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Top: CUTE NUV 2D CCD spectra of Alpha Centauri ...

Top: CUTE NUV 2D CCD spectra of Alpha Centauri from a single 240 s exposure. The spectra...

Dolon Bhattacharyya et al, The Astronomical Journal 172 1

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The top panel presents the photosphere 1, chrom...

The top panel presents the photosphere 1, chromosphere, and photosphere 2 intensity vari...

Dolon Bhattacharyya et al, The Astronomical Journal 172 1

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Top: these panels present the Lomb–Scargle powe...

Top: these panels present the Lomb–Scargle power for different activity cycle power freq...

Dolon Bhattacharyya et al, The Astronomical Journal 172 1

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Top: these panels represent Lomb–Scargle power ...

Top: these panels represent Lomb–Scargle power for different rotation period power frequ...

Dolon Bhattacharyya et al, The Astronomical Journal 172 1

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The top panel presents the photosphere 1, chrom...

The top panel presents the photosphere 1, chromosphere, and photosphere 2 intensity vari...

Dolon Bhattacharyya et al, The Astronomical Journal 172 1

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The top panel compares a flaring spectrum vs. a...

The top panel compares a flaring spectrum vs. a normal spectrum of Alpha Centauri A as o...

Dolon Bhattacharyya et al, The Astronomical Journal 172 1

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This figure displays the orbital correction app...

This figure displays the orbital correction applied to CUTE’s recorded photosphere 1 int...

Dolon Bhattacharyya et al, The Astronomical Journal 172 1

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PIL extraction based on the RBF kernel SVC clas...

PIL extraction based on the RBF kernel SVC classification. (a) The HARD detection result...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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The flowchart of the HDBSCAN clustering applied...

The flowchart of the HDBSCAN clustering applied to solar magnetograms on 2023 February 1...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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An example shows the entire procedure of Predic...

An example shows the entire procedure of Prediction and Match for a specific active regi...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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Two line charts of the three tracking evaluatio...

Two line charts of the three tracking evaluation indicators, MOTA (blue), IDR (green), a...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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The thermogram of the different evaluation indi...

The thermogram of the different evaluation indicators changes depending on the parameter...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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An example of PIL-svc extraction on 2023 July 1...

An example of PIL-svc extraction on 2023 July 15. (a) The HARD detection results. Panels...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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Results of PIL-mask extraction using different ...

Results of PIL-mask extraction using different sigma and n_cluster parameters are presen...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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An example of tracking results. (a) The active ...

An example of tracking results. (a) The active regions detected by the HARD method on 20...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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The DSARD result for the SOHO/MDI magnetogram o...

The DSARD result for the SOHO/MDI magnetogram on 2000 May 20, with minDistance set to 20...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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HDBSCAN-based solar active region detection res...

HDBSCAN-based solar active region detection result of the SOHO/MDI magnetogram on 2000 M...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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Panel (a) is the result under the parameters in...

Panel (a) is the result under the parameters in Figure 1. Panel (b) is the result of set...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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Solar active region detection results of the SO...

Solar active region detection results of the SOHO/MDI magnetogram on 1999 August 1 (a), ...

C. X. Shi et al, The Astrophysical Journal Supplement Series 285 1

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Standard deviation of the line center of gravit...

Standard deviation of the line center of gravity as a function of RV-weighted line-forma...

V. Vasilyev et al, The Astrophysical Journal 1004 2

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Comparison of solar line sensitivities with tho...

Comparison of solar line sensitivities with those in the G9 and K4 models. Each point co...

V. Vasilyev et al, The Astrophysical Journal 1004 2

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Spatial maps of line strength and COG velocity ...

Spatial maps of line strength and COG velocity for a representative Fe II line at disk c...

V. Vasilyev et al, The Astrophysical Journal 1004 2

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Dependence of Fe I and Fe II line sensitivity t...

Dependence of Fe I and Fe II line sensitivity to granulation on effective temperature. E...

V. Vasilyev et al, The Astrophysical Journal 1004 2

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MURaM simulations used in the analysis. Top: ma...

MURaM simulations used in the analysis. Top: maps of vertical velocity Vz at the continu...

V. Vasilyev et al, The Astrophysical Journal 1004 2

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Spatial maps of line strength and COG velocity ...

Spatial maps of line strength and COG velocity for an Fe I line at disk center. The maps...

V. Vasilyev et al, The Astrophysical Journal 1004 2

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