Abstract
In this chapter, we introduce the way the energetic electromagnetic flux is emitted by the Sun, and we present how it creates an upper partly ionized layer in the Earth atmosphere. © 2006 Springer.
Cite
CITATION STYLE
APA
Lilensten, J., & Kretzschmar, M. (2006). The solar spectrum in the UV, EUV, and X ranges: Observations, modelling, and effects on the Earth upper atmosphere in the frame of space weather. Lecture Notes in Physics, 699, 53–91. https://doi.org/10.1007/3-540-33759-8_4
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free