On the spatial distribution of radicals produced by irradiation
Electron spin resonance techniques to determine spatial distribution of radicals produced by irradiation
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Electron spin resonance techniques to determine spatial distribution of radicals produced by irradiation
Space lifetime of possible parent molecules of radicals in comets estimated from absorption cross sections and solar uv flux
Nature of free radicals in Bokkeveld meteorite from paramagnetic resonance signals
Electronic paramagnetic resonance of free organic radicals in meteorites
Matrix isolation of reaction of fluorine atoms with carbon monoxide - infrared and ultraviolet spectrum of free radical fluorocarbon monoxide
IR and UV spectra of free radical FCO in argon matrix at cryogenic temperature of reaction of F atoms with CO
Spectrum, adsorption, and bonding of carbon monoxide radicals on magnesium oxide with electron paramagnetic resonance techniques
Electron paramagnetic resonance studies of OH RADICAL in ice and several crystal hydrates after irradiation
Infrared and ultraviolet absorption spectra of free radical in photolysis of cyanogen azide
IR and UV absorption spectra of free radical NCN observed following photolysis of matrix isolated cyanogen nitride
Free radical CCO spectroscopy when produced by vacuum UV photolysis of matrix isolated carbon suboxide
Temperature dependence and reaction energetics of free radical addition of trifluoroacetonitrile to ethylene
Free radical addition of perfluoroacetonitrile to vinyl fluoride, noting formation of one isomeric compound
Orientation of free radicals in addition reactions with unsymmetrical monoolefins
Free radical formation in amino acids exposed to thermal hydrogen atoms
Radio signals reflection by free radicals in ionosphere, observing predicted intensity and particle detection
Decadal trends and interannual variations in the hydroxyl radical (OH), while poorly constrained at present, are critical for understanding the observed evolution of atmospheric methane (CH4). Through analyzing the OH fields simulated by the model ensemble of the Chemistry-Climate Model Initiative (CCMI), we find (1) the negative OH anomalies during the El Niño years mainly corresponding to the enhanced carbon monoxide (CO) emissions from biomass burning and (2) a positive OH trend during 1980-2010 dominated by the elevated primary production and the reduced loss of OH due to decreasing CO after 2000. Both two-box model inversions and variational 4D inversions suggest that ignoring the negative anomaly of OH during the El Niño years leads to a large overestimation of the increase in global CH4 emissions by up to10±3Tg yr-1to match the observed CH4 increase over these years. Not accounting for the increasing OH trends given by the CCMI models leads to an underestimation of the CH4 emission increase by 23±9Tg yr-1from 1986 to 2010. The variational inversion estimated CH4 emissions show that the tropical regions contribute most to the uncertainties related to OH. This study highlights the significant impact of climate and chemical feedbacks related to OH on the top-down estimates of the global CH4 budget.
On 15th Jan. 2022 the submarine Hunga volcano erupted injecting approximately 0.5 Tg of sulfur dioxide into the stratosphere, but more significantly added 150-170 Tg of water vapor to the stratospheric background (over a 10% perturbation) in a matter of several hours. The sulfur dioxide rapidly converted to sulfate aerosol and along with water vapor, was transported around the Southern Hemisphere sub-tropics into midlatitudes and beyond with some transport into the Northern Hemisphere. With a much longer lifetime than sulfate aerosol, measurable water vapor mass anomalies have persisted with only small losses over more than 2 years since the eruption and are likely to continue above background for the remainder of the decade. Satellite measurements from limb and nadir viewing observing instruments provide the information needed to reasonably initialize the Hunga eruption in the Goddard Earth Observing System (GEOS) model using the “replay” framework coupled to the Global Modeling Initiative (GMI) stratosphere-troposphere chemical mechanism for the recent past and have continued the simulations into the future with the free running chemistry climate model (CCM). Using a number of model ensemble members together with the satellite observations, we quantify how the Hunga eruption is perturbing atmospheric composition and climate and projecting the influences to come as the enhanced water vapor continues in the stratosphere with only very slow removal mechanisms. Modeling suggests that the water rich eruption enhanced stratospheric hydroxyl radiacal (OH) and is supported by the speed of the observed conversion of SO2 into sulfate aerosol. These simulations also suggest a significant reduction in tropospheric OH over the mid-high latitude Southern Hemisphere, which has implications for numerous species that are impacted by this radical. The Hunga eruption provides a useful test of chemistry climate models and an opportunity for observation-based process understanding and in making new connections.