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- In 1966, he was awarded the Eddington Medal by the Royal Astronomical Society for his "discovery of the importance of negative hydrogen ions as a contributor to the solar atmosphere's opacity".
- The ambitious Solar Orbiter Mission, based on a suggestion from the institute, will see a probe approach our star to within a fifth of the Earth-Sun distance in order to investigate the magnetic field and its effects in the various layers of the solar atmosphere.
- The radio bursts are associated with solar flare plasma that interacts with the ambient solar atmosphere.
- The turbulent behavior of the outer solar atmosphere soon became the primary subject of research at the Einstein Tower.
- The Rapid Oscillations in the Solar Atmosphere (ROSA) instrument is a single-controlled system of 6 imaging fast-readout CCD cameras.
- Water vapor is a relatively common atmospheric constituent, present even in the solar atmosphere as well as every planet in the Solar System and many astronomical objects including natural satellites, comets and even large asteroids.
- The MLSO is tasked with monitoring the solar atmosphere and recording data on plasmic and energetic emissions from the chromosphere and corona.
- period) were detected in the solar atmosphere (at temperatures typical of the transition region and corona) by TRACE.
- The first Stratoscope produced high resolution images of solar granules and sunspots, confirming the existence of convection in the solar atmosphere, and the second obtained infrared spectra of planets, red giant stars, and the nuclei of galaxies.
- The plasma source is small magnetic fields created by convection cells in the solar atmosphere.
- It also produces data to enable estimates of the coronal magnetic field for studies of variability in the extended solar atmosphere.
- Prior to 1983, it was thought that the whole Sun has the same composition as the solar atmosphere.
- It was correctly deduced that dark lines in the solar spectrum are caused by absorption by chemical elements in the solar atmosphere.
- It was correctly deduced that dark lines in the solar spectrum are caused by absorption by chemical elements in the solar atmosphere.
- They are very complex phenomena, visible at different wavelengths; they involve several zones of the solar atmosphere and many physical effects, thermal and not thermal, and sometimes wide reconnections of the magnetic field lines with material expulsion.
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Contains translations by TU Chemnitz and Mr Honey's Business Dictionary (German-English only).
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