scholarly journals Cloud geometry from oxygen-A-band observations through an aircraft side window

2019 ◽  
Vol 12 (2) ◽  
pp. 1167-1181 ◽  
Author(s):  
Tobias Zinner ◽  
Ulrich Schwarz ◽  
Tobias Kölling ◽  
Florian Ewald ◽  
Evelyn Jäkel ◽  
...  

Abstract. During the ACRIDICON-CHUVA (Aerosol, Cloud, Precipitation, and Radiation Interactions and Dynamics of Convective Cloud Systems–Cloud Processes of the Main Precipitation Systems in Brazil: A Contribution to Cloud Resolving Modeling and to the GPM (Global Precipitation Measurement)) aircraft campaign in September 2014 over the Amazon, among other topics, aerosol effects on the development of cloud microphysical profiles during the burning season were studied. Hyperspectral remote sensing with the imaging spectrometer specMACS provided cloud microphysical information for sun-illuminated cloud sides. In order to derive profiles of phase or effective radius from cloud side observations, vertical location information is indispensable. For this purpose, spectral measurements of cloud-side-reflected radiation in the oxygen A absorption band collected by specMACS were used to determine absorption path length between cloud sides and the instrument aboard the aircraft. From these data, horizontal distance and eventually vertical height were derived. It is shown that, depending on aircraft altitude and sensor viewing direction, an unambiguous relationship of absorption and distance exists and can be used to retrieve cloud geometrical parameters. A comparison to distance and height information from stereo image analysis (using data of an independent camera) demonstrates the efficiency of the approach. Uncertainty estimates due to method, instrument and environmental factors are provided. The main sources of uncertainty are unknown in cloud absorption path contributions due to complex 3-D geometry or unknown microphysical properties, variable surface albedo and aerosol distribution. A systematic difference of 3.8 km between the stereo and spectral method is found which can be attributed to 3-D geometry effects not considered in the method's simplified cloud model. If this offset is considered, typical differences found are 1.6 km for distance and 230 m for vertical position at a typical distance around 20 km between sensor and convective cloud elements of typically 1–10 km horizontal and vertical extent.

2018 ◽  
Author(s):  
Tobias Zinner ◽  
Ulrich Schwarz ◽  
Tobias Kölling ◽  
Florian Ewald ◽  
Evelyn Jäkel ◽  
...  

Abstract. During the ACRIDICON-CHUVA aircraft campaign in September 2014 over the Amazon, among other topics aerosol effects on the development of cloud microphysical profiles during the burning season were studied. Hyperspectral remote sensing with the imaging spectrometer specMACS provided cloud microphysical information for sun-illuminated cloud sides. In order to derive profiles of phase or effective radius from cloud side observations vertical location information is indispensable. For this purpose, spectral measurements of cloud side reflected radiation in the oxygen-A absorption band collected by specMACS were used to determine absorption path length between cloud sides and the instrument aboard the aircraft. From these data horizontal distance and eventually vertical height were derived. It is shown that, depending on aircraft altitude and sensor viewing direction, an unambiguous relationship of absorption and distance exists and can be used to retrieve cloud geometrical parameters. A comparison to distance and height information from stereo image analysis (using data of an independent camera) demonstrates the efficiency of the approach. Uncertainty estimates due to method, instrument and environmental factors are provided by the method. Main sources of uncertainty are unknown in-cloud absorption path contributions due to complex 3D geometry or unknown microphysical properties, variable surface albedo and aerosol distribution. A systematic difference of 3.8 km between stereo and spectral method is found which can be attributed to 3D geometry effects not considered in the methods simplified cloud model. If this offset is considered, typical differences found are 1.6 km for distance and 230 m for vertical position at a tpyical distance around 20 km between sensor and convective cloud elements of typically 1–10 km horizontal and vertical extent.


Atmosphere ◽  
2021 ◽  
Vol 12 (1) ◽  
pp. 63
Author(s):  
Sidou Zhang ◽  
Shiyin Liu ◽  
Tengfei Zhang

By using products of the cloud model, National Centers for Environmental Prediction (NCEP) Final Operational Global Analysis (FNL) reanalysis data, and Doppler weather radar data, the mesoscale characteristics, microphysical structure, and mechanism of two hail cloud systems which occurred successively within 24 h in southeastern Yunnan have been analyzed. The results show that under the influence of two southwest jets in front of the south branch trough (SBT) and the periphery of the western Pacific subtropical high (WPSH), the northeast-southwest banded echoes affect the southeastern Yunnan of China twice. Meanwhile, the local mesoscale radial wind convergence and uneven wind speed lead to the intense development of convective echoes and the occurrence of hail. The simulated convective cloud bands are similar to the observation. The high-level mesoscale convergence line leads to the development of convective cloud bands. The low-level wind direction or wind speed convergence and the high-level wind speed divergence form a deep tilted updraft, with the maximum velocity of 15 m·s−1 at the −40~−10 °C layer, resulting in the intense development of local convective clouds. The hail embryos form through the conversion or collision growth of cloud water and snowflakes and have little to do with rain and ice crystals. Abundant cloud water, especially the accumulation region of high supercooled water (cloud water) near the 0 °C layer, is the key to the formation of hail embryos, in which qc is up to 1.92 g·kg−1 at the −4~−2 °C layer. The hail embryos mainly grow by collision-coalescence (collision-freezing) with cloud water (supercooled cloud drops) and snow crystal riming.


