39 citations · 83 across the 5 of their papers we have counts for
5 papers
Evolving Solar Wind Flow Properties of Magnetic Inversions Observed by Helios
Allan R Macneil, Mathew J Owens, Robert T Wicks +1
In its first encounter at solar distances as close as r = 0.16AU, Parker Solar Probe (PSP) observed numerous local reversals, or inversions, in the heliospheric magnetic field (HMF…
Parker Solar Probe Observations of Suprathermal Electron Flux Enhancements Originating from Coronal Hole Boundaries
Allan R Macneil, Mathew J Owens, Laura Berčič +1
Reconnection between pairs of solar magnetic flux elements, one open and the other a closed loop, is theorised to be a crucial process for both maintaining the structure of the cor…
The Evolution of Inverted Magnetic Fields Through the Inner Heliosphere
Allan Macneil, Mathew Owens, Robert Wicks +3
Local inversions are often observed in the heliospheric magnetic field (HMF), but their origins and evolution are not yet fully understood.Parker Solar Probe has recently observed…
On the Origin of Otho-Gardenhose Heliospheric Flux
Mike Lockwood, Mat Owens, Allan Macneil
Parker spiral theory predicts the heliospheric magnetic field (HMF) will have components of opposite polarity radially toward the Sun and tangentially antiparallel to the solar rot…
Tests for coronal electron temperature signatures in suprathermal electron populations at 1 AU
Allan R. Macneil, Christopher J. Owen, Robert T. Wicks
The development of knowledge of how the coronal origin of the solar wind affects its in situ properties is one of the keys to understanding the relationship between the Sun and the…