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On Modeling Profiles instead of Values
[article]
2012
arXiv
pre-print
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Instead of maximum likelihood, which maximizes the probability of the ob served values, we propose a different estimate, the high-profile distribution, which maximizes the probability of the observed profile ...
, the high-profile and maximum-likelihood distributions are roughly the same, but when the number of symbols is large, the distributions differ, and high-profile better explains the data. ...
It is based on the simple premise that the underlying distribution should be estimated based not on the specific values observed, but only on the number of values appearing any given number of times. ...
arXiv:1207.4175v1
fatcat:bmczrtsv7bdsborsflg2pr7yxy
Model comparison for the density structure along solar prominence threads
[article]
2015
arXiv
pre-print
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period ratio values. ...
A Gaussian profile would require unrealistically large values of the density gradient parameter and a parabolic density distribution does not enable us to obtain well constrained posterior probability ...
We acknowledge financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) through projects AYA2011-22846 (Dynamics and Seismology of Solar Coronal Structures), AYA2014-55456-P ...
arXiv:1505.03448v1
fatcat:huq77lh2zfhu5csgfgaqvoyisu
Model comparison for the density structure along solar prominence threads
2015
Astronomy and Astrophysics
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period ratio values. ...
A Gaussian profile would require unrealistically large values of the density gradient parameter and a parabolic density distribution does not enable us to obtain well constrained posterior probability ...
We acknowledge financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) through projects AYA2011-22846 (Dynamics and Seismology of Solar Coronal Structures), AYA2014-55456-P ...
doi:10.1051/0004-6361/201525720
fatcat:rll53zyoa5d5hbki6tyjx7ok6q
Page 203 of Astronomy and Astrophysics Vol. 230, Issue 1
[page]
1990
Astronomy and Astrophysics
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These 3 restrictions above, can be combined in the following one: all profiles that have a maximum value of contrast less than 0.1 have been processed; we have taken a maximum value of 0.1 instead of zero ...
The influence of the background profile on the velocity values will be discussed in the next section.
5. Results and discussion 5.1. ...
Page 110 of Astronomy and Astrophysics Vol. 214, Issue 1-2
[page]
1989
Astronomy and Astrophysics
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best isotropic model yields x2 =4.79 for the fit to the surface brightness profile, instead of 72 = 2.20 for the best anisotropic model). ...
This is also true for models based on the assumption that the individual mass of such objects equals 2.0m, instead of 1.4m, and for models with m,, = 0.0, i.e., without heavy rem- nants at all. ...
ERRATUM: "ATMOSPHERIC RETRIEVAL ANALYSIS OF THE DIRECTLY IMAGED EXOPLANET HR 8799b" (2013, ApJ, 778, 97)
2013
Astrophysical Journal
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However, since one of our conclusions (which remains unchanged) is that UC models are marginally inferior to CF and IN ones, we report these numbers only for completeness. ...
For Figure 11 , the caption should read τ = 0.12 (instead of τ = 2). For Figure 18 , the caption should read τ = 0.12 and 0.37 for the IN and UC models, respectively (instead of τ = 2). ...
doi:10.1088/0004-637x/780/2/190
fatcat:q63to425pfgyjl7agkuecu4cqq
Single and joint statistics of ducting layer parameters determined from vertical profiles of atmospheric refractivity
2011
2011 XXXth URSI General Assembly and Scientific Symposium
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Vertical profiles of atmospheric refractivity measured on 150 m mast are fitted with a modified Webster duct model. Time series of duct model parameters are obtained with one minute resolution. ...
Empirical single and joint statistics of duct model parameters are determined from 7 month data. Interrelations between the duct parameters are discussed. ...
Instead, it should be taken as simply one parameter of (1) that in combination with the other four parameters models a particular vertical profile. ...
doi:10.1109/ursigass.2011.6050869
fatcat:jot7eakavff7rfvfjibexu6zri
Page 151 of Astronomy and Astrophysics Vol. 239, Issue 1-2
[page]
1990
Astronomy and Astrophysics
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The model with the index 5a differs from the model 5 only by the central value of the projected velocity dispersion, taken equal to 11.1 kms~‘ in model 5a instead of 10.1 kms~' in model 5; the model with ...