2015 ◽  
Vol 51 (1) ◽  
pp. 11-27 ◽  
Author(s):  
Vlado Spiridonov ◽  
Theodore Karacostas ◽  
Dimitrios Bampzelis ◽  
Ioannis Pytharoulis

2009 ◽  
Vol 9 (6) ◽  
pp. 24361-24410 ◽  
Author(s):  
V. Marécal ◽  
M. Pirre ◽  
E. D. Rivière ◽  
N. Pouvesle ◽  
J. N. Crowley ◽  
...  

Abstract. The present paper is a preliminary study preparing the introduction of reversible trace gas uptake by ice particles into a 3-D cloud resolving model. For this a 3-D simulation of a tropical deep convection cloud was run with the BRAMS cloud resolving model using a two-moment bulk microphysical parameterization. Trajectories encountering the convective clouds were computed from these simulation outputs along which the variations of the pristine ice, snow and aggregate mixing ratios and size distributions were extracted. The reversible uptake of 11 trace gases by ice was examined assuming applicability of Langmuir isotherms using recently evaluated (IUPAC) laboratory data. The results show that ice uptake is only significant for HNO3, HCl, CH3COOH and HCOOH. For H2O2, using new results for the partition coefficient results in significant partitioning to the ice phase for this trace gas also. It was also shown that the uptake is largely dependent on the temperature for some species. The adsorption saturation at the ice surface for large gas concentrations is generally not a limiting factor except for HNO3 and HCl for gas concentration greater than 1 ppbv. For HNO3, results were also obtained using a trapping theory, resulting in a similar order of magnitude of uptake, although the two approaches are based on different assumptions. The results were compared to those obtained using a BRAMS cloud simulation based on a single-moment microphysical scheme instead of the two moment scheme. We found similar results with a slightly more important uptake when using the single-moment scheme which is related to slightly higher ice mixing ratios in this simulation. The way to introduce these results in the 3-D cloud model is discussed.


2008 ◽  
Vol 47 (2) ◽  
pp. 562-575 ◽  
Author(s):  
J. A. Weinman ◽  
F. S. Marzano

Abstract Global precipitation measurements from space-based radars and microwave radiometers have been the subject of numerous studies during the past decade. Rainfall retrievals over land from spaceborne microwave radiometers depend mainly on scattering from frozen hydrometeors. Unfortunately, the relationship between frozen hydrometeors and rainfall varies considerably. The large field of view and related beam filling of microwave radiometer footprints introduce additional difficulties. Some of these problems will be addressed by the improved sensors that will be placed on the Global Precipitation Measurement (GPM) core satellite. Two shuttle missions demonstrated that X-band synthetic aperture radar (X-SAR) could observe rainfall over land. Several X-band SARs that can provide such measurements will be launched in the coming decade. These include four Constellation of Small Satellites for Mediterranean Basin Observations (COSMO-SkyMed), two TerraSAR-X, and a fifth Korea Multipurpose Satellite (KOMPSAT-5) to be launched by the Italian, German, and Korean Space Agencies, respectively. Data from these satellites could augment the information available to the GPM science community. The present study presents computations of normalized radar cross sections (NRCS) that employed a simple, idealized two-layer cloud model that contained both rain and frozen hydrometeors. The modeled spatial distributions of these hydrometeors varied with height and horizontal distance. An exploratory algorithm was developed to retrieve the shape, width, and simple representations of the vertical profiles of frozen hydrometeors and rain from modeled NRCS scans. A discussion of uncertainties in the retrieval is presented.


1977 ◽  
Vol 55 (6) ◽  
pp. 1104-1110 ◽  
Author(s):  
John E. Drake ◽  
J. Lawrence Hencher ◽  
Quang Shen

The molecular structures of dichloro(dimethyl)germane and trichloro(methyl)germane have been determined in the vapour phase by electron diffraction. The principal geometrical parameters for (CH3)2GeCl2 are rg(Ge—Cl) = 2.143 ± 0.004 Å, rg(Ge—C) = 1.928 ± 0.006 Å, [Formula: see text].and [Formula: see text] In the analysis of CH3GeGl3 recently reported values of the rotational constants were combined with the electron diffraction data to give rg(Ge—Cl) = 2.132 ± 0.003 Å, rg(Ge—C) = 1.893 ± 0.010 Å, [Formula: see text] and [Formula: see text]In both cases the methylgermane geometry was assumed for the methyl group [Formula: see text] which was fixed in the staggered configuration with respect to the C2GeCl2 and CGeCl3 frames respectively. Both random and systematic errors were included in the uncertainty estimates, which are believed to be approximately at the 95% confidence level. In the case of (CH3)2GeCl2 the uncertainties in [Formula: see text] were enlarged to four times the least-squares values in order to reflect the difficulty of resolving the Cl … Cl, C … Cl, and C … C distances in the analysis.


