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The dominant large-scale variations in the sola...
Beginning in late 2018 through early 2023, an e...
The solar wind speed gradually decreases with i...
Few missions have collected solar wind measurem...
Slower wind was observed at 1 au within the cor...
When comparing solar rotation–averaged speeds i...
The long slow wind interval observed by NH in t...
Simulation results reproduce the large-scale fe...
Comparison of the predicted core density–radius...
Diversity of rotation curves predicted from FIP...
The effect of baryons in the inner core is negl...
Halo density profiles normalized by the central...
Schematic illustration of the proposed structur...
Effects of baryons on the DM outer core. Note t...
Relation between the planetary magnetosphere si...
Same relation as Figure 3, but for the E. N. Pa...
Velocity profiles of the HBC359 star considerin...
Ratio of X-ray to bolometric luminosity log(LX⋆...
Comparison between the planetary magnetospheric...
Upper panel: Ca II H and K line luminosities vs...
Statistical relationships between solar wind pa...
Orbit-by-orbit variations of solar wind paramet...
Orbit-by-orbit variations of solar wind paramet...
Orbit-by-orbit variations of solar wind paramet...
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