KnowraSolar coronaLinked fromLinked fromThe 23 pages that link to Solar corona, each with the reason it gives.All 23Broader topic 10Related 9Narrower topic 2Compared with 2Solar eclipseRelated: Totality briefly makes the corona visible against the darkened sky.Solar magnetic fieldRelated: The corona’s shape and heating are strongly governed by magnetic structure.HeliosphereRelated: The solar wind flows outward from the corona.Alfvén waveRelated: Alfvén-wave energy is a proposed contributor to coronal heating and solar-wind acceleration.Thomson scatteringRelated: Free coronal electrons scatter sunlight, producing the corona's white-light component.ChromosphereRelated: The corona begins above the chromosphere, with the transition region between them.Anton PannekoekRelated: Pannekoek investigated the corona’s brightness and structure through eclipse observations.Interplanetary mediumRelated: The corona continuously supplies particles that escape as the solar wind.Kreutz sungrazerRelated: Bright Kreutz comets can pass through the corona's hot, tenuous plasma.