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The algorithm registers two point clouds by first associating a [[piecewise]] [[normal distribution]] to the first p ...">{{harv|Biber|Straßer|2003}}</ref> the algorithm was extended to 3D point clouds<ref>{{harv|Magnusson|2009}}</ref> and has wide applications in [[computer v ...

...not easily push high density clouds. As the cosmic winds start to push the clouds, they start to separate and start looking like taffy being pulled apart.<re ...

...s are often greater than those of the synoptic flow. Parameterizations of clouds and convection aim to address the scaling differences between GCM grids and ...ther way to account for large-scale supersaturation clouds is to benchmark clouds via temperature variability, in that wherever the temperature "causes the r ...

...applied to various PDEs on surfaces. Reaction–diffusion problems on point clouds '''[RD]''', eigenvalue problems '''[EV]''', and level set equations '''[LS] ...S. J. (2013). Simple computation of reaction-diffusion processes on point clouds. Proceedings of the National Academy of Sciences, 110(23), 9209–9214 [http: ...

...|last2=Lucas |first2=R. |date=2001 |title=Comparative chemistry of diffuse clouds: II. CN, HCN, HNC, CH₃CN & N₂H⁺ |journal=[ *Dissociative recombination in diffuse clouds:<ref name="Comparative"/> ...

}}</ref> The castellanus characteristic is particularly obvious when the clouds are observed from the side (i.e., from a vantage point on a line perpendicu ...sation]].<ref name=Corfidi>{{Harvnb|Corfidi|2008|ref=Corfidi}}</ref> Those clouds some would classify as cumulus castellanus typically do not have a common b ...

.../ref> This is believed to be due to the hydrogen scarcity of some of these clouds. Interference with hydrogen is one of the reason for the molecule's instabi Cyanopolyynes were first discovered in interstellar molecular clouds in 1971 using [[millimeter wave]] and [[radio telescopes|microwave telescop ...

...=":0">{{Cite book |last1=Pruppacher |first1=Hans R. |title=Microphysics of clouds and precipitation |last2=Klett |first2=James D. |date=2010 |publisher=Sprin ...l=https://www.worldcat.org/title/694393873 |title=Physics and chemistry of clouds |last2=Verlinde |first2=Johannes |date=2011 |publisher=Cambridge University ...

...cities which are measured in excess of 70–90&nbsp;km s⁻¹. These clouds of gas can be massive in size, some on the order of millions of times the [ ...amount of [[baryonic matter]] in the galactic halo. In addition, as these clouds fall into the disk of the galaxy, they add material that can form stars in ...

...us feature of the less bright [[Orion molecular cloud complex]]) and broad-clouds [[North America Nebula]] (and [[Pelican Nebula]]) which is an intrinsic par ...ard University|language=en|access-date=2020-01-09}}</ref> Inside the dense clouds, gas can be so compressed that new [[stars]] are born.<ref name="bbc"/> It ...

...st3 = A. A. | title = Dust-enshrouded giants in clusters in the Magellanic Clouds. | arxiv = astro-ph/0507571 | doi = 10.1051/0004-6361:20053528 | journal = ...=Hyland|first6=A. R.|date=October 1992|title=OH/IR Stars in the Magellanic Clouds|journal= The Astrophysical Journal|language=en|volume=397|pages=552|doi=10. ...

..._017_0847_lfrsob_2_0_co_2.xml Low-Frequency Resonant Scattering of Bubble Clouds] by Paul A. Hwang and William J. Teague, 2000, Journal of Atmospheric and O ...

...ore be some process that fragments the [[cloud]] into smaller high density clouds whose masses are in the same range as that of stars. Self-gravity cannot do ...

...o several months.<ref name=":1" /> Regardless of the event's lifespan, the clouds it produces increase [[turbidity]] and hamper light penetration.<ref name=" ...43..200H|issn=0024-3590|doi-access=free}}</ref> The cyanobacteria abundant clouds also hold the potential to act as a means to study the microorganism's role ...

...o-ph/0008454 }}</ref> The method is also employed for prestellar molecular clouds.<ref>{{cite journal |last1=Crutcher |first1=Richard M. |last2=Nutter |first ...

The global effective particle radius has different values for water and ice clouds: the former is around 14 μm, whereas for ice it is around 25 μm. Studies al ...

...of gaseous objects (for example, [[star formation]] occurs when molecular clouds collapse under gravity), and thus the stability of gaseous systems is of gr ...

...13 February 2012|title=The Optical Depth of H II Regions in the Magellanic Clouds|journal=The Astrophysical Journal|volume=755|issue=1|pages=30|bibcode=2012A ...J.|date=1976|title=The nebular complexes of the Large and Small Magellanic Clouds|journal=Memoirs of the Royal Astronomical Society|volume=81|pages=89|url=ht ...

...ymétrique conditionnelle.svg|thumb|Upward movement in an area of CSI gives clouds, downward movement clears the sky.]] ...[[precipitation]] within a region otherwise [[wikt:stratiform|stratiform]] clouds.<ref name=Schultz/> As the motion is in an area near saturation, the partic ...

...]], [[snow]], [[Freezing rain|sleet]], etc...), and the different types of clouds that produce them vary in time and space, the coefficients of the drop dist ...hunderstorms) or [[Nimbostratus cloud|stratiform]] (like from nimbostratus clouds) which have different <math>\Lambda</math>, K, N₀ and <math>\scr ...