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Demonstrating the sensitivity of each parameter...

Demonstrating the sensitivity of each parameter on the CO fundamental band of Model P at...

T. Mera et al, The Astrophysical Journal 1003 2

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Left: the coordinate systems of (r, θ) and (p, ...

Left: the coordinate systems of (r, θ) and (p, z). rphoto is the photosphere, r1 and r1 ...

T. Mera et al, The Astrophysical Journal 1003 2

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Temperature structures from selected models fro...

Temperature structures from selected models from Tables 1 and 2 at days 285 (top) and 38...

T. Mera et al, The Astrophysical Journal 1003 2

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A schematic showing the iteration scheme used i...

A schematic showing the iteration scheme used in MOFAT. The outermost loop loops through...

T. Mera et al, The Astrophysical Journal 1003 2

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Demonstrating the χ2 convergence for each of th...

Demonstrating the χ2 convergence for each of the seven parameters for Model P at day 385...

T. Mera et al, The Astrophysical Journal 1003 2

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Same as Figure 6 except that we scale the absol...

Same as Figure 6 except that we scale the absolute flux of our model to minimize the tot...

T. Mera et al, The Astrophysical Journal 1003 2

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Same as Figure 4 but with the CO overtone band....

Same as Figure 4 but with the CO overtone band. Total mass (B) and temperature (C) influ...

T. Mera et al, The Astrophysical Journal 1003 2

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Demonstration of the sensitivity of each parame...

Demonstration of the sensitivity of each parameter to the SiO fundamental band of Model ...

T. Mera et al, The Astrophysical Journal 1003 2

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For given initial temperature structures of Mod...

For given initial temperature structures of Models P (left) and O (right, Figure 3) we s...

T. Mera et al, The Astrophysical Journal 1003 2

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Optical depth of Model P at day 385 for the loc...

Optical depth of Model P at day 385 for the local peaks of the vibrational modes of the ...

T. Mera et al, The Astrophysical Journal 1003 2

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Demonstrating how the strength of decoupling be...

Demonstrating how the strength of decoupling between Trot and Tvib can change the ratios...

T. Mera et al, The Astrophysical Journal 1003 2

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Optical depth of Model PP at day 385 for the lo...

Optical depth of Model PP at day 385 for the local peaks of the vibrational modes of the...

T. Mera et al, The Astrophysical Journal 1003 2

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Spectrum of Model P with and without clumping.

T. Mera et al, The Astrophysical Journal 1003 2

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Corner plot showing the distribution of paramet...

Corner plot showing the distribution of parameters for 105 samples drawn from a normaliz...

T. Mera et al, The Astrophysical Journal 1003 2

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Demonstration of the χ2 convergence for the fun...

Demonstration of the χ2 convergence for the fundamental band for each of the six primary...

T. Mera et al, The Astrophysical Journal 1003 2

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Same as Figure 14 except that we scale the abso...

Same as Figure 14 except that we scale the absolute flux of our model to minimize the to...

T. Mera et al, The Astrophysical Journal 1003 2

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Solar radio dynamic spectrum of the 2024 May 5 ...

Solar radio dynamic spectrum of the 2024 May 5 event observed by CBSm. (a) Overview of t...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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Same as Figure 1, but for the 2024 May 8 event....

Same as Figure 1, but for the 2024 May 8 event. A zoomed-in view of the white box is sho...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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SDO observations and magnetic field modeling of...

SDO observations and magnetic field modeling of the 2024 May 9 event, along with schemat...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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Model setup and Z-mode (UH) wave analysis. (a) ...

Model setup and Z-mode (UH) wave analysis. (a) Temporal evolution of the plasma density ...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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DART radio images and simultaneous HMI line-of-...

DART radio images and simultaneous HMI line-of-sight magnetograms of the ARs associated ...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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Solar radio dynamic spectrum of the 2024 May 9 ...

Solar radio dynamic spectrum of the 2024 May 9 event observed by CBSm. (a) Zoomed-in vie...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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Same as Figure 1, but for the 2025 October 13 e...

Same as Figure 1, but for the 2025 October 13 event. The black dashed line and plus sign...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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(a) Maximum growth rate of the UH mode as a fun...

(a) Maximum growth rate of the UH mode as a function of ωpe/Ωce (t). (b) Corresponding r...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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UH mode growth rates and radiation spectra unde...

UH mode growth rates and radiation spectra under three cases: no modulation (left column...

Chuanyang Li et al, The Astrophysical Journal 1003 2

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