Long-term evolution of solar coronal holes
Abstract Solar coronal holes are regions of open magnetic field lines in the solar corona. They are the source region of high-speed solar wind streams that play an important role for geomagnetic activity and are the most important driver of energetic particle precipitation into the Earth’s atmosphere.
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Quality Assessment of Solar EUV Remote Sensing Images Using Multi-Feature Fusion. [PDF]
Dai S +8 more
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Quantifying the Consistency and Characterizing the Confidence of Coronal Holes Detected by Active Contours Without Edges (ACWE). [PDF]
Grajeda JA +4 more
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Exploring the extremes: The cosmic laboratory. [PDF]
Huang Y, He S, Ge L, Li Z, Mao Y, Liu J.
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Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
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Solar coronal holes and their geo-effectiveness
Santi Sulistiani, Dhani Herdiwijaya
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A tidal disruption event from an intermediate-mass black hole revealed by comprehensive multi-wavelength observations. [PDF]
Wang J +14 more
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The Amerigo Vespucci as a traveling laboratory for studying the cosmic-ray fluxes at sea level. [PDF]
Cerasole D +15 more
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Complexity analyses of geomagnetic and solar activity indices time series. [PDF]
Javaherian M +4 more
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Comparing and Contrasting the Properties of the Inner Heliosphere for the Three Most Recent Solar Minima. [PDF]
Riley P +4 more
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