Solar wind energy flux observations in the inner heliosphere: First results from Parker Solar Probe
M. Liu, K. Issautier, N. Meyer-Vernet, M. Moncuquet, M. Maksimovic, J., S. Halekas, J. Huang, L. Griton, S. Bale, J. W. Bonnell, A. W. Case, K., Goetz, P. R. Harvey, J. C. Kasper, R. J. MacDowall, D. M. Malaspina, M., Pulupa, M. L. Stevens

TL;DR
This study measures the solar wind energy flux close to the Sun using Parker Solar Probe data, finding values consistent with previous observations and noting symmetrical distributions at these inner heliospheric distances.
Contribution
First detailed measurements of solar wind energy flux in the inner heliosphere using Parker Solar Probe data, extending previous observations closer to the Sun.
Findings
Energy flux normalized to 1 R_sun is about 70 W/m^2.
Distribution of energy flux is nearly Gaussian and symmetrical.
Inner heliosphere shows less interaction with transient plasma structures.
Abstract
We investigate the solar wind energy flux in the inner heliosphere using 12-day observations around each perihelion of Encounter One (E01), Two (E02), Four (E04), and Five (E05) of Parker Solar Probe (PSP), respectively, with a minimum heliocentric distance of 27.8 solar radii (). Energy flux was calculated based on electron parameters (density , core electron temperature , and suprathermal electron temperature ) obtained from the simplified analysis of the plasma quasi-thermal noise (QTN) spectrum measured by RFS/FIELDS and the bulk proton parameters (bulk speed and temperature ) measured by the Faraday Cup onboard PSP, SPC/SWEAP. Combining observations from E01, E02, E04, and E05, the averaged energy flux value normalized to 1 plus the energy necessary to overcome the solar gravitation () is about 7014 $W…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Geomagnetism and Paleomagnetism Studies
