The solar atmosphere is known to be replete with magneto-hydrodynamic wave modes, and
there has been significant investment in understanding how these waves propagate through …

The Solar MAgnetic Connection HAUS tool (Solar-MACH) is an open-source tool completely
written in Python that derives and visualizes the spatial configuration and solar magnetic …

On 2022 February 15, an impressive filament eruption was observed off the solar eastern
limb from three remote-sensing viewpoints, namely, Earth, STEREO-A, and Solar Orbiter. In …

While the photospheric magnetic field of our Sun is routinely measured, its extent into the
upper atmosphere is typically not accessible by direct observations. Here we present an …

Abstract On 3 February 2022, SpaceX launched 49 Starlink satellites, 38 of which
unexpectedly de‐orbited. Although this event was attributed to space weather, definitive …

Sun-as-a-star analyses in which observational data is spatially integrated are useful for
interpreting stellar data. For future applications to stellar observations, we performed Sun-as …

Drawing connections between heliospheric spacecraft and solar wind sources is a vital step
in understanding the evolution of the solar corona into the solar wind and contextualizing in …

Context. On 2020 November 29, an eruptive event occurred in an active region located
behind the eastern solar limb as seen from Earth. The event consisted of an M4. 4 class …

This paper presents a multiwavelength Sun-as-a-star analysis of the M8. 7 flare on 2022
October 2, which was associated with a filament eruption and the subsequent coronal mass …

Context. Coronal dimmings are localized regions of reduced emission in the extreme-
ultraviolet (EUV) and soft X-rays formed as a result of the expansion and mass loss by …