Unresolved Coronal Structures: I am forward modeling coronal loops from SXT observed
flares, and XRT observed Active Region Transient Brightentings. The model allows many unresolved loops to be
contained within the observed pixel, which better matches the observed light curves.
XRT Noise: I am attempting to characterize the sources of uncertainty within the X-Ray
Telescope (XRT) on board the HINODE satellite, to create a toolset to be implemented with the
prepping of the XRT data which will return the uncertainty in the value of each pixel.
Information on the JPEG compression can be found
Heliophysics Knowledge Base: Search through and notate features in the TRACE catalog of data
HyLoop: Look at solar flares taken by SXT and analyze the evolution of the source loop
for comparison to predictions of the HyLoop suite written by