Jay M. Pasachoff

TL;DR: A brief history of coronal studies can be found in this paper, where the authors describe the first four decades of the solar cycle and the first 4 decades of ground-based observations from space.

TL;DR: Observations at a variety of visible and infrared wavelengths of an occultation of a star by Pluto in August 2002 reveal evidence for extinction in Pluto's atmosphere and show that it has indeed changed, having expanded rather than collapsed, since 1988.

TL;DR: In this article, a 3D magnetohydrodynamic model of the solar corona driven by measured magnetic fields was used to predict what the corona would look like one week before the eclipse.

TL;DR: In this paper, an observational program at the Sacramento Peak Observatory in 1965 provided high-dispersion spectra of the solar chromosphere in several spectral regions simultaneously, including the spectral lines Hα, Hβ and Hβ, the D3-line of Hei, the infrared triplet of Oi, and the H- and K-lines of ionized calcium.

TL;DR: Observations of a multi-chord stellar occultation by KBO 55636, which occurred on 9 October 2009, find that it has a mean radius of 143 ± 5 km and a geometric albedo of in the V photometric band, which establishes that KBO55636 is smaller than previously thought and that, like its parent body, it is highly reflective.