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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.

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At least 127 records · Page 7
All sourcesNASA NTRSDOE OSTI
NASA NTRS1987

Determination of O2(a1 delta g) and O2(b1 sigma+ g) yields in the reaction O + ClO --> Cl + O2: implications for photochemistry in the atmosphere of Venus

A discharge flow apparatus with chemiluminescence detector has been used to study the reaction O + ClO --> Cl + O2, where O2 = O2(a1 delta g) or O2(b1 sigma+ g). The measured quantum yields for producing O2(a1 delta g) and O2(b1 sigma+ g) in the above reaction are less than 2.5 x 10(-2) and equal to (4.4 +/- 1.1) x 10(-4), respectively. The observed O2(a1 delta g) airglow of Venus cannot be explained in the context of standard photochemistry using our experimental results and those reported in recent literature. The possibility of an alternative source of O atoms derived from SO2 photolysis in the mesosphere of Venus is suggested.

Non-NASA Center↗
NASA NTRS1980

Asymmetrical ClO3 - Its possible formation from ClO and O2 and its possible reactions

An analysis of recent accurate experimental studies of Cl2-photosensitized O3 decomposition, in which O3 disappearance and OClO formation were directly monitored, suggests the possibility that the suppression of the quantum yield in the presence of O2 may be due to the formation of asymmetrical chlorine trioxide (ClO.O2). Other intermediaries, such as Cl2O2, which may also form in the system are not thought to explain the observations. In addition to its capacity to oxidize, which it shares with other peroxo compounds, asymmetrical ClO3 appears to undergo an interesting class of reactions in which the loosely bound O2 adduct is relatively easily displaced by reactive atoms and radicals such as chlorine.

Prasad, S. S.↗
NASA NTRS1981

Kinetics study of the reactions of NO with FO, ClO, BrO, and IO at 298 K

The kinetics of the four considered reactions were studied by means of the discharge flow/mass spectrometric technique. The discharge flow/mass spectrometer has been described by Sander et al. (1981). The flow velocity in the investigation was varied in the range from 750 to 2100 cm/s, while total pressures in the range from 1.0 torr to 2.1 torr were employed. The results of the study are compared to the values of current literature. With minor exceptions, the new results are in excellent agreement with the data of the previous studies. It is pointed out that the reported results will have a minimal impact on the predictions of atmospheric photochemical model calculations as they have confirmed prior expectations.

Ray, G. W.↗
NASA NTRS1988

Absolute infrared band strength measurement of the ClO radical by Fourier transform infrared spectroscopy

High-resolution (0.005/cm) FTIR spectra of the X2Pi(i)-X2Pi(i) (1-0) rovibrational bands of (C-35)(O-16) and (Cl-37)(O-16) were obtained in 1 torr of helium carrier gas. After measuring the strengths of approximately 830 individual IR lines from several spectra, a total band strength of 13.1 + or - 1.1/sq cm atm and a first Herman-Wallis coefficient of (4.12 + or - 0.62) x 10 to the -3rd were determined.

Lang, Valerie I.↗
NASA NTRS2001

In Situ Detection of OH, HO2, ClO, BrO, NO2, ClONO2, BrONO2, ClOOCl, H2O, and O3 from the ER2

We review here the scientific progress that has emerged during the period January 1, 1998 through March 31, 2001. Results from the Sage III Ozone Loss and Validation Experiment (SOLVE) and Photochemistry of Ozone Loss in the Arctic Region in Summer (POLARIS) mission, and continuing work on prior missions, taken in order, including radical control of ozone on the northern hemisphere stratosphere, evolution of NO2 over the arctic winter and its effects on reactive chlorine, and the first measurements of ClOOCl in the stratosphere.

Anderson, James G.↗
NASA NTRS2005

Chemistry, Dynamics, and Radiation of Ozone Loss: Airborne Measurements of OH, HO2, NO2, ClO, BrO, IO, ClONO2, BrONO2, ClOOCl, and H2O

This grant continued the research initially funded under NAG1-01095. This research addresses, through a combination of in situ and remote aircraft-borne instruments, the following scientific questions: Which mechanisms are responsible for the continuing erosion of ozone over midlatitudes of the Northern Hemisphere? Will the rapid loss of ozone over the Arctic in late winter continue to worsen over the next two decades? Are these large losses dynamically coupled to midlatitudes? Which mechanisms dictate the rate of exchange of material between the troposphere and stratosphere? How will these processes change in response to changes in climate? Will regional scale pollution episodes, that are emerging as predictable seasonal events, significantly affect the middle-to-upper troposphere chemical composition. If so, how will these changes alter the chemical composition of the middle world? What changes are predicted for the overworld? Why has the arctic stratosphere become colder in the late winter phase in recent years? Have increases in tropical upper troposphere temperatures increased the temperature gradient such as to change the trajectories of vertically propagating waves, thus reducing the effectiveness of the meridional circulation for transport of heat, momentum and ozone from the tropics to high latitudes?

Anderson, James G.↗