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Remote sensing the vertical profile of cloud droplet effective radius, thermodynamic phase, and temperature
(COPERNICUS GESELLSCHAFT MBH, 2011)
Cloud-aerosol interaction is a key issue in the climate system, affecting the water cycle, the weather, and the total energy balance including the spatial and temporal distribution of latent heat release. Information on ...
Internet of things-based cloud computing platform for analyzing the physical health condition
BACKGROUND: Health monitoring is important for early disease diagnosis and will reduce the discomfort and treatment expenses, which is very relevant in terms of prevention. The early diagnosis and treatment of multiple ...
Dense clumps in giant molecular clouds in the large magellanic cloud: density and temperature derived from (co)-c-13(j=3-2) observations
(AMERICAN INSTITUTE OF PHYSICS, 2011)
A cluster approach to cloud cover classification over South America and adjacent oceans using a k-means/k-means++ unsupervised algorithm on GOES IR imagery
(Molecular Diversity Preservation International, 2020-09)
An unsupervised k-means/k-means++ clustering algorithm was implemented on daily images of standardized anomalies of brightness temperature (Tb) derived from the Geostationary Operational Environmental Satellite (GOES)-13 ...
Modelling [C I] emission from turbulent molecular clouds
(Royal Astronomical Society, 2015)
We use detailed numerical simulations of a turbulent molecular cloud to study the usefulness
of the [CI] 609 and 370 μmfine structure emission lines as tracers of cloud structure. Emission
from these lines is observed ...
A (C-12)O survey of the Small Magellanic Cloud
(1991-02-10)
The central 2 arcsec x 2 arcsec region of the SMC has been fully surveyed to search for (C-12)O emission in the J = 1-0 transition. (C-12)O emission from two large complexes located in the southwest and northeast regions ...
LABOCA observations of giant molecular clouds in the southwest region of the Small Magellanic Cloud
(2010)
Context. The amount of molecular gas is a key to understanding the future star formation in a galaxy. Because H2 is difficult to
observe directly in dense and cold clouds, tracers such as the CO molecule are used. However, ...
A cautionary note on the computation of daily mean temperatures and their trends
(John Wiley & Sons Ltd, 2017-07)
There are different methodologies to compute daily mean temperatures (DMT), including averaging the 24-hourly temperature values, readings at specific times throughout the day or simply averaging the minimum and maximum ...
Submillimeter Observations of Giant Molecular Clouds in the Large Magellanic Cloud: Temperature and Density as Determined from J=3-2 and J=1-0 Transitions of CO
(2008)
We have carried out submillimeter 12CO(J = 3–2) observations of six giant molecular clouds (GMCs) in the Large Magellanic Cloud (LMC) with the ASTE 10 m submillimeter telescope at a spatial resolution of 5 pc and very high ...
Dense Clumps in Giant Molecular Clouds in the Large Magellanic Cloud: Density and Temperature Derived from 13CO(J = 3-2) Observations
(2011)
In order to precisely determine the temperature and density of molecular gas in the Large Magellanic Cloud, we made observations of the optically thin (13)CO(J = 3-2) transition using the ASTE 10 m telescope toward nine ...