A Search and Analysis Tool for HESSI Ancillary Observations

Astronomy and Astrophysics – Astrophysics

Scientific paper

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7500 Solar Physics, Astrophysics, And Astronomy, 7519 Flares

Scientific paper

To fully maximize its scientific return, the HESSI mission will rely heavily on coordinated analysis of context (or ancillary) observations from ground- and space-based observatories. To facilitate this analysis, we have developed an archive and software system that allows users to search, browse, and retrieve ancillary data for HESSI-observed flares. The system includes images, spectra, and lightcurves that span a wide range of wavelengths (radio, optical, UV/EUV, soft X-rays, and hard X-rays) as well as magnetic field observations. These observations are mirrored within 24 hours from remote sites around the world to a central server at the NASA/GSFC Solar Data Analysis Center. The central archive currently includes Yohkoh (SXT), SOHO (EIT, MDI), TRACE, H-alpha (Meudon), radio (RSTN, OVSA, Phoenix, Nancay, Nobeyama) and the Czech Hard X-ray Spectrometer observations. This poster will demonstrate an IDL interface that we have developed for accessing the HESSI ancillary data archive. [EOB]

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