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Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding the Physics of Solar Wind Acceleration
Ultraviolet Coronagraph Spectroscopy Physics of Solar Wind Acceleration
2010/11/15
Understanding the physical processes responsible for accelerating the solar wind requires detailed measurements of the collisionless plasma in the extended solar corona. Some key clues about these pro...
Evidence for a current sheet forming in the wake of a Coronal Mass Ejection from multi-viewpoint coronagraph observations
Solar and Stellar Astrophysics (astro-ph.SR)
2010/12/23
Ray-like features observed by coronagraphs in the wake of Coronal Mass Ejections (CMEs) are sometimes interpreted as the white light counterparts of current sheets (CSs) produced by the eruption.
Coronagraph feasibility studies on FRIDA。
Next Generation UV Coronagraph Instrumentation for Solar Cycle-24
Solar instrumentation solar spectroscopy solar corona solar wind coronal mass ejections
2009/5/6
Ultraviolet coronagraph observations of the extended solar
corona (defined here as 1.5 to 10 solar radii from Sun-center) have become a
powerful tool for obtaining detailed empirical descriptions o...