Cross helicity of magnetic clouds observed by Parker Solar Probe
<p>Magnetic clouds are large-scale transient structures in the solar wind with low plasma <em>&#946;</em>, low-amplitude magnetic field fluctuations, and twisted field lines with both ends often connected to the Sun. We analyse the normalised cross helicity, <em>&#963;</em><sub>c</sub>, and residual energy, <em>&#963;</em><sub>r</sub>, in magnetic clouds observed by Parker Solar Probe (PSP). In the November 2018 cloud observed at 0.25 au, a low value of <em>&#963;</em><sub>c</sub> was present in the cloud core, indicating that wave power parallel and anti-parallel to the mean field was approximately balanced, while the cloud&#8217;s outer layers displayed larger amplitude Alfv&#233;nic fluctuations with high <em>&#963;</em><sub>c</sub> values and <em>&#963;</em><sub>r</sub> ~ 0. These properties are compared and contrasted to those found in clouds observed by PSP at larger heliocentric distances. We suggest that low <em>&#963;</em><sub>c</sub> is likely a common feature of magnetic clouds given their typically closed field structure, in contrast to the generally higher <em>&#963;</em><sub>c</sub> found on the open field lines of the solar wind.</p>