54 citations · 316 across the 15 of their papers we have counts for
15 papers
The 2023 Australian Total Solar Eclipse: Line Emission of Fe XIV, Fe X and Fe XI out to 6 solar radii
Benjamin Boe, Shadia Habbal, Miloslav Druckmüller +6
We present narrowband observations of the Fe XIV (530.3 nm), Fe X (637.4 nm), and Fe XI (789.2 nm) coronal emission lines from the 2023 April 20 Total Solar Eclipse in Australia. W…
Total Solar Eclipse White Light Images as a Benchmark for PFSS Coronal Magnetic Field Models: An In-Depth Analysis over a Solar Cycle
Luke Fushimi Benavitz, Benjamin Boe, Shadia Rifai Habbal
Potential Field Source Surface (PFSS) models are widely used to simulate coronal magnetic fields. PFSS models use the observed photospheric magnetic field as the inner boundary con…
Spectroscopic Observations of the Solar Corona during the 2017 August 21 Total Solar Eclipse: Comparison of Spectral Line Widths and Doppler Shifts Between Open and Closed Magnetic Structures
Yingjie Zhu, Shadia R. Habbal, Adalbert Ding +5
The spectroscopic observations presented here were acquired during the 2017 August 21 total solar eclipse with a three-channel partially multiplexed imaging spectrometer (3PAMIS) o…
The Solar Minimum Eclipse of 2019 July 2. III. Inferring the Coronal with a Radiative Differential Emission Measure Inversion
Benjamin Boe, Cooper Downs, Shadia Habbal
Differential Emission Measure (DEM) inversion methods use the brightness of a set of emission lines to infer the line-of-sight (LOS) distribution of the electron temperature (…
A Total Solar Eclipse Earth-Based Mission: Multi-wavelength Observations from Land, Sea and Air to Probe the Critical middle Corona
Shadia R Habbal, Benjamin Boe, Colby Haggerty +1
There has been an unfortunate gap in coronal emission line observations from space in the visible and near IR (V+NIR). Their distinct scientific advantage stems from the dominance…
The Need for a New Generation of Space-based Visible and Near-IR Emission Line Observations of the Corona
Benjamin Boe, Shadia Habbal, Adalbert Ding
Visible and near-infrared (V+NIR) emission lines were the first to be discovered in the corona, during total solar eclipses, and they continue to offer unique opportunities to stud…