Over the past ten years there has been a large increase in the number of projects using
sound to represent astronomical data and concepts. Motivation for these projects includes …

The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …

In situ measurements of the solar wind have been available for almost 60 years, and in that
time plasma physics simulation capabilities have commenced and ground‐based solar …

It is common for us today to associate the practice of science primarily with the act of seeing—
with staring at computer screens, analyzing graphs, and presenting images. We may notice …

While it is certain that the fast solar wind originates from coronal holes, where and how the
slow solar wind (SSW) is formed remains an outstanding question in solar physics even in …

A three‐parameter algebraic scheme is developed to categorize the solar wind at 1 AU into
four plasma types: coronal‐hole‐origin plasma, streamer‐belt‐origin plasma, sector …

Robustly identifying the solar sources of individual packets of solar wind measured in
interplanetary space remains an open problem. We set out to see if this problem is easier to …

Sonification is the technique of representing data with sound, with potential applications in
astronomy research for aiding discovery and accessibility. Several astronomy-focused …

Whereas slow solar wind is known to be highly structured, the fast (coronal hole origin) wind
is usually considered to be homogeneous. Using measurements from Helios 1+ 2, ACE …

We use audification of 0.092 s cadence magnetometer data from the Wind spacecraft to
identify waves with amplitudes $\gt 0.1$ nT near the ion gyrofrequency (∼ 0.1 Hz) with …