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The coronal density and emission measure

High-temperature differential emission measure and altitude variations in the temperature and density of solar flare coronal X-ray sources

High-temperature differential emission measure and altitude variations in the temperature and density of solar flare coronal X-ray sources

... We developed a thermal bremsstrahlung X-ray emission model with inhomogeneous temperature and density distributions to simultaneously reproduce i DEMT ; ii altitude as a function of ener[r] ...

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Differential Emission Measure Analysis of a Polar Coronal Hole During the Solar Minimum in 2007

Differential Emission Measure Analysis of a Polar Coronal Hole During the Solar Minimum in 2007

... of coronal holes and the quiet ...the coronal hole plasma is made of two distinct components, one at typical coronal hole temperatures (log T = ...

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New Infrared Tools to Measure the Solar Coronal Magnetic Field.

New Infrared Tools to Measure the Solar Coronal Magnetic Field.

... normalize coronal spectra and divide out the gain ...the coronal spectra and this is often not the case due to temperature variations inside the optical ...for coronal HeI1083 emission because ...

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MITIGATION MEASURE FOR VEHICLES EXHAUST EMISSION

MITIGATION MEASURE FOR VEHICLES EXHAUST EMISSION

... METHODOLOGY FOR ESTIMATING GHG There are two approaches for calculating the emission factor. The first one is "The Energy based approach" which is the simplest and accurate way of calculating ...

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On the influence of CMEs on the global 3-D coronal electron density

On the influence of CMEs on the global 3-D coronal electron density

... 3-D coronal electron density In the present paper we study the pre- and post-CME coro- nal electron density structure and compared it with the poten- tial field source surface (PFSS) models for the ...

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Coronal density structure and its role in wave damping in loops

Coronal density structure and its role in wave damping in loops

... Next, we consider heating by phase mixing in the evolving atmosphere discussed in Section 3. The case of resonant absorption will be discussed in a subsequent publication. The decrease in wave energy ( kinetic + magnetic ...

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Forward modeling of EUV and gyrosynchrotron emission from coronal plasmas with FoMo

Forward modeling of EUV and gyrosynchrotron emission from coronal plasmas with FoMo

... UV emission from optically thin coronal ...plasma density, temperature and velocity on a 3D ...the emission channels for synthetic AIA imaging ...gyrosynchrotron emission from plasmas ...

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Density Determinations and Various Methods to Measure

Density Determinations and Various Methods to Measure

... cylinder’s density is between that of aluminum and of brass, you should calculate a percent of aluminum that makes ...a density near that of Al, X should be near ...

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Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations

Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations

... of coronal loops, it is important that any proposed mod- els can be tested against the observed oscillatory ...plasma density and flux tube cross-sectional area (in- versely proportional to magnetic field ...

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Coronal loop density profile estimated by forward modelling of EUV intensity

Coronal loop density profile estimated by forward modelling of EUV intensity

... the density contrast and the layer ...the density contrast of coronal loops since the intensity contrast is also function of an unknown column ...the density contrast to be ...

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Resonant absorption in expanding coronal magnetic flux tubes with uniform density

Resonant absorption in expanding coronal magnetic flux tubes with uniform density

... the coronal volume, even in the absence of visible, dense, loop ...and coronal conditions at a single altitude will not fully determine the nature of MHD ...the density profile upon which they ...

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Chandra observations of coronal emission from the early G supergiants Alpha and Beta Aquarii

Chandra observations of coronal emission from the early G supergiants Alpha and Beta Aquarii

... of coronal X-rays from the early-G supergiants α Aquarii (HD209750: G2 Ib) and β Aquarii (HD204867: G0 ...faint emission at the location of β Aqr, now well sepa- rated from the stronger source to the SE ...

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DICHOTOMY OF GLOBAL CAPACITY DENSITY IN METRIC MEASURE SPACES

DICHOTOMY OF GLOBAL CAPACITY DENSITY IN METRIC MEASURE SPACES

... Key words and phrases. capacitarily stable collection, capacitary potential, capacity density, di- chotomy, metric space, Sobolev capacity, variational capacity. The first author was partially supported by JSPS ...

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Using Factual Density to Measure Informativeness of Web Documents

Using Factual Density to Measure Informativeness of Web Documents

... Consequently, we conclude that the factual density measure can be applied for adequate assessment of the informativeness of textual content on the Web. In future work, we plan to conduct similar experiments ...

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A Microblock Density-Based Similarity Measure for Graph Clustering

A Microblock Density-Based Similarity Measure for Graph Clustering

... similarity measure based on microblock density, which computes the similarity between a pair of vertices by calculating the densities of their common adjacent ...This measure extends the scope and ...

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Using Factual Density to Measure Informativeness of Web Documents

Using Factual Density to Measure Informativeness of Web Documents

... Assessment of information quality becomes increasingly important because nowadays deci- sion making is based on information from various sources that are sometimes unknown or of questionable reliability. Besides, a large ...

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Active region emission measure distributions and implications for nanoflare heating

Active region emission measure distributions and implications for nanoflare heating

... the emission measure (EM) in the core of active regions coronal loops is an important diagnostic of heating ...stressed coronal field to a near-potential state, the time taken to build up the ...

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Far-infrared HD emission as a measure of protoplanetary disk mass

Far-infrared HD emission as a measure of protoplanetary disk mass

... 2. Model The thermochemical code Dust and Lines (DALI) was used to calculate the line fluxes for the disk models (Bruderer et al. 2012; Bruderer 2013). This 2D physical-chemical code calcu- lates the thermal and chemical ...

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Broadening of the differential emission measure by multi shelled and turbulent loops

Broadening of the differential emission measure by multi shelled and turbulent loops

... The reconstructed DEM has a broad peak near the peak temper- ature of the plasma, perhaps caused by the lack of DEM resolu- tion. This is clearly reflected in the graph for its FWHM: its value is significantly larger ...

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Broadening of the differential emission measure by multi-shelled and turbulent loops

Broadening of the differential emission measure by multi-shelled and turbulent loops

... of density (top row), temperature (middle row) and DEM (bottom row) in the loop top cross section of the impulsively excited model, at the times specified in the title of each ...

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