Electric Fields, Currents, and Magnetic Fluctuations of the Photosphere and Solar Wind
Abstract
In the (collisional) solar interior, the heat flux necessarily generates a radial electric field, integrating to a surface field eEth(Rs)≅1.4eV/Mm, comparable to the proton weight mpg = 2.8eV/Mm. In the (less collisional) plasma "sheath" of the photosphere and heliosphere, the outward photon flux Γγ = 60.MW/m2 causes additional electron displacement, giving eEγ(r) =σγe Γγ /c. Here, the main uncertainty is the photon cross-section σγe for electrons correlated with protons: H-minus and "rydberg" hydrogen states have σγe ≅ 0.5x10^-20m2, whereas isolated electrons have Thompson cross-section σγe ≅ 0.7x10^-28m2. A 1D-radial average cross-section σγe ≅ 3x10^-24m2 will generate the observed solar wind, as "collisional runaway" protons accelerate out of the 2.keV gravity well and up to 1.3 keV kinetic energy within several Rs. This coherent proton/electron flow will glow as the K-Corona, obviating the traditional T=100eV hydrostatic models.
Analyzing spacecraft magnetic data from this perspective provides three insights into the fluctuating wind currents. 1) Variable-duration spectral analyses clearly show that there is no persistent magnetic "spiral" at 1AU, merely the integrated fluctuations of local currents. Similarly, spectral components B(f) above f~50.mHz clearly show the √N scaling of random noise. 2) Pervasive dynamical "arc" events are observed on time-scales 10^3< t < 10^5 sec, presumably related to spiky "switchbacks" observed by PSP at 0.1AU. The dynamics appears as Bθ-Bz, Br-Bz, and Br-Bθ temporal arcs, with occurrence rates differing by direction. The observed dynamics is closely modelled by finite-duration "pinched" +/- current filaments, representing fractional charge non-neutrality of 10^-5 over distances d~10^3Mm and times t~2000s. 3) The Br and Bθ (but not Bz) spectral components at the solar rotation frequency frot are quite exceptional, varying between 0% and 30% (average 17%) of the total Brms^2 magnetic energy. In only these variable components (with differing radial dependencies) is there a Br-Bθ anti-correlation, which is traditionally mis-interpreted as a persistent spiral. These frot components probably reflect variable z-currents, driven by θ- and z-dependent electric potentials from exceedingly small differences in e-/p+ ejection from the rotating solar surface.- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2020
- Bibcode:
- 2020AGUFMSH0290020D
- Keywords:
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- 2164 Solar wind plasma;
- INTERPLANETARY PHYSICS;
- 2169 Solar wind sources;
- INTERPLANETARY PHYSICS;
- 7509 Corona;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7524 Magnetic fields;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY