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Published on: July 27, 2018
Spectropolarimetric analysis of waves linked to first ionization potential
Mariarita Murabito1, Marco Stangalini2
1INAF-Osservatorio Astronomico di Roma , Via Frascati 33, I-00078 Monteporzio Catone, Italy.
High-resolution spectropolarimetry reveals how chromospheric waves influence coronal plasma composition. New research explores Stokes-V amplitude asymmetries as a tool to study wave behavior linked to solar atmospheric abundances.
Area of Science:
- Solar physics
- Plasma astrophysics
- Spectropolarimetry
Background:
- Chromospheric waves are crucial for shaping coronal plasma composition.
- Ponderomotive force from Alfvénic perturbations is a key factor.
- Spectropolarimetric studies link chromospheric waves to enhanced First Ionization Potential (FIP) bias in the corona.
Purpose of the Study:
- Investigate Stokes-V amplitude asymmetries as a novel diagnostic tool.
- Explore wave behavior relevant to solar compositional fractionation processes.
- Enhance understanding of solar atmospheric abundances.
Main Methods:
- Utilizing high-resolution spectropolarimetry measurements.
- Analyzing Stokes-V amplitude asymmetries.
- Connecting chromospheric wave activity to coronal composition.
Main Results:
- Stokes-V amplitude asymmetries show potential as a diagnostic tool.
- Wave behavior can be investigated through these asymmetries.
- This method offers insights into compositional fractionation.
Conclusions:
- Stokes-V amplitude asymmetries provide an alternative diagnostic for chromospheric waves.
- This technique aids in understanding solar atmospheric composition and FIP bias.
- Further research can refine this method for solar abundance studies.
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