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(a)–(d) An example of a bow-shock crossing even...

(a)–(d) An example of a bow-shock crossing event around 21:34 UT on 1998 October 25: omn...

Xinnian Guo et al, The Astrophysical Journal Letters 1006 2

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(a)–(c) Histograms of Jab (a), Jsh (b), and Jsh...

(a)–(c) Histograms of Jab (a), Jsh (b), and Jsh/Jab (c) for Group A (purple), B (yellow–...

Xinnian Guo et al, The Astrophysical Journal Letters 1006 2

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(a) Histograms of Edrift for UDPL (pink), SPL (...

(a) Histograms of Edrift for UDPL (pink), SPL (light blue), DDPL (dark blue), and ER (or...

Xinnian Guo et al, The Astrophysical Journal Letters 1006 2

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(a) Scatter plot of Jsh/Jab versus rB for spect...

(a) Scatter plot of Jsh/Jab versus rB for spectral types in path #1 (black), path #2 (re...

Xinnian Guo et al, The Astrophysical Journal Letters 1006 2

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Spatial distribution of bow-shock crossings pro...

Spatial distribution of bow-shock crossings projected onto the GSE x–y-plane, color-code...

Xinnian Guo et al, The Astrophysical Journal Letters 1006 2

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Cosmic star formation history. The blue stars r...

Cosmic star formation history. The blue stars represent our estimates from Swift LGRBs, ...

Jing-Meng Hao et al, The Astrophysical Journal Letters 1006 2

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Hydrogen reionization history. Left panel: the ...

Hydrogen reionization history. Left panel: the predictions of the timeline of the neutra...

Jing-Meng Hao et al, The Astrophysical Journal Letters 1006 2

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The luminosity-redshift distribution of Swift L...

The luminosity-redshift distribution of Swift LGRBs. The gray shaded region represents a...

Jing-Meng Hao et al, The Astrophysical Journal Letters 1006 2

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Predictions of the Thomson scattering optical d...

Predictions of the Thomson scattering optical depth. The gray line and region represent ...

Jing-Meng Hao et al, The Astrophysical Journal Letters 1006 2

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Evolution of the observable fraction of star fo...

Evolution of the observable fraction of star formation, ...

Jing-Meng Hao et al, The Astrophysical Journal Letters 1006 2

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Prediction of solar cycle evolution. Panel (a) ...

Prediction of solar cycle evolution. Panel (a) shows the evolution of the polar field, w...

Zi-Fan Wang et al, The Astrophysical Journal Letters 1006 2

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Stack plot displaying ARs during CRs 2275–2285....

Stack plot displaying ARs during CRs 2275–2285. Each tile is obtained from the synoptic ...

Zi-Fan Wang et al, The Astrophysical Journal Letters 1006 2

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SFT simulation of the ARs in the northern hemis...

SFT simulation of the ARs in the northern hemisphere during CRs 2275–2285. Panel (a) sho...

Zi-Fan Wang et al, The Astrophysical Journal Letters 1006 2

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Observational large-scale magnetic field evolut...

Observational large-scale magnetic field evolution of the Sun during cycle 25. Panel (a)...

Zi-Fan Wang et al, The Astrophysical Journal Letters 1006 2

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Statistical properties of AR emergence predicti...

Statistical properties of AR emergence prediction and one example of random realizations...

Zi-Fan Wang et al, The Astrophysical Journal Letters 1006 2

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P200/DBSP spectroscopy of HSC J0233−0205. The r...

P200/DBSP spectroscopy of HSC J0233−0205. The right panels show the HSC color image of t...

Zizhao He et al, The Astrophysical Journal Letters 1006 2

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Best-fitting five-band HSC lens-modeling result...

Best-fitting five-band HSC lens-modeling results. Columns show the data, lens-light mode...

Zizhao He et al, The Astrophysical Journal Letters 1006 2

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CIGALE SED fitting results for the two lens gal...

CIGALE SED fitting results for the two lens galaxies. The black curves show the best-fit...

Zizhao He et al, The Astrophysical Journal Letters 1006 2

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Deflector redshift versus lens–lens angular sep...

Deflector redshift versus lens–lens angular separation for HSC J0233−0205 and a literatu...

Zizhao He et al, The Astrophysical Journal Letters 1006 2

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Left panel: the γ-ray flux from within a 6° rad...

Left panel: the γ-ray flux from within a 6° radius emission region for Iroshnikov–Kraich...

Zhaodong Shi et al, The Astrophysical Journal Letters 1006 2

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The γ-ray flux from within a 6° radius emission...

The γ-ray flux from within a 6° radius emission region for Iroshnikov–Kraichnan turbulen...

Zhaodong Shi et al, The Astrophysical Journal Letters 1006 2

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Same as Figure 1, but the right panel displays ...

Same as Figure 1, but the right panel displays the azimuthally averaged integrated γ-ray...

Zhaodong Shi et al, The Astrophysical Journal Letters 1006 2

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Same as the right panel of Figure 1, but the ga...

Same as the right panel of Figure 1, but the gas density is given as shown in the inset ...

Zhaodong Shi et al, The Astrophysical Journal Letters 1006 2

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Electron energy distribution at ﹩r=100﹩ km as c...

Electron energy distribution at ﹩r=100﹩ km as calculated with ...

Erik Vigren and Anders I. Eriksson, The Astronomical Journal 172 2

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Modeled fraction of hot electrons at the locati...

Modeled fraction of hot electrons at the location of Rosetta versus date. The data is he...

Erik Vigren and Anders I. Eriksson, The Astronomical Journal 172 2

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