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Books on the topic 'Planetary Modeling'

Author: Grafiati
Published: 4 June 2021
Last updated: 15 February 2022

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1

Haider, S. A., Haider S. A, and Shyam Lal. Modeling of planetary atmospheres. Edited by Physical Research Laboratory (Ahmadābād, India). Delhi: Macmillan Publishers India, 2010.

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2

Parker, Robert G. Modeling, modal properties, and mesh stiffness variation instabilities of planetary gears. [Cleveland, Ohio]: National Aeronautics and Space Administration, Glenn Research Center, 2001.

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3

Borysow, Aleksandra. Modeling of collision induced absorption spectra of CO₂-CO₂ pairs for planetary atmosphere of Venus. [Washington, DC: National Aeronautics and Space Administration, 1995.

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4

Borysow, Aleksandra. Modeling of collision induced absorption spectra of CO₂-CO₂ pairs for planetary atmosphere of Venus. [Washington, DC: National Aeronautics and Space Administration, 1995.

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5

Kargel, J. S. (Jeffrey Stuart), 1958- and SpringerLink (Online service), eds. Cold Aqueous Planetary Geochemistry with FREZCHEM: From Modeling to the Search for Life at the Limits. Berlin, Heidelberg: Springer-Verlag, 2008.

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6

Lin, Yuh-Lang. Numerical modeling studies of wake vortex transport and evolution within the planetary boundary layer: FY94 July semi-annual report. Raleigh, NC: Dept. of Marine, Earth and Atmospheric Sciences, North Carolina State University, 1994.

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7

Haskin, Larry A. Analytical, experimental, and modelling studies of lunar and terrestrial rocks: Final report--summary of research, NASA grant no. NAGW-3343, Washington University fund #1041-59981. [Washington, DC: National Aeronautics and Space Administration, 1997.

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8

Manfrida, Roberto, and Daniele Contini, eds. Proceedings of Physmod 2003 International Workshop on Physical Modelling of Flow and Dispersion Phenomena. Florence: Firenze University Press, 2003. http://dx.doi.org/10.36253/88-8453-095-4.

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The various articles which make up this book concern both modelling (numerical and analytical) and experimental activities in relation to aspects of environmental fluid dynamics. Issues dealt with include the dispersion of pollutants in both urban and extra-urban areas, the effect of obstacles on the flow and dispersion in the turbulent boundary layer, and the simulation of the planetary boundary layer in proximity with the earth's surface. There is also a discussion of advanced issues which are also of interest in the sphere of urban planning, such as "wind comfort" and the effects of the shelter belt.
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9

Burlina, E. I︠A︡. Gorod, strana, planeta: Modeli gumanizma v khudozhestvennoiĭ kulʹture. Samara: Samarskiĭ Dom pechati, 1995.

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10

Hollingsworth, Jeffery L. Modeling of forced planetary waves in the Mars atmosphere. 1992.

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11

Constructing an advanced software tool for planetary atmospheric modeling. [Moffett Field, CA]: NASA, Ames Research Center, Artificial Intelligence Research Branch, 1990.

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12

L, Green James, and United States. National Aeronautics and Space Administration., eds. Modeling and inestigative stuides of Jovian low frequency emissions: Final report. Washington, DC: National Aeronautics and Space Administration, 1986.

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13

Agnor, Craig B. Modeling the late stage of planetary formation: An N-body approach. 1996.

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14

Agnor, Craig B. Modeling the late stage of planetary formation: An N-body approach. 1996.

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15

Heinsch, Faith Ann. Transportation and the atmospheric boundary layer: Progress in modeling feedback mechanisms. 1997.

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16

Proposal for constructing an advanced software tool for planetary atmospheric modeling. [Moffett Field, CA]: Ames Research Center, Artificial Intelligence Research Branch, 1990.

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17

United States. National Aeronautics and Space Administration., ed. Early differentiation of the moon: Experimental and modeling studies and experimental modeing studies of massive anorthosites, 3-1-89 - 8-31-94. [Washington, DC: National Aeronautics and Space Administration, 1994.

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18

Jewell, Gregory M. Modeling the mid-stage evolution of the protoplanetary cloud using a hybrid statistical/N-body simulator. 1996.

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19

Jewell, Gregory M. Modeling the mid-stage evolution of the protoplanetary cloud using a hybrid statistical/N-body simulator. 1996.

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20

Krishnamurti, T. N., H. S. Bedi, and V. M. Hardiker. An Introduction to Global Spectral Modeling. Oxford University Press, 1998. http://dx.doi.org/10.1093/oso/9780195094732.001.0001.

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This book is an indispensable guide to the methods used by nearly all major weather forecast centers in the United States, England, Japan, India, France, and Australia. Designed for senior-level undergraduates and first-year graduate students, the book provides an introduction to global spectral modeling. It begins with an introduction to elementary finite-difference methods and moves on towards the gradual description of sophisticated dynamical and physical models in spherical coordinates. Topics include computational aspects of the spectral transform method, the planetary boundary layer physics, the physics of precipitation processes in large-scale models, the radiative transfer including effects of diagnostic clouds and diurnal cycle, the surface energy balance over land and ocean, and the treatment of mountains. The discussion of model initialization includes the treatment of normal modes and physical processes, and the concluding chapter covers the spectral energetics as a diagnostic tool for model evaluation.
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21

Kargel, Jeffrey S., and Giles M. Marion. Cold Aqueous Planetary Geochemistry with FREZCHEM: From Modeling to the Search for Life at the Limits. Springer, 2010.

