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The Solar X-ray Limb View all abstracts by submitter

Marina Battaglia   Submitted: 2017-06-01 01:03

We describe a new technique to measure the height of the X-ray limb with observations from occulted X-ray flare sources as observed by the RHESSI (the Reuven Ramaty High-Energy Spectroscopic Imager) satellite. This method has model dependencies different from those present in traditional observations at optical wavelengths, which depend upon detailed modeling involving radiative transfer in a medium with complicated geometry and flows. It thus provides an independent and more rigorous measurement of the ''true'' solar radius, meaning that of the mass distribution. RHESSI's measurement makes use of the flare X-ray source's spatial Fourier components (the visibilities), which are sensitive to the presence of the sharp edge at the lower boundary of the occulted source. We have found a suitable flare event for analysis, SOL2011-10-20T03:25 (M1.7), and report a first result from this novel technique here. Using a 4-minute integration over the 3-25 keV photon energy range, we find RX-ray=964.05 ? 0.15-0.29 arcsec, where the uncertainties include statistical uncertainties from the method and a systematic error. The standard VAL-C model predicts a value of 963.48 arcsec, about 2σ below our value.

Authors: M. Battaglia, H. S. Hudson, G. J. Hurford, S. Krucker, R. A. Schwartz
Projects: RHESSI

Publication Status: ApJ, accepted
Last Modified: 2017-06-01 10:21
Go to main E-Print page  Exploring the potential of microwave diagnostics in SEP forecasting: The occurrence of SEP events  HIGH-RESOLUTION OBSERVATIONS OF DOWNFLOWS AT ONE END OF A PRE-ERUPTION FILAMENT  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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