemetry stream and construct spectra, time profiles, and images from these data. Files are named hsi_yyyymmdd_hhmmss_ver.fits, where the date and time are the start time of the file, and ver is a version number. | ||||||||||||||||
DBASE directory |
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METADATA directory |
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