Search Results - "Van Kooten, Samuel J."
-
1
Using Bright Point Shapes to Constrain Wave Heating of the Solar Corona: Predictions for DKIST
Published in The Astrophysical journal (01-03-2024)“…Abstract Magnetic bright points on the solar photosphere mark the footpoints of kilogauss magnetic flux tubes extending toward the corona. Convective buffeting…”
Get full text
Journal Article -
2
Characterizing the Motion of Solar Magnetic Bright Points at High Resolution
Published in The Astrophysical journal (20-11-2017)“…Magnetic bright points in the solar photosphere, visible in both continuum and G-band images, indicate footpoints of kilogauss magnetic flux tubes extending to…”
Get full text
Journal Article -
3
Defining the Middle Corona
Published in Solar physics (01-06-2023)“…The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar radii, encompasses almost all of the influential physical transitions…”
Get full text
Journal Article -
4
Defining the Flora Family: Orbital properties, reflectance properties and age
Published in Icarus (New York, N.Y. 1962) (01-11-2014)“…•We introduce the “core sample method” for family identification.•We find the Flora family to be distinct in orbital and reflectance properties.•We use this…”
Get full text
Journal Article -
5
A Refined Model of Convectively Driven Flicker in Kepler Light Curves
Published in The Astrophysical journal (01-05-2021)“…Abstract Light curves produced by the Kepler mission demonstrate stochastic brightness fluctuations (or flicker ) of stellar origin which contribute to the…”
Get full text
Journal Article -
6
Observations of the Polarized Solar Corona During the Annular Eclipse of 14 October 2023
Published in Solar physics (01-06-2024)“…We present results of a dual eclipse expedition to observe the solar corona from two sites during the annular solar eclipse of 14 October 2023 using a novel…”
Get full text
Journal Article -
7
Cause and Effect: Stellar Convection Studied through Flickering Brightness, and the Convectively-Driven Motions of Solar Bright Points
Published 01-01-2021“…Magnetic bright points on the solar photosphere, prominent in the G band but also visible in the continuum, mark the footpoints of kilogauss magnetic flux…”
Get full text
Dissertation -
8
Cause and Effect: Stellar Convection Studied Through Flickering Brightness, and the Convectively-Driven Motions of Solar Bright Points
Published 24-08-2021“…Magnetic bright points on the solar photosphere mark the footpoints of kilogauss magnetic flux tubes extending toward the corona. Convective buffeting of these…”
Get full text
Journal Article -
9
Using Bright-Point Shapes to Constrain Wave-Heating of the Solar Corona: Predictions for DKIST
Published 19-01-2024“…Magnetic bright points on the solar photosphere mark the footpoints of kilogauss magnetic flux tubes extending toward the corona. Convective buffeting of these…”
Get full text
Journal Article -
10
A Refined Model of Convectively-Driven Flicker in Kepler Light Curves
Published 13-04-2021“…Light curves produced by the Kepler mission demonstrate stochastic brightness fluctuations (or "flicker") of stellar origin which contribute to the noise…”
Get full text
Journal Article -
11
Observations of the Polarized Solar Corona during the Annular Eclipse of October 14, 2023
Published 03-04-2024“…Solar Physics, Vol. 299, 79 (20pp); 2024 June 10 We present results of a dual eclipse expedition to observe the solar corona from two sites during the annular…”
Get full text
Journal Article -
12
Characterizing the Motion of Solar Magnetic Bright Points at High Resolution
Published 12-10-2017“…Magnetic bright points in the solar photosphere, visible in both continuum and G-band images, indicate footpoints of kilogauss magnetic flux tubes extending to…”
Get full text
Journal Article -
13
Moosinesq Convection in the Cores of Moosive Stars
Published 30-03-2022“…Stars with masses $\gtrsim 4 \times 10^{27}M_{\rm{moose}} \approx 1.1 M_\odot$ have core convection zones during their time on the main sequence. In these…”
Get full text
Journal Article -
14
Defining the Middle Corona
Published 09-03-2023“…Solar Physics, Vol. 298, 78 (61pp); 2023 June 14 The middle corona, the region roughly spanning heliocentric altitudes from $1.5$ to $6\,R_\odot$, encompasses…”
Get full text
Journal Article -
15
The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
Published 28-06-2022“…The Astropy Project supports and fosters the development of open-source and openly-developed Python packages that provide commonly needed functionality to the…”
Get full text
Journal Article -
16
Defining the Flora Family: Orbital Properties, Reflectance Properties and Age
Published 27-04-2014“…The Flora family resides in the densely populated inner main belt, bounded in semimajor axis by the $\nu_6$ secular resonance and the Jupiter 3:1 mean motion…”
Get full text
Journal Article