Academic and public talks, slideshows for sharing information with collaborators
Occulted Flares observed by RHESSI and MESSENGER
Talk given at the 2017 RHESSI Workshop
Non-LTE Formation of Photospheric Fe-I Lines
Poster presented at NSO Sunspot Workshop 2017
The Micro Solar Flare Apparatus (MiSolFA)
Poster presented at the 2018 Solar Physics Division of the AAS meeting
Highly Occulted Flare and CME of May 1,2013
Talk given at 2018 RHESSI Workshop
The Micro Solar Flare Apparatus (MiSolFA) and High-energy Solar Observations from Multiple Perspectives
PhD thesis defense talk
SKA SDC2 Truth Catalog Exploration & De-Noising Attempts
Prep work for the SKA Science Data Challenge 2
NuSTAR temperature and loci curves
Small solar flare of 12 September 2020
The Sun in Data
Zurich Women in Machine Learning and Data
Science (WiMLDS) event public talk
AIA + XRT + NuSTAR DEM
Joint Differential Emission Measure inversion
with three instruments
Joint DEM 12-Sept-2021 (orbit 6)
12 September 2020 flare at 17:00
Joint DEM 12-Sept-2021 (orbit 8)
12 September 2020 flare at 20:40
Joint DEM 12-Sept-2021 (orbit 8 updated)
using NuSTAR counts from spectrum files and including contribution functions
PyXspec fit comparisons with NuSTAR orbit 8 data
With fixed T but EM allowed to vary, how does this compare to best fit result?
CFL, Back Projection, and AIA Flare Location Comparison
How do flare locations given by the STIX
Coarse Flare Locator, STIX Back Projection images, and the HEK/AIA
database compare?
Notebook - visualization
For Andrea
Gaussian Mixture Model applied to Back Projection and AIA Flare Locations
Do the flares which
disagree strongly in location determined via STIX and AIA come from
different populations, based only on the features of the flares themselves?
STIX-GOES Relationship
What is the relationship between peak counts in STIX flares and GOES class/flux?
STIX-GOES Relationship - simplified
with additional explanation and more code
for non-solar specialists
Thermal + Thick-target fit with pyXspec
Optimizing sunxspex's thick-target model for
speed and
use with XSPEC
STIX-GOES Relationship with background subtraction
How does subtraction of daily X-ray background measurements affect the relationship between STIX counts and GOES flux?