2005 ◽  
Vol 5 (10) ◽  
pp. 2749-2759 ◽  
Author(s):  
F. J. Nober ◽  
H. F. Graf

Abstract. A new cumulus convection parameterisation is presented in this paper. The parameterisation uses an explicit spectral approach and determines, unlike other convection schemes, for each convection event a new cloud distribution function regarding to the given vertical temperature and humidity profiles. This is done by using a one dimensional cloud model to create a spectrum of different clouds. The interaction between all non convective physical processes in the AGCM and all different clouds is taken into account to calculate a selfconsistent cloud spectrum. The model has been implemented in the ECHAM5 AGCM and tested against a large eddy simulation model. The representation of a shallow cumulus cloud field by the AGCM could be much improved. Diurnal cycle, cloud cover, liquid water path and the vertical structure of the mass flux, determined by the new convection scheme are close to the large eddy simulation, whereas the standard convection scheme failed in simulating this convection episode.


1870 ◽  
Vol 160 ◽  
pp. 117-174 ◽  

The following investigations were commenced about nine years ago, and some of the results were laid before the Physiological Subsection of the British Association Meeting at Manchester in 1861. Circumstances, during a series of years, prevented the writer from elaborating so fully as he desired the results of the measurements which he had already made ; but this is the less to be regretted, as in the meantime he has had opportunity of making additional measurements, and the writings of others which have from time to time appeared have given him additional information without interfering with the line of inquiry which he proposed to himself to pursue. That inquiry was commenced in the belief that descriptions of crania expressing, however precisely, the surface-peculiarities which meet the eye, were not sufficient to determine the real nature of the differences existing between the crania of different nations or individuals ; that it was necessary to consider the arch and the base of the skull in their connexion one with the other, and to measure the relations of parts by means of distances and angles more systematically than had been done ; and that if this were done it would appear that there were far more important variations in the antero-posterior direction in skulls than were suspected, or than existed in their breadth. The various forms of forehead, vertex, and occiput are noted by anatomists without sufficient knowledge how these local appearances are related to the structure of the cranium as a whole. Even such generally used words as dolichocephalous, brachycephalous, orthognathous, and prognathous, though efforts have been made to render them perfectly explicit, refer to varieties of form which have not been properly understood. Mode of measurement . —It may be frankly admitted that probably the system of “geometrical drawing” recommended and described by Lucae * would have been preferable in some respects to the mode of craniometry employed by the writer, but most of the measurements were made before Lucae’s method was published. Also it may be admitted that vertical sections, which afford the most accurate of all bases for profile views, might have been used to a greater extent than they were; but there was a difficulty in asking that a number of skulls in Museums should be bisected for examination by a private individual. Still some bisections have been obtained, sufficient to illustrate the substantial accuracy of the system in most instances followed; and while mentioning this, it is right to say how much indebted the writer has been to the late Professor Goodsir and Professor Allman of Edinburgh, and to Professor Allen Thomson, for their kindness in placing specimens at his disposal. The craniometer which the writer has employed is not without its advantages, being an instrument fitted to determine the exact relation of any point in space to a given starting-point. The skull is suspended in a horizontal frame by means of two pointed screws, one on each side, which work in fixed supports; and by other screws moving on slides it may be set with any two points on a level. A vertical bar, which can be slipped up and down, slides along the side of the frame, and bears a sliding horizontal bar directed inwards, to which a needle may be attached at right angles if necessary, in either a vertical or longitudinal direction. The frame, the bars, and the needle are all marked off in inches and tenths, and by this means the vertical and horizontal distance of any point on the skull from the place of suspension is easily determined and marked on paper, so that by a series of such points a diagram may be constructed. With the assistance of a sheet of ruled paper such a diagram may be constructed in a few minutes from a series of figures not occupying more than a couple of lines. It is convenient to register the number indicating the vertical position of a point with that indicating the horizontal position placed immediately below it, like the denominator of a vulgar ^fraction; while backward and downward directions may be respectively distinguished from forward and upward directions by placing — before the figure. Thus the following formula is sufficient for the construction of a diagram of the Irish skull 54:— -.4/.05 -.7/-1.35 .1/1.05 -.65/1.9 -1.2/3.5 -6/3.65 -.3/-3. .75/-3.65 1.9/-3.65 4.4/-2.3 5./.55 3.85/3.05 1.8/3.65 1.3/3.55 1.1/1.5 If to this formula there be added the breadth at as many points as may be desired, and the positions of those points, the utmost completeness may be given to it. By this system of notation the outline of the profile of every skull in every Museum might be recorded with the greatest accuracy, either from measurements taken with the craniometer described, or from geometrical drawings, or tracings of vertical sections.


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