67 citations · 264 across the 8 of their papers we have counts for
8 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…
The Double-Bubble CME of the 2020 December 14 Total Solar Eclipse
Benjamin Boe, Bryan Yamashiro, Miloslav Druckmuller +1
Total solar eclipses (TSEs) continue to provide an invaluable platform for exploring the magnetic topology of the solar corona and for studying dynamic events such as Coronal Mass…
Identifying the Coronal Source Regions of Solar Wind Streams from Total Solar Eclipse Observations and in situ Measurements Extending Over a Solar Cycle
Shadia R. Habbal, Miloslav Druckmuller, Nathalia Alzate +7
This Letter capitalizes on a unique set of total solar eclipse observations, acquired between 2006 and 2020, in white light, Fe XI 789.2 nm ( = MK) and…
The Color and Brightness of the F-Corona Inferred from the 2019 July 2 Total Solar Eclipse
Benjamin Boe, Shadia Habbal, Cooper Downs +1
Total solar eclipses (TSEs) provide a unique opportunity to quantify the properties of the K-corona (electrons), F-corona (dust) and E-corona (ions) continuously from the solar sur…
Coronal Magnetic Field Topology From Total Solar Eclipse Observations
Benjamin Boe, Shadia Habbal, Miloslav Druckmuller
Measuring the global magnetic field of the solar corona remains exceptionally challenging. The fine-scale density structures observed in white light images taken during Total Solar…
CME Induced Thermodynamic Changes in the Corona as Inferred from Fe XI and Fe XIV Emission Observations during the 2017 August 21 Total Solar Eclipse
Benjamin Boe, Shadia Habbal, Miloslav Druckmuller +3
We present the first remote sensing observations of the impact from a Coronal Mass Ejection (CME) on the thermodynamic properties of the solar corona between 1 and 3 Rs. Measuremen…
Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse
A. R. Yeates, T. Amari, I. Contopoulos +17
Seven different models are applied to the same problem of simulating the Sun's coronal magnetic field during the solar eclipse on 2015 March 20. All of the models are non-potential…
First Empirical Determination of the Fe 10+ and Fe 13+ Freeze-in Distances in the Solar Corona
Benjamin Boe, Shadia Habbal, Miloslav Druckmuller +5
Heavy ions are markers of the physical processes responsible for the density and temperature distribution throughout the fine scale magnetic structures that define the shape of the…