Measurements of electron anisotropy in solar flares using albedo with RHESSI X-ray data
arXiv:1210.4757 · doi:10.1007/s11207-012-0178-3
Abstract
The angular distribution of electrons accelerated in solar flares is a key parameter in the understanding of the acceleration and propagation mechanisms that occur there. However, the anisotropy of energetic electrons is still a poorly known quantity, with observational studies producing evidence for an isotropic distribution and theoretical models mainly considering the strongly beamed case. We use the effect of photospheric albedo to infer the pitch angle distribution of X-ray emitting electrons using Hard X-ray data from RHESSI. A bi-directional approximation is applied and a regularized inversion is performed for eight large flare events to deduce the electron spectra in both downward (towards the photosphere) and upward (away from the photosphere) directions. The electron spectra and the electron anisotropy ratios are calculated for broad energy range from about 10 and up to ~ 300 keV near the peak of the flares. The variation of electron anisotropy over short periods of time intervals lasting 4, 8 and 16 seconds near the impulsive peak has been examined. The results show little evidence for strong anisotropy and the mean electron flux spectra are consistent with the isotropic electron distribution. The 3-sigma level uncertainties, although energy and event dependent, are found to suggest that anisotropic distribution with anisotropy larger than ~ 3 are not consistent with the hard X-ray data. At energies above 150-200 keV, the uncertainties are larger and thus the possible electron anisotropies could be larger.
arXiv comment24 pages, 14 figures, Accepted for publication in Solar Physics
References in corpus (11)
- Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares
- Deducing Electron Properties From Hard X-Ray Observations
- Compton backscattered and primary X-rays from solar flares: angle dependent Green's function correction for photospheric albedo
- Stereoscopic electron spectroscopy of solar hard X-ray flares with a single spacecraft
- Hard X-ray Spectra and Positions of Solar Flares observed by RHESSI: photospheric albedo, directivity and electron spectra
- Generalized Regularization Techniques With Constraints For The Analysis Of Solar Bremsstrahlung X-Ray Spectra
- RHESSI as a Hard X-Ray Polarimeter
- Determination Of Electron Flux Spectra In A Solar Flare With An Augmented Regularization Method: Application To Rhessi Data
- X-Ray Polarization of Solar Flares Measured with Rhessi
- Low-energy cutoffs in electron spectra of solar flares: statistical survey
- Spatially resolved hard X-ray polarization in solar flares: effects of Compton scattering and bremsstrahlung
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