On extracting plasma compression signatures from white light coronal images

14th Annual International Astrophysics Conference: Linear and Nonlinear Particle Energization throughout the Heliosphere and Beyond

物理学;天文学

Roelof, E.C.^1 ; Vourlidas, A.^1

Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd., Laurel

MD

20723, United States^1

关键词: Acceleration rates;    Coronal mass ejection;    Density features;    Empirical formulas;    Generalized mean value;    Plasma compression;    Plasma velocity;    Solar energetic particles;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/642/1/012024/pdf
DOI  :  10.1088/1742-6596/642/1/012024

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

We offer the intriguing possibility that the divergence of the plasma velocity (∇•V) in outward-moving density features can be extracted directly from coronal and heliospheric white-light images of coronal mass ejections (CMEs). The relevant empirical formula is quite simple to apply. It follows directly from the conservation of electrons. We derive an approximate relation between the measured white-light intensities in the brightest image pixels and the dominant electron densities along the pixel line of sight by invoking the generalized mean value theorem for integrals. If the formula holds with acceptable accuracy, we then may have a measure of not only (∇•V) itself, but also the related compressive acceleration rate of solar energetic particles within the CME.