It has been known for some time that there exists a substantial amount of 'hidden'magnetic
energy in the quiet solar photosphere, and unlocking an understanding of this phenomenon …

Context. While the longitudinal field that dominates in photospheric network regions has
been studied extensively, small-scale transverse fields have recently been found to be …

Context. With the advent of next generation high resolution telescopes, our understanding of
how the magnetic field is organized in the internetwork (IN) photosphere is likely to advance …

The objective of this thesis is to develop methods to improve the quality of restored ground-
based observations, and to use such restored observations, along with 3D radiative MHD …

Understanding the dynamics and energetics of the solar atmosphere requires a good
understanding of photospheric magnetic fields, particularly on small spatial scales. Through …

A new era of solar physics commences with observations of the quiet Sun using the 4-metre
Daniel K. Inouye Solar Telescope/Visible Spectropolarimeter (DKIST/ViSP). We present full …

The magnetic nature of the solar poles has profound implications for the solar cycle, space
weather, and space climate. Virtually every measurement of the magnetic field in the polar …

Internetwork (IN) magnetic fields are highly dynamic, short-lived magnetic structures that
populate the interior of supergranular cells. Since they are spread all over the Sun, they may …

Synthetic observations produced from radiative magnetohydrodynamic simulations have
predicted that higher polarization fractions in the quiet solar photosphere would be revealed …

Context. Early magnetographic observations indicated that the magnetic field in the solar
photosphere has an unresolved small-scale structure. Near-infrared and optical data with …