Presentations

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?