Lower Atmospheric Energy Sources for the Upper Atmosphere

Author(s):  
Richard S. Lindzen
2015 ◽  
Vol 6 (1) ◽  
pp. 49 ◽  
Author(s):  
Nasrullah Khan ◽  
Naeem Abas ◽  
Anam Kalair

1959 ◽  
Vol 1 (1) ◽  
pp. 14-19 ◽  
Author(s):  
V.I. Krassovsky

2008 ◽  
Vol 4 (S251) ◽  
pp. 321-326 ◽  
Author(s):  
J. H. Waite ◽  
D. T. Young ◽  
A. J. Coates ◽  
F. J. Crary ◽  
B. A. Magee ◽  
...  

AbstractIon-neutral chemistry in Titan's upper atmosphere (~ 1000 km altitude) is an unexpectedly prodigious source of hydrocarbon-nitrile compounds. We report observations from the Cassini Ion Neutral Mass Spectrometer (INMS; Waite et al. 2004) and Cassini Plasma Spectrometer (CAPS; Young et al. 2004) that allow us to follow the formation of the organic material from the initial ionization and dissociation of nitrogen and methane driven by several free energy sources (extreme ultraviolet radiation and energetic ions and electrons) to the formation of negative ions with masses exceeding 10,000 amu.


IEE Review ◽  
1991 ◽  
Vol 37 (4) ◽  
pp. 152
Author(s):  
Kenneth Spring

2020 ◽  
Vol 64 (1-4) ◽  
pp. 1447-1452
Author(s):  
Vincent Mazauric ◽  
Ariane Millot ◽  
Claude Le Pape-Gardeux ◽  
Nadia Maïzi

To overcome the negative environemental impact of the actual power system, an optimal description of quasi-static electromagnetics relying on a reversible interpretation of the Faraday’s law is given. Due to the overabundance of carbon-free energy sources, this description makes it possible to consider an evolution towards an energy system favoring low-carbon technologies. The management for changing is then explored through a simplified linear-programming problem and an analogy with phase transitions in physics is drawn.


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