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Journal articles on the topic 'Millenium simulation'

Author: Grafiati

Published: 4 June 2021

Last updated: 16 February 2022

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1

Ferry, D. K. "Simulation at the Start of the New Millenium: Crossing the Quantum-Classical Threshold." VLSI Design 13, no. 1-4 (2001): 155–61. http://dx.doi.org/10.1155/2001/59871.

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It is clear that continued scaling of semiconductor devices will bring us to a regime with gate lengths less than 50nm within another decade. The questions that must be addressed in simulation are difficult. Pushing to dimensional sizes such as this will probe the transition from classical to quantum transport, and there is no present approach to this regime that has proved effective. Contrary to the classical case in which electrons are negligibly small, the finite extent of the momentum space available to the electron set size limitations on the minimum wave packet–this is of the order of a

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2

Müller, Volker. "Color and magnitude dependence of galaxy clustering." Proceedings of the International Astronomical Union 11, S308 (2014): 293–94. http://dx.doi.org/10.1017/s1743921316010012.

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AbstractA quantitative study of the clustering properties of galaxies in the cosmic web as a function of absolute magnitude and colour is presented using the SDSS Data Release 7 galaxy redshift survey. We compare our results with mock galaxy samples obtained with four different semi-analytical models of galaxy formation imposed on the merger trees of the Millenium simulation.

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3

Chan, K. C., C. Y. Tang, and W. B. Lee. "Innovation and new technology for the new millenium." Journal of Materials Processing Technology 138, no. 1-3 (2003): 1. http://dx.doi.org/10.1016/s0924-0136(03)00030-x.

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4

Novrial and G. N. Ginting. "Evaluation Of Evacuation Routes And Fire Prevention Management On High Rise Buildings (Case Study: Millenium ICT Center, Medan)." Jurnal Koridor 10, no. 2 (2019): 109–15. http://dx.doi.org/10.32734/koridor.v10i2.1392.

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In the form of evacuation routes, safety handling must be prioritized especially in high-rise buildings. When the fire occurs, the most important thing apart from extinguishing the fire is to bring the occupants out of the building as soon as possible to prevent any casualties. It is necessary to take effective, efficient and integrated fire hazard prevention measures in a management system so that its implementation and renewal can follow the needs. This is also regulated in building regulations and is technically regulated in the Indonesian National Standard. Shopping center building is for

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Ratsimbazafy, A. L., C. M. Cress, S. L. Blyth, S. M. Crawford, E. A. Olivier, and K. J. van der Heyden. "Stellar populations in Luminous Red Galaxies: cosmic chronometers?" Proceedings of the International Astronomical Union 5, S262 (2009): 414–15. http://dx.doi.org/10.1017/s1743921310003480.

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AbstractThe expansion rate of the Universe can potentially be measured using age-dating of Luminous Red Galaxies (LRGs). Here, we explore the validity of the assumptions implicit in this method using LRGs identified in the Millenium Simulation (MS). We use stellar population modelling and spectral synthesis to estimate the errors on ages that can be expected and discuss optimization of such an experiment. We find that H(z) using simulated galaxies from MS can be recovered with high accuracy. Using single stellar populations (SSPs) to age-date LRGs is not sufficient but if the MS star formation

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6

Harley, Maria. "From Point to Sphere: Spatial Organization of Sound in Contemporary Music (after 1950)." Canadian University Music Review, no. 13 (February 22, 2013): 123–44. http://dx.doi.org/10.7202/1014300ar.

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In this study of spatial organization of sound, that is of "spatialization" in music, the term "spatial" refers to the three-dimensional performance space, not to pitch. "Spatialized music," distinct both from polychoral music and from musical theatre, means music with quasi-spatial structure defined by the composer in the score or in another medium of sound coding (digital or analog recording, specific software). Spatialization includes ensemble dispersion, movement of sounds, performers and audience, juxtaposition and interaction of real and virtual sound sources – every situation in which t

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7

Bothe, O., J. H. Jungclaus, D. Zanchettin, and E. Zorita. "Climate of the last millennium: ensemble consistency of simulations and reconstructions." Climate of the Past Discussions 8, no. 3 (2012): 2409–44. http://dx.doi.org/10.5194/cpd-8-2409-2012.

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Abstract. Are simulations and reconstructions of past climate and its variability comparable with each other? We assess if simulations and reconstructions are consistent under the paradigm of a statistically indistinguishable ensemble. Ensemble consistency is assessed for Northern Hemisphere mean temperature, Central European mean temperature and for global temperature fields for the climate of the last millennium. Reconstructions available for these regions are evaluated against the simulation data from the community simulations of the climate of the last millennium performed at the Max Planc

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8

González-Rouco, J. F., H. Beltrami, E. Zorita, and M. B. Stevens. "Borehole climatology: a discussion based on contributions from climate modeling." Climate of the Past Discussions 4, no. 1 (2008): 1–80. http://dx.doi.org/10.5194/cpd-4-1-2008.

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Abstract. Progress in understanding climate variability through the last millennium leans on simulation and reconstruction efforts. Exercises blending both approaches present a great potential for answering questions relevant both for the simulation and reconstruction of past climate, and depend on the specific peculiarities of proxies and methods involved in climate reconstructions, as well as on the realism and limitations of model simulations. This paper explores research specifically related to paleoclimate modeling and borehole climatology as a branch of climate reconstruction that has co

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González-Rouco, J. F., H. Beltrami, E. Zorita, and M. B. Stevens. "Borehole climatology: a discussion based on contributions from climate modeling." Climate of the Past 5, no. 1 (2009): 97–127. http://dx.doi.org/10.5194/cp-5-97-2009.

