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A list of all the posts and pages found on the site. For you robots out there is an XML version available for digesting as well.
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Posts
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outreach
publications
A Solar-cycle Study of Coronal Rotation: Large Variations, Rapid Changes, and Implications for Solar-wind Models
Published in The Astrophysical Journal, 2022
Information on the rotation rate of the corona, and its variation over latitude and solar cycle, is valuable for making global connections between the corona and the Sun, for global estimates of reconnection rates and as a basic parameter for solar-wind modeling. Here, we use a time series of tomographical maps gained from coronagraph observations between 2007 and 2020 to directly measure the longitudinal drift of high-density streamers over time. The method reveals abrupt changes in rotation rates, revealing a complex relationship between the coronal rotation and the underlying photosphere. The majority of rates are between −1.0 degree/day to +0.5 degree/day relative to the standard Carrington rate of 14.18 degree/day, although rates are measured as low as −2.2 degree/day and as high as 1.6 degree/day. Equatorial rotation rates during the 2008 solar minimum are slightly faster than the Carrington rate, with an abrupt switch to slow rotation in 2009, then a return to faster rates in 2017. Abrupt changes and large variations in rates are seen at all latitudes. Comparison with a magnetic model suggests that periods of equatorial fast rotation are associated with times when a large proportion of the magnetic footpoints of equatorial streamers are near the equator, and we interpret the abrupt changes in terms of the latitudinal distribution of the streamer photospheric footpoints. The coronal rotation rate is a key parameter for solar-wind models, and variations of up to a degree per day or more can lead to large systematic errors over forecasting periods of longer than a few days. The approach described in this paper gives corrected values that can form a part of future forecasting efforts.
Recommended citation: Liam Edwards et al. 2022 ApJ 928 42 http://liamtomosedwards.github.io/files/Edwards_2022_ApJ_928_42.pdf
Derived Electron Densities from Linear Polarization Observations of the Visible-Light Corona During the 14 December 2020 Total Solar Eclipse
Published in Solar Physics, 2023
A new instrument was designed to take visible-light (VL) polarized brightness (pB) observations of the solar corona during the 14 December 2020 total solar eclipse. The instrument, called the Coronal Imaging Polarizer (CIP), consisted of a 16 MP CMOS detector, a linear polarizer housed within a piezoelectric rotation mount, and an f-5.6, 200 mm DSLR lens. Observations were successfully obtained, despite poor weather conditions, for five different exposure times (0.001 s, 0.01 s, 0.1 s, 1 s, and 3 s) at six different orientation angles of the linear polarizer (0 degree, 30 degree, 60 degree, 90 degree, 120 degree, 150 degree). The images were manually aligned using the drift of background stars in the sky and images of different exposure times were combined using a simple signal-to-noise ratio cut. The polarization and brightness of the local sky were also estimated and the observations were subsequently corrected. The pB of the K-corona was determined using least-squares fitting and radiometric calibration was done relative to the Mauna Loa Solar Observatory (MLSO) K-Cor pB observations from the day of the eclipse. The pB data was then inverted to acquire the coronal electron density, n_e, for an equatorial streamer and a polar coronal hole, which agreed very well with previous studies. The effect of changing the number of polarizer angles used to compute the pB is also discussed and it is found that the results vary by up to approx. 13% when using all six polarizer angles versus only a select of three angles.
Recommended citation: Liam Edwards et al. 2023 Solar Physics 298 140 http://academicpages.github.io/files/s11207-023-02231-5.pdf
talks
Talk 1 on Relevant Topic in Your Field
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Conference Proceeding talk 3 on Relevant Topic in Your Field
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teaching
Postgraduate Demonstrator - PH15720 Laboratory Techniques for Experimental Physicists and Engineers
Undergraduate module, Aberystwyth University, 2019
This module introduced undergraduates to laboratory practice in key areas of the physical sciences, which can be used to understand the world around us. Emphasis was placed on accuracy of note-taking. Undergraduates were expected to keep a laboratory diary as they conducted the experiments. In addition to the notes kept in the diary, students were expected to write up two of the experiments as formal reports, including background research into the topics. In addition to this, in the second semester, students were introduced to ways of capturing and presenting data using electronic devices and computer packages.
Postgraduate Demonstrator - PH05720 Introduction to Laboratory Physics
Undergraduate module, Aberystwyth University, 2020
This laboratory module gave an introduction to experimental practices in the physical sciences. Emphasis was placed on the training of students to use basic instruments, perform simple error calculations, and critically assess results in order to draw reliable conclusions. Experiments were designed to reflect theoretical topics covered in other modules - hence included experiments covering properties of matter, forces, mechanics, electricity, magnetism, and electronics. Presentational skills were also developed in the context of experiments.
Postgraduate Demonstrator - PH10020 Dynamics, Waves and Heat
Undergraduate module, Aberystwyth University, 2023
The module presented core topics in Physical Sciences degree schemes and their applications. It comprised of three main parts. The first part covered translational, rotational and oscillatory motion. The second part introduced waves and the behaviour of light. Thermal physics on macroscopic and atomic scales was considered in the final section.
Guest Lecturer - PH38410 The Solar Atmosphere & Heliosphere
Undergraduate module, Aberystwyth University, 2023
This module provided an in-depth treatment of the physics of the solar atmosphere and heliosphere, including coupling between the solar wind and non-magnetised objects.