Many phenomena taking place in the solar photosphere are controlled by plasma motions. Although the line-of-sight component of the velocity can be estimated using the Doppler effect, we do not have direct spectroscopic access to the components that are perpendicular to the line of sight. These components are typically estimated using methods based on local correlation tracking. We have designed DeepVe
Abstract The application of machine learning in solar physics has the potential to greatly enhance o...
Context. Flows on the solar surface are intimately linked to solar activity, and local correlation t...
The volume of data being collected in solar physics has exponentially increased over the past decade...
Many phenomena taking place in the solar photosphere are controlled by plasma motions. Although the ...
Direct measurements of plasma motions are limited to the line-of-sight component at the Sun's surfac...
Coverage of plasma motions is limited to the line-of-sight component at the Sun’s surface. Multiple ...
Context. The dynamics in the photosphere is governed by the multi-scale turbulent convection termed ...
We propose a useful method for mapping large-scale velocity fields in the solar photosphere. It is b...
Context. The measurement of Doppler velocities in spectroscopic solar observations requires a refere...
We propose a useful method for mapping large-scale velocity fields in the solar photosphere. It is b...
Emanating from the base of the Sun’s corona, the solar wind fills the interplanetary medium with a m...
In the recent decades, the difficult task of understanding and predicting violent solar eruptions an...
The Sunyaev–Zel’dolvich (SZ) effect is expected to be instrumental in measuring velocities of distan...
Obtaining high-quality magnetic and velocity fields through Stokes inversion is crucial in solar phy...
Large-scale velocity fields in the solar photosphere remain a mystery in spite of many years of inte...
Abstract The application of machine learning in solar physics has the potential to greatly enhance o...
Context. Flows on the solar surface are intimately linked to solar activity, and local correlation t...
The volume of data being collected in solar physics has exponentially increased over the past decade...
Many phenomena taking place in the solar photosphere are controlled by plasma motions. Although the ...
Direct measurements of plasma motions are limited to the line-of-sight component at the Sun's surfac...
Coverage of plasma motions is limited to the line-of-sight component at the Sun’s surface. Multiple ...
Context. The dynamics in the photosphere is governed by the multi-scale turbulent convection termed ...
We propose a useful method for mapping large-scale velocity fields in the solar photosphere. It is b...
Context. The measurement of Doppler velocities in spectroscopic solar observations requires a refere...
We propose a useful method for mapping large-scale velocity fields in the solar photosphere. It is b...
Emanating from the base of the Sun’s corona, the solar wind fills the interplanetary medium with a m...
In the recent decades, the difficult task of understanding and predicting violent solar eruptions an...
The Sunyaev–Zel’dolvich (SZ) effect is expected to be instrumental in measuring velocities of distan...
Obtaining high-quality magnetic and velocity fields through Stokes inversion is crucial in solar phy...
Large-scale velocity fields in the solar photosphere remain a mystery in spite of many years of inte...
Abstract The application of machine learning in solar physics has the potential to greatly enhance o...
Context. Flows on the solar surface are intimately linked to solar activity, and local correlation t...
The volume of data being collected in solar physics has exponentially increased over the past decade...