• Corpus ID: 222412634

Über das Fraunhofersche Spektrum der Sonnenkorona. Mit 10 Abbildungen.

@inproceedings{Grotrian1934berDF,
  title={{\"U}ber das Fraunhofersche Spektrum der Sonnenkorona. Mit 10 Abbildungen.},
  author={Walter Grotrian},
  year={1934}
}
The First Empirical Determination of the Fe10+ and Fe13+ Freeze-in Distances in the Solar Corona
Heavy ions are markers of the physical processes responsible for the density and temperature distribution throughout the fine-scale magnetic structures that define the shape of the solar corona. One
The response of the corona to different spatial distributions of heat input
Explaining the existence of the million degree corona on top of the much cooler Solar surface has provided scientist with a challenge for a several decades. It is not possible for a cooler object to
Multi-Scale Variability of Coronal Loops Set by Thermal Non-Equilibrium and Instability as a Probe for Coronal Heating
Solar coronal loops are the building blocks of the solar corona. These dynamic structures are shaped by the magnetic field that expands into the solar atmosphere. They can be observed in X-ray and
Preface to the Revised Issue
  • Cosmic Discovery
  • 2019
Information, Capacity, and Information Rates
  • Computer Science
    Cosmic Discovery
  • 2019
The Number of Undetected Species
  • Cosmic Discovery
  • 2019
Discoveries
  • Cosmic Discovery
  • 2019
Preface to the 1981 Publication
  • Cosmic Discovery
  • 2019
...
...