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22

Pal, Arya S., Kaplan Michael L, and United States. National Aeronautics and Space Administration., eds. Numerical modeling studies of wake vortex transport and evolution within the planetary boundary layer: FY94 July semi-annual report. Raleigh, NC: Dept. of Marine, Earth and Atmospheric Sciences, North Carolina State University, 1994.

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23

United States. National Aeronautics and Space Administration., ed. MHD modeling of the interaction of the solar wind with Venus: Final report, NASA grant no. NAGW-3779, SwRI project no. 15-6083. [San Antonio, Tex.]: Southwest Research Institute, Venus Data Analysis Program, 1996.

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24

United States. National Aeronautics and Space Administration., ed. MHD modeling of the interaction of the solar wind with Venus: Final report, NASA grant no. NAGW-3779, SwRI project no. 15-6083. [San Antonio, Tex.]: Southwest Research Institute, Venus Data Analysis Program, 1996.

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25

Numerical modeling studies of wake vortex transport and evolution within the planetary boundary layer: NASA grant NCC-1-188 : FY 97 annual report. [Washington, DC: National Aeronautics and Space Administration, 1998.

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26

Yuh-Lang, Lin, and United States. National Aeronautics and Space Administration., eds. Numerical modeling studies of wake vortex transport and evolution within the planetary boundary layer: NASA grant NCC-1-188 : FY 97 annual report. [Washington, DC: National Aeronautics and Space Administration, 1998.

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27

1935-, Lasker G. E., International Institute for Advanced Studies in Systems Research and Cybernetics., and International Conference on Systems Research, Informatics and Cybernetics (8th : 1996 : Baden-Baden, Germany), eds. Advances in sociocybernetics and human development: Dialogue of cultures, planetary thinking and cultural synergy, cross-cultural research methodology, policy development and implementation, promoting democratic reforms, population policy analysis, global problems and global knowledge, assumptive worlds and pseudo-environments formation, modeling interactions in human systems, measuring interactions of the economy and the environment, transitional processes in Central and Eastern Europe. Windsor, Ont: International Institute for Advanced Studies in Systems Research and Cybernetics, 1996.

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28

Tibaldi, Stefano, and Franco Molteni. Atmospheric Blocking in Observation and Models. Oxford University Press, 2018. http://dx.doi.org/10.1093/acrefore/9780190228620.013.611.

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The atmospheric circulation in the mid-latitudes of both hemispheres is usually dominated by westerly winds and by planetary-scale and shorter-scale synoptic waves, moving mostly from west to east. A remarkable and frequent exception to this “usual” behavior is atmospheric blocking. Blocking occurs when the usual zonal flow is hindered by the establishment of a large-amplitude, quasi-stationary, high-pressure meridional circulation structure which “blocks” the flow of the westerlies and the progression of the atmospheric waves and disturbances embedded in them. Such blocking structures can have lifetimes varying from a few days to several weeks in the most extreme cases. Their presence can strongly affect the weather of large portions of the mid-latitudes, leading to the establishment of anomalous meteorological conditions. These can take the form of strong precipitation episodes or persistent anticyclonic regimes, leading in turn to floods, extreme cold spells, heat waves, or short-lived droughts. Even air quality can be strongly influenced by the establishment of atmospheric blocking, with episodes of high concentrations of low-level ozone in summer and of particulate matter and other air pollutants in winter, particularly in highly populated urban areas.Atmospheric blocking has the tendency to occur more often in winter and in certain longitudinal quadrants, notably the Euro-Atlantic and the Pacific sectors of the Northern Hemisphere. In the Southern Hemisphere, blocking episodes are generally less frequent, and the longitudinal localization is less pronounced than in the Northern Hemisphere.Blocking has aroused the interest of atmospheric scientists since the middle of the last century, with the pioneering observational works of Berggren, Bolin, Rossby, and Rex, and has become the subject of innumerable observational and theoretical studies. The purpose of such studies was originally to find a commonly accepted structural and phenomenological definition of atmospheric blocking. The investigations went on to study blocking climatology in terms of the geographical distribution of its frequency of occurrence and the associated seasonal and inter-annual variability. Well into the second half of the 20th century, a large number of theoretical dynamic works on blocking formation and maintenance started appearing in the literature. Such theoretical studies explored a wide range of possible dynamic mechanisms, including large-amplitude planetary-scale wave dynamics, including Rossby wave breaking, multiple equilibria circulation regimes, large-scale forcing of anticyclones by synoptic-scale eddies, finite-amplitude non-linear instability theory, and influence of sea surface temperature anomalies, to name but a few. However, to date no unique theoretical model of atmospheric blocking has been formulated that can account for all of its observational characteristics.When numerical, global short- and medium-range weather predictions started being produced operationally, and with the establishment, in the late 1970s and early 1980s, of the European Centre for Medium-Range Weather Forecasts, it quickly became of relevance to assess the capability of numerical models to predict blocking with the correct space-time characteristics (e.g., location, time of onset, life span, and decay). Early studies showed that models had difficulties in correctly representing blocking as well as in connection with their large systematic (mean) errors.Despite enormous improvements in the ability of numerical models to represent atmospheric dynamics, blocking remains a challenge for global weather prediction and climate simulation models. Such modeling deficiencies have negative consequences not only for our ability to represent the observed climate but also for the possibility of producing high-quality seasonal-to-decadal predictions. For such predictions, representing the correct space-time statistics of blocking occurrence is, especially for certain geographical areas, extremely important.
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