Results 141 to 150 of about 10,729 (219)

Long-term evolution of solar coronal holes

open access: yes, 2020
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.
openaire   +1 more source

Quality Assessment of Solar EUV Remote Sensing Images Using Multi-Feature Fusion. [PDF]

open access: yesSensors (Basel)
Dai S   +8 more
europepmc   +1 more source

Exploring the extremes: The cosmic laboratory. [PDF]

open access: yesInnovation (Camb)
Huang Y, He S, Ge L, Li Z, Mao Y, Liu J.
europepmc   +1 more source

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]

open access: yesLiving Rev Sol Phys
Veronig AM   +12 more
europepmc   +1 more source

Solar coronal holes and their geo-effectiveness

open access: yesJournal of Physics: Conference Series, 2019
Santi Sulistiani, Dhani Herdiwijaya
openaire   +1 more source

A tidal disruption event from an intermediate-mass black hole revealed by comprehensive multi-wavelength observations. [PDF]

open access: yesNat Commun
Wang J   +14 more
europepmc   +1 more source

The Amerigo Vespucci as a traveling laboratory for studying the cosmic-ray fluxes at sea level. [PDF]

open access: yesSci Rep
Cerasole D   +15 more
europepmc   +1 more source

Complexity analyses of geomagnetic and solar activity indices time series. [PDF]

open access: yesSci Rep
Javaherian M   +4 more
europepmc   +1 more source

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