R. Casini
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View article: DKIST resolves sub-arcsec photospheric scattering polarization
DKIST resolves sub-arcsec photospheric scattering polarization Open
Scattering polarization signals offer unique diagnostics of the physical conditions in the solar atmosphere, in particular magnetic fields via the Hanle effect. However, their spatial structure remains poorly constrained due to the difficu…
View article: Using the Hanle Effect in Mg <scp>ii</scp> k to Quantify the Open Flux above the Solar Poles
Using the Hanle Effect in Mg <span>ii</span> k to Quantify the Open Flux above the Solar Poles Open
We test the use of the Mg ii resonant lines for measurement of the magnetic field at the top of the chromosphere of polar coronal holes (CHs). The Hanle effect in the core of Mg II k enables access to a regime of field strengths where the …
View article: Metasurface-Enabled Astronomical Polarimetry
Metasurface-Enabled Astronomical Polarimetry Open
In the last decade or so, metasurface optical components have received considerable scientific and industrial interest for a variety of applications. The miniaturization afforded by metasurfaces could benefit astronomy in particular (which…
View article: Image Instabilities and Polarization Crosstalk
Image Instabilities and Polarization Crosstalk Open
We expand on our previous study of the impact of atmospheric seeing on polarization crosstalk, and show how the formalism that was developed in that work can be applied to treat the case of spatial modulators of polarization. Beside formal…
View article: Detection of ``diffuse'' coronal He I1083 during the April 8 2024 Solar Eclipse: evidence for terrestrial atmospheric scattering contribution
Detection of ``diffuse'' coronal He I1083 during the April 8 2024 Solar Eclipse: evidence for terrestrial atmospheric scattering contribution Open
Strong He I 1083 nm atomic line signals have previously been measured during total solar eclipses at coronal heights above the lunar limb. Theserather unexpected measurements have kindled a discussion about the suggested presence of signif…
View article: Spectropolarimetry for Discerning Geometry and Structure in Circumstellar Media of Hot Massive Stars
Spectropolarimetry for Discerning Geometry and Structure in Circumstellar Media of Hot Massive Stars Open
Spectropolarimetric techniques are a mainstay of astrophysical inquiry, ranging from Solar System objects to the Cosmic Background Radiation. This review highlights applications of stellar polarimetry for massive hot stars, particularly in…
View article: Spectropolarimetry for Discerning Geometry and Structure in Circumstellar Media of Hot Massive Stars
Spectropolarimetry for Discerning Geometry and Structure in Circumstellar Media of Hot Massive Stars Open
Spectropolarimetric techniques are a mainstay of astrophysical inquiry, ranging from Solar System objects to the Cosmic Background Radiation. This review highlights applications of stellar polarimetry for massive hot stars, particularly in…
View article: A Unifying Polarization Formalism for Electric and Magnetic Multipole Interactions
A Unifying Polarization Formalism for Electric and Magnetic Multipole Interactions Open
We extend the spherical tensorial formalism for polarization to the treatment of electric and magnetic multipole transitions of any order. We rely on the spherical-wave expansion to derive the tensor form of the operator describing the int…
View article: Detection of "diffuse" coronal He I 1083 during the April 8 2024 Solar Eclipse: evidence for terrestrial atmospheric scattering origin
Detection of "diffuse" coronal He I 1083 during the April 8 2024 Solar Eclipse: evidence for terrestrial atmospheric scattering origin Open
Strong He I 1083 nm atomic line signals have been previously measured during total solar eclipses at coronal heights above the lunar limb. This rather unexpected measurement has kindled a discussion about the hypothesized presence of signi…
View article: Magnetic Diagnostics of Prominence Eruptions through the Hanle Effect of the He i 1083 nm Line
Magnetic Diagnostics of Prominence Eruptions through the Hanle Effect of the He i 1083 nm Line Open
The magnetic field vector of the solar corona is not regularly and comprehensively being measured because of the complexity and degeneracy inherently present in the types of observations currently available. To address some of the current …
View article: Magnetic diagnostics of prominence eruptions through the Hanle effect of the He I 1083 nm line
Magnetic diagnostics of prominence eruptions through the Hanle effect of the He I 1083 nm line Open
The magnetic field vector of the solar corona is not regularly and comprehensively being measured, because of the complexity and degeneracy inherently present in the types of observations currently available. To address some of the current…
View article: Magnetic diffusion in solar atmosphere produces measurable electric fields
Magnetic diffusion in solar atmosphere produces measurable electric fields Open
View article: Erratum: “Analysis of Seeing-induced Polarization Cross-talk and Modulation Scheme Performance” (2012, ApJ, 757, 45)
Erratum: “Analysis of Seeing-induced Polarization Cross-talk and Modulation Scheme Performance” (2012, ApJ, 757, 45) Open
View article: Extreme-ultraviolet Polarimetric Diagnostics of the Solar Corona: The Hanle Effect of Ne viii 770 Å
Extreme-ultraviolet Polarimetric Diagnostics of the Solar Corona: The Hanle Effect of Ne viii 770 Å Open
Magnetic fields are the primary driver of the plasma thermodynamics in the upper solar atmosphere, especially in the corona. However, magnetic field measurements in the solar corona are sporadic, thereby limiting us from the complete under…
View article: EUV polarimetric diagnostics of the solar corona: the Hanle effect of Ne VIII 770 Å
