In situ spectroscopic identification of the six types of asbestos

2021 ◽  
Vol 403 ◽  
pp. 123951
Author(s):  
Vladimir Zholobenko ◽  
Frank Rutten ◽  
Aleksey Zholobenko ◽  
Amy Holmes
2020 ◽  
Author(s):  
Lieven Clarisse ◽  
Alexandre Deguine ◽  
Tim Hultberg ◽  
Nicolas Theys ◽  
Simon Carn ◽  
...  

<p>Hydrogen Chloride (HCl) is an important but still poorly understood magmatic volatile species. Degassed HCl and ratios with other volatiles can be used to monitor, understand and forecast volcanic activity. As the dominant chlorine reservoir species in the stratosphere, and a source of reactive halogens, HCl also plays an important role in the depletion of ozone. The contribution of volcanic HCl to the stratospheric budget is however somewhat debated, but it is generally accepted that scavenging by hydrometeors is a dominant process. Unlike the less soluble SO<sub>2</sub>, this prevents the majority of volcanically emitted HCl from reaching the stratosphere. Currently HCl measurements have only been reported from limb sounders (MLS and ACE-FTS in particular), but given their viewing geometry, their vertical sensitivity is limited to the upper troposphere/lower stratosphere. In the past ten years, MLS was able to measure traces of HCl in a number of large volcanic plumes such as those originating from Sarychev Peak, Nabro and Calbuco.</p><p>Here, we report the first measurements from IASI of HCl in volcanic plumes. We provide unambiguous spectroscopic identification of HCl in the 2670-2760 cm<sup>-1</sup> spectral region in several IASI observed spectra. A survey of 12 years of IASI data was carried out, and revealed several large plumes of volcanic HCl. We show two notably large plumes of HCl identified in the eruptions of Calbuco (2015) and Raikoke (2019). For these two eruptions, we show that HCl is detected in the lower altitude plumes emitted towards the end of the eruptions (and not in the main, higher-altitude and SO<sub>2</sub>-rich plumes).  This finding could be a result of the greater scavenging of HCl relative to SO<sub>2</sub> in rapidly rising plumes, but could also be related to particular degassing mechanics of different volatile components in the erupted melt. First quantitative estimates indicate that for the analysed plumes, the HCl/SO<sub>2</sub> molar ratios exceed one, which is much higher than the typical ratios measured by MLS (typically below 0.05) and also higher than reported from petrological data or in situ measurements (typically in the range 0.1-0.3).</p>


2015 ◽  
Vol 49 (4) ◽  
pp. 2560-2567 ◽  
Author(s):  
Katharina Müller ◽  
Annett Gröschel ◽  
André Rossberg ◽  
Frank Bok ◽  
Carola Franzen ◽  
...  

1999 ◽  
Vol 188 (2) ◽  
pp. 426-430 ◽  
Author(s):  
M. Cavers ◽  
J.M. Davidson ◽  
I.R. Harkness ◽  
L.V.C. Rees ◽  
G.S. McDougall

1996 ◽  
Vol 436 ◽  
Author(s):  
E. C. Samano ◽  
Gerardo Soto ◽  
Arturo Gamietea ◽  
Leonel Cota

AbstractThin carbon films were grown on Si (111) substrates by ablating a graphite target utilizing an excimer pulsed laser in a UHV Riber © LDM-32 system. Two kinds of films were produced, a highly oriented pyrolytic graphite (HOPG) type and a diamond-like carbon (DLC) type. A relationship of the films microstructure with laser power density and substrate conditions was observed. The HOPG films were homogeneous but the DLC films were heterogeneous, as shown by micrographs. The thin films are monitored and analyzed in situ during the first stages of the deposition process. The monitoring was done by RHEED and the characterization by several surface spectroscopic techniques, AES, XPS and EELS. The formation of a SiC interface was observed for both films due to the reaction of the first carbon species with the substrate surface.


2016 ◽  
Vol 7 (23) ◽  
pp. 4847-4853 ◽  
Author(s):  
Hsin-Yi Wang ◽  
Sung-Fu Hung ◽  
Ying-Ya Hsu ◽  
Lulu Zhang ◽  
Jianwei Miao ◽  
...  

1984 ◽  
Vol 75 ◽  
pp. 743-759 ◽  
Author(s):  
Kerry T. Nock

ABSTRACTA mission to rendezvous with the rings of Saturn is studied with regard to science rationale and instrumentation and engineering feasibility and design. Future detailedin situexploration of the rings of Saturn will require spacecraft systems with enormous propulsive capability. NASA is currently studying the critical technologies for just such a system, called Nuclear Electric Propulsion (NEP). Electric propulsion is the only technology which can effectively provide the required total impulse for this demanding mission. Furthermore, the power source must be nuclear because the solar energy reaching Saturn is only 1% of that at the Earth. An important aspect of this mission is the ability of the low thrust propulsion system to continuously boost the spacecraft above the ring plane as it spirals in toward Saturn, thus enabling scientific measurements of ring particles from only a few kilometers.


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