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An example (HARP 5983 on 2015 September 30 at 0...

An example (HARP 5983 on 2015 September 30 at 03:00:00 UT) illustrating different mask t...

Z. Zheng et al, The Astrophysical Journal Letters 1008 1

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Examples of active regions. (a) HARP 5983 on 20...

Examples of active regions. (a) HARP 5983 on 2015 September 30 at 03:00:00 TAI. (b) HARP...

Z. Zheng et al, The Astrophysical Journal Letters 1008 1

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The flowchart of this study. It involves: (1) t...

The flowchart of this study. It involves: (1) training a CNN-based flare prediction mode...

Z. Zheng et al, The Astrophysical Journal Letters 1008 1

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The joint (center) and univariate (top and righ...

The joint (center) and univariate (top and right) distributions of the Polarity Imbalanc...

Z. Zheng et al, The Astrophysical Journal Letters 1008 1

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Schematic representation of the CNN model used ...

Schematic representation of the CNN model used in this work. Four-channel magnetic field...

Z. Zheng et al, The Astrophysical Journal Letters 1008 1

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The flowchart of the data splitting.

The flowchart of the data splitting.

Z. Zheng et al, The Astrophysical Journal Letters 1008 1

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Distribution of the alpha-to-proton temperature...

Distribution of the alpha-to-proton temperature ratio (Tα/Tp) in different solar wind sp...

Aakash Gupta et al, The Astrophysical Journal Letters 1008 1

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Solar cycle evolution of the ratio between the ...

Solar cycle evolution of the ratio between the mass-proportional and equal-temperature p...

Aakash Gupta et al, The Astrophysical Journal Letters 1008 1

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This figure shows the variation of the temperat...

This figure shows the variation of the temperature ratio Tα/Tp as a function of the Coul...

Aakash Gupta et al, The Astrophysical Journal Letters 1008 1

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Solar cycle modulation of solar wind collisiona...

Solar cycle modulation of solar wind collisionality and mass-proportional alpha particle...

Aakash Gupta et al, The Astrophysical Journal Letters 1008 1

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A 2D projection of the magnitude of an isotropi...

A 2D projection of the magnitude of an isotropic turbulent magnetic field as constructed...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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The dependence of the parallel and perpendicula...

The dependence of the parallel and perpendicular MFPs (left and middle columns, respecti...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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The running parallel MFP for a purely compressi...

The running parallel MFP for a purely compressive field is shown in the left panel. Pres...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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The magnitude of a high-resolution transverse 2...

The magnitude of a high-resolution transverse 2D field as might be used in the AC model,...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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Omnidirectional spectral forms measured from co...

Omnidirectional spectral forms measured from code output for turbulent magnetic fields w...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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2D projections of a transversally enhanced (Z =...

2D projections of a transversally enhanced (Z = 25%) turbulent field magnitude with the ...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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Magnitude projections of a turbulent field with...

Magnitude projections of a turbulent field with an isotropic component as depicted in Fi...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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Perpendicular MFPs computed in the case of ...

Perpendicular MFPs computed in the case of ﹩{(\delta {B}_{z}/\delta B)}^{2}=100 \% ﹩, as...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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The same energy-dependent MFPs as shown in Figu...

The same energy-dependent MFPs as shown in Figure 8, but for the AC model introduced in ...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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The variation of MFPs with the compressibility ...

The variation of MFPs with the compressibility ﹩{(\delta {B}_{z}/\delta B)}^{2}﹩. Left, ...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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The MFPs as a function of compressibility, as s...

The MFPs as a function of compressibility, as shown in Figure 10, but for the AC field d...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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Left panel: sample trajectories computed over t...

Left panel: sample trajectories computed over the duration of one simulation for 70 MeV ...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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The ratios of the parallel (left panel) and per...

The ratios of the parallel (left panel) and perpendicular (right panel) MFPs computed fo...

J. S. Troskie and N. E. Engelbrecht, The Astrophysical Journal Supplement Series 286 1

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Left: an illustration showing the SDO AIA 131 Å...

Left: an illustration showing the SDO AIA 131 Å view, from the direction of Earth, at 06...

Samuel Carter et al, The Astrophysical Journal Supplement Series 286 1

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Fluence spectra, shown without FAF on the left ...

Fluence spectra, shown without FAF on the left and with FAF on the right. Panels (a) and...

Samuel Carter et al, The Astrophysical Journal Supplement Series 286 1

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