Goldhelox: A Soft X-Ray Solar Telescope

Article type: Research Article

Authors: Durfee, D. S. | Moody, J. W. | Brady, K. D. | Brown, C. | Campbell, B. | Durfee, M. K. | Early, D. | Hansen, E. | Madsen, D. W. | Morey, D. B. | Roming, P. W. A. | Savage, M. B. | Eastman, P. F. | Jensen, V.

Affiliations: Department of Physics and Astronomy, Brigham Young University, Provo Utah, 84602

Abstract: The Goldhelox Project is the construction and use of a near-normal incidence soft x-ray robotic solar telescope by undergraduate students at Brigham Young University. Once it is completed and tested, it will be deployed from a Get-Away-Special (GAS) canister in the bay of a space shuttle. It will image the sun at a wavelength of 171-181Å with a time resolution of 1 sec and a spatial resolution of 2.5 arcsec. The observational bandpass was chosen to image x-rays from highly ionized coronal Fe lines. The data will be an aid in better understanding the beginning phases of solar flares and how flaring relates to the physics of the corona-chromosphere transition region. Goldhelox is tentatively scheduled to fly on a space shuttle sometime in 1995 or 1996. This paper outlines the project goals, basic instrument design, and the unique aspects of making this an undergraduate endeavor.

DOI: 10.3233/XST-1995-5102

Journal: Journal of X-Ray Science and Technology, vol. 5, no. 1, pp. 20-28, 1995