Depending on the model, the values obtained for the total mass of the cluster range from 0.70 to 1.55 10° Mo, with a mean total mass <M,,, > = 1.0+0.3 10° M.. ...
Profile shape parameterization of JET electron temperature and density profiles
1997
Nuclear Fusion
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2018 pre-print arXiv:1803.10895v1 fatcat:ynmedx24j5hqdp7t6luxgowahq
The temperature and density profiles of the Joint European Torus are parameterized using log-additive models in the control variables. ...
The L-mode normalized density shape depends primarily on the ratio of line average density, n̅, to the edge safety factor, q_95. As n̅/q_95 increases, the profile shape broadens. ...
If the effective charge is added, the PAR value is .0632, while using the line average density instead of Z ef f yields a worse value of .0640. ...
doi:10.1088/0029-5515/37/1/i08
fatcat:p24dux7sszea5grfx2h3vnkpwm
Dynamic extension for Ideal Kinematics
2022
Transportation Systems in Buildings
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This paper presents a new set of equations for modelling kinematic profiles using a combination of mathematical and computational techniques. ...
The implementation of these equations will extend the capabilities of the kinematic model to produce asymmetric and dynamic profiles. ...
ACKNOWLEDGEMENTS The authors acknowledge the work of Gabrielle Anderson and her research into the field of lift kinematics with multiple maximum velocities and with separate acceleration and deceleration ...
doi:10.14234/tsib.v4i1.163
fatcat:sv2itmjpczhrni3rnctdr7nnq4
Графова модель представлення профілів користувачів на стороні платформи DSP за допомогою засобів NoSQL бази даних Hbase
2015
Adaptivni Sistemi Avtomatičnogo Upravlinnâ
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Annotation: Success of Real-Time Bidding and advertising campaigns depends on building precise target audience profiles on Demand Side Platoform side. ...
This article addresses a data model to represent a large profile databases with subset of graph-based operations and corresponding mapping to modern NoSQL databases like HBASE. ...
Addressing that, master profiles, instead of having NULL-valued M AST ERID column, should be just suppressed, that speeds up the operation "Retrieve complete list of unique profiles". ...
doi:10.20535/1560-8956.27.2015.63433
fatcat:26jm5s7lkbhybcduuhlyhss7xq
The Tornadic Vortex Signature: An Update
2012
Weather and forecasting
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To understand this dilemma, the choice of vortex model and reflectivity profile is investigated. ...
It is found that the choice of vortex model does not have a significant effect on the simulation results. ...
profiles on the tornadic vortex signature. ...
doi:10.1175/waf-d-11-00111.1
fatcat:hbol4r6hijhodjg3n3vmcd3y2e
Optimizing self-consistent field theory block copolymer models with X-ray metrology
2018
Molecular Systems Design & Engineering
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Thus, the values found are instead more dependent on the interfacial width model used in relating and to than the pure SCFT model used. ...
The SCFT model (bottom) best fit results show both the SCFT density profile on the left and profile on the right. ...
doi:10.1039/c7me00098g
pmid:29892480
fatcat:ht3lw6ueo5b6pklufiwp57xekm
Page 860 of Astronomy and Astrophysics Vol. 274, Issue 3
[page]
1993
Astronomy and Astrophysics
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The 4—-SPOT STAR. a Reconstruction based on an (instead of 60° ). b Recon- struction based on an overestimated inclination value of 7 = 70
underestimated inclination value of 7 = 50
Fig. 9. ...
Reconstruction based on an underestimated limb darkening value of we = 0.3 (instead of 0.6)
ential rotation measurements) this defect does not constitute a serious problem.
4.4. ...
A meta-level specification and profile for AspectJ in UML
2007
Proceedings of the 10th international workshop on Aspect-oriented modeling - AOM '07
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Increasingly, calls for support of AOP on the software model level are being voiced. This paper addresses these calls by offering a meta-model of AspectJ in UML. ...
Moreover, the use of standard XMI based modelling allows the use of the profile in commercially available CASE tools and supports easy code generation. ...
Similarly, values of stereotype attributes will become values of tags when the profile is applied [25] . ...
doi:10.1145/1229375.1229379
fatcat:ayu7t36ewvd2zkujzn6dakqa7u
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