scholarly journals Photochirogenesis: Photochemical Models on the Origin of Biomolecular Homochirality

Symmetry ◽  
2010 ◽  
Vol 2 (2) ◽  
pp. 1055-1080 ◽  
Author(s):  
Cornelia Meinert ◽  
Jean-Jacques Filippi ◽  
Laurent Nahon ◽  
Søren V. Hoffmann ◽  
Louis D’Hendecourt ◽  
...  
Keyword(s):  
Biomolecular Homochirality ◽  
Photochemical Models

scholarly journals One dimension photochemical models in global mean conditions in question: Application to Titan

Icarus ◽  
2021 ◽  
Vol 364 ◽  
pp. 114477
Author(s):  
M. Dobrijevic ◽  
J.C. Loison ◽  
V. Hue ◽  
T. Cavalié
Keyword(s):  
One Dimension ◽  
Global Mean ◽  
Photochemical Models

scholarly journals THE DUST PROPERTIES OFz∼ 3 MIPS-LBGs FROM PHOTOCHEMICAL MODELS

2013 ◽  
Vol 768 (2) ◽  
pp. 178 ◽  
Author(s):  
X. L. Fan ◽  
A. Pipino ◽  
F. Matteucci
Keyword(s):  
Photochemical Models

Biomolecular homochirality

1988 ◽  
Vol 17 ◽  
pp. 347 ◽  
Author(s):  
Stephen Mason
Keyword(s):  
Biomolecular Homochirality

How Measurements of Rate Coefficients at Low Temperature Increase the Predictivity of Photochemical Models of Titan’s Atmosphere†

2009 ◽  
Vol 113 (42) ◽  
pp. 11227-11237 ◽  
Author(s):  
E. Hébrard ◽  
M. Dobrijevic ◽  
P. Pernot ◽  
N. Carrasco ◽  
A. Bergeat ◽  
...  
Keyword(s):  
Low Temperature ◽  
Temperature Increase ◽  
Rate Coefficients ◽  
Photochemical Models

scholarly journals Quiescent and flaring lyman-α radiation of host stars and effects on exoplanets

2015 ◽  
Vol 11 (S320) ◽  
pp. 391-396
Author(s):  
Jeffrey L. Linsky ◽  
Kevin France ◽  
Yamila Miguel ◽  
Lisa Kaltenegger
Keyword(s):  
Emission Lines ◽  
Late Type ◽  
Chemical Abundances ◽  
Interstellar Absorption ◽  
Ultraviolet Spectra ◽  
M Stars ◽  
Host Stars ◽  
Stars Flare ◽  
Photochemical Models

AbstractLyman-α radiation dominates the ultraviolet spectra of G, K, and M stars and is a major photodissociation source for H2O, CO2, and CH4 in the upper atmospheres of exoplanets. We obtain intrinsic Lyman-α line fluxes for late-type stars by correcting for interstellar absorption or by scaling from other spectroscopic observables. When stars flare, all emission lines brighten by large factors as shown by HST spectra. We describe photochemical models of the atmosphere of the mini-Neptune GJ 436b (Miguel et al. 2015) that show the effects of flaring Lyman-α fluxes on atmospheric chemical abundances.

In situ measurements of the NO2/NO ratio for testing atmospheric photochemical models

1994 ◽  
Vol 21 (23) ◽  
pp. 2555-2558 ◽  
Author(s):  
L. Jaeglé ◽  
C. R. Webster ◽  
R. D. May ◽  
D. W. Fahey ◽  
E. L. Woodbridge ◽  
...  
Keyword(s):  
In Situ Measurements ◽  
Photochemical Models

scholarly journals Loss of isoprene and sources of nighttime OH radicals at a rural site in the United States: Results from photochemical models

2002 ◽  
Vol 107 (D5) ◽  
pp. ACH 2-1-ACH 2-14 ◽  
Author(s):  
Sanford Sillman ◽  
Mary Anne Carroll ◽  
Troy Thornberry ◽  
Brian K. Lamb ◽  
Hal Westberg ◽  
...  
Keyword(s):  
United States ◽  
The United States ◽  
Rural Site ◽  
Oh Radicals ◽  
Photochemical Models
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