EUV polarimetric diagnostics of the solar corona: the Hanle effect of Ne VIII 770 Å Open
Magnetic fields are the primary driver of the plasma thermodynamics in the upper solar atmosphere, especially in the corona. However, magnetic field measurements in the solar corona are sporadic, thereby limiting us from the complete under…
View article: Magnetic Fields and Plasma Heating in the Sun’s Atmosphere
Magnetic Fields and Plasma Heating in the Sun’s Atmosphere Open
We use the first publicly available data from the Daniel K. Inouye Solar Telescope to track magnetic connections from the solar photosphere into the corona. We scrutinize relationships between chromospheric magnetism and bright chromospher…
View article: Magnetic fields and plasma heating in the Sun's atmosphere
Magnetic fields and plasma heating in the Sun's atmosphere Open
We use the first publically available data from the Daniel K. Inouye Solar Telescope (DKIST) to track magnetic connections from the solar photosphere into the corona. We scrutinize relationships between chromospheric magnetism and bright c…
View article: Coronal Polarimetry: Determining the Magnetic Origins of Coronal Mass Ejections
Coronal Polarimetry: Determining the Magnetic Origins of Coronal Mass Ejections Open
Whitepaper #127 in the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033. Main topics: basic research. Additional topics: ground-based missions/projects; solar physics; space-based missions/projects; user-need-driven basi…
View article: COSMO ChroMag: The Chromosphere and Prominence Magnetometer
COSMO ChroMag: The Chromosphere and Prominence Magnetometer Open
Whitepaper #088 in the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033. Main topics: space weather applications; basic research. Additional topics: space weather research/operations/research loop; space weather research…
View article: COMPLETE: a flagship mission for complete understanding of 3D coronal magnetic energy release
COMPLETE: a flagship mission for complete understanding of 3D coronal magnetic energy release Open
COMPLETE is a flagship mission concept combining broadband spectroscopic\nimaging and comprehensive magnetography from multiple viewpoints around the Sun\nto enable tomographic reconstruction of 3D coronal magnetic fields and\nassociated d…
View article: COSMO: The COronal Solar Magnetism Observatory
COSMO: The COronal Solar Magnetism Observatory Open
Whitepaper #392 in the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033. Main topics: space weather applications; infrastructure/workforce/other programmatic. Additional topics: space weather research/applications/operat…
View article: Solar Coronal Polarization Diagnostics with H I Ly-α
Solar Coronal Polarization Diagnostics with H I Ly-α Open
Whitepaper #047 in the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033. Main topics: basic research. Additional topics: solar physics; space-based missions/projects; user-need-driven basic space weather research.
View article: Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release
Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release Open
Synopsis The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poorly observed and understood. We highlight key ques…
View article: Improving Multi-Dimensional Data Formats, Access, and Assimilation Tools for the Twenty-First Century
Improving Multi-Dimensional Data Formats, Access, and Assimilation Tools for the Twenty-First Century Open
Heliophysics image data largely relies on a forty-year-old ecosystem built on\nthe venerable Flexible Image Transport System (FITS) data standard. While many\nin situ measurements use newer standards, they are difficult to integrate with\n…
View article: First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP: The Anatomy of an Umbral Flash
First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP: The Anatomy of an Umbral Flash Open
The Visible Spectro-Polarimeter (ViSP) of the NSF Daniel K. Inouye Solar Telescope (DKIST) collected its Science Verification data on May 7-8, 2021. The instrument observed multiple layers of a sunspot atmosphere simultaneously, in passban…
View article: First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP: The Anatomy of an Umbral Flash
First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP: The Anatomy of an Umbral Flash Open
The Visible Spectro-Polarimeter of the NSF Daniel K. Inouye Solar Telescope collected its Science Verification data on 2021 May 7–8. The instrument observed multiple layers of a sunspot atmosphere simultaneously, in passbands of Ca ii 397 …
View article: Systems Approach to Polarization Calibration for the Daniel K. Inouye Solar Telescope (DKIST)
Systems Approach to Polarization Calibration for the Daniel K. Inouye Solar Telescope (DKIST) Open
The Daniel K. Inouye Solar Telescope (DKIST) advances studies of solar magnetism through high-precision and accuracy in polarimetry at frontier spatial and temporal scales. A system model for polarization response in azimuth and altitude h…
View article: Ultraviolet spectropolarimetry with Polstar: using Polstar to test magnetospheric mass-loss quenching
Ultraviolet spectropolarimetry with Polstar: using Polstar to test magnetospheric mass-loss quenching Open
View article: Optimal Spectral Lines for Measuring Chromospheric Magnetic Fields
Optimal Spectral Lines for Measuring Chromospheric Magnetic Fields Open
This paper identifies spectral lines from X-ray to IR wavelengths which are optimally suited to measuring vector magnetic fields as high as possible in the solar atmosphere. Instrumental and Earth's atmospheric properties, as well as solar…
View article: Ultraviolet spectropolarimetry: investigating stellar magnetic field diagnostics
Ultraviolet spectropolarimetry: investigating stellar magnetic field diagnostics Open