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Abstract. Progress in understanding climate variability through the last millennium leans on simulation and reconstruction efforts. Exercises blending both approaches present a great potential for answering questions relevant both for the simulation and reconstruction of past climate, and depend on the specific peculiarities of proxies and methods involved in climate reconstructions, as well as on the realism and limitations of model simulations. This paper explores research specifically related to paleoclimate modeling and borehole climatology as a branch of climate reconstruction that has co

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10

Ljungqvist, Fredrik Charpentier, Qiong Zhang, Gudrun Brattström, et al. "Centennial-Scale Temperature Change in Last Millennium Simulations and Proxy-Based Reconstructions." Journal of Climate 32, no. 9 (2019): 2441–82. http://dx.doi.org/10.1175/jcli-d-18-0525.1.

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AbstractSystematic comparisons of proxy-based reconstructions and climate model simulations of past millennium temperature variability offer insights into climate sensitivity and feedback mechanisms, besides allowing model evaluation independently from the period covered by instrumental data. Such simulation–reconstruction comparisons can help to distinguish more skillful models from less skillful ones, which may subsequently help to develop more reliable future projections. This study evaluates the low-frequency simulation–reconstruction agreement within the past millennium through assessing

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11

Wang, Yi-Han, Nathan W. C. Leigh, Alberto Sesana, and Rosalba Perna. "The cosmological distribution of compact object mergers from dynamical interactions with SMBH binaries." Monthly Notices of the Royal Astronomical Society 490, no. 2 (2019): 2627–47. http://dx.doi.org/10.1093/mnras/stz2780.

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ABSTRACT We combine sophisticated high-precision scattering experiments, together with results from the Millenium-II simulation, to compute the cosmic merger rate of bound compact object (CO) binaries dynamically interacting with supermassive black hole binaries (SMBHBs). We consider binaries composed of white dwarfs (WDs), neutron stars (NSs), and black holes (BHs). The overall merger rates for WD–WD, NS–NS, BH–BH, BH–NS binaries, and EBBH (eccentric binaries of BHs) from redshift ∼5 are found to be $4.32\times 10^3\, \mathrm{yr}^{-1}(5.93\times 10^2\, \mathrm{yr}^{-1}$ for Type Ia SNe), $82.

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12

Henriksson, S. V., P. Räisänen, J. Silen, H. Järvinen, and A. Laaksonen. "Power-law behavior in millennium climate simulations." Earth System Dynamics Discussions 3, no. 1 (2012): 391–416. http://dx.doi.org/10.5194/esdd-3-391-2012.

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Abstract. Using a method of discrete Fourier transform with varying starting point and length of time window and the long time series provided by millennium Earth System Model simulations, we get good fits to power laws between two characteristic oscillatory timescales of the model climate: multidecadal (50–80 yr) and El Nino (3–6 yr) timescales. For global mean temperature, we fit β ~ 0.35 in a relation S(f) ~ f−β in a simulation without external climate forcing and β over 0.7 in a simulation with external forcing included. We also fit a power law with β ~ 8 to the narrow frequency range betw

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13

Lehner, F., F. Joos, C. C. Raible, et al. "Climate and carbon cycle dynamics in a CESM simulation from 850 to 2100 CE." Earth System Dynamics 6, no. 2 (2015): 411–34. http://dx.doi.org/10.5194/esd-6-411-2015.

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Abstract. Under the protocols of phase 3 of the Paleoclimate Modelling Intercomparison Project, a number of simulations were produced that provide a range of potential climate evolutions from the last millennium to the end of the current century. Here, we present the first simulation with the Community Earth System Model (CESM), which includes an interactive carbon cycle, that covers the last millennium. The simulation is continued to the end of the twenty-first century. Besides state-of-the-art forcing reconstructions, we apply a modified reconstruction of total solar irradiance to shed light

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14

Bothe, O., J. H. Jungclaus, D. Zanchettin, and E. Zorita. "Climate of the last millennium: ensemble consistency of simulations and reconstructions." Climate of the Past 9, no. 3 (2013): 1089–110. http://dx.doi.org/10.5194/cp-9-1089-2013.

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Abstract. Are simulations and reconstructions of past climate and its variability consistent with each other? We assess the consistency of simulations and reconstructions for the climate of the last millennium under the paradigm of a statistically indistinguishable ensemble. In this type of analysis, the null hypothesis is that reconstructions and simulations are statistically indistinguishable and, therefore, are exchangeable with each other. Ensemble consistency is assessed for Northern Hemisphere mean temperature, Central European mean temperature and for global temperature fields. Reconstr

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15

Gómez-Navarro, J. J., J. P. Montávez, S. Jerez, et al. "A regional climate simulation over the Iberian Peninsula for the last millennium." Climate of the Past Discussions 6, no. 5 (2010): 2071–116. http://dx.doi.org/10.5194/cpd-6-2071-2010.

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Abstract. In this study we present a regional paleoclimate simulation which covers the last millennium over the Iberian Peninsula (IP) with an unprecedented resolution of 30 km. The simulation was performed with a climate version of the mesoscale model MM5 coupled to the global model ECHO-G. Both experiments were driven by the same reconstructions of several external factors. The high spatial resolution of the regional model allows to simulate realistically many aspects of the climate in the IP when comparing the simulation to an observational data set in a reference period (1961–1990). Althou

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Gómez-Navarro, J. J., J. P. Montávez, S. Jerez, et al. "A regional climate simulation over the Iberian Peninsula for the last millennium." Climate of the Past 7, no. 2 (2011): 451–72. http://dx.doi.org/10.5194/cp-7-451-2011.

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Abstract. A high-resolution (30 km) regional paleoclimate simulation of the last millennium over the Iberian Peninsula (IP) is presented. The simulation was performed with a climate version of the mesoscale model MM5 driven by the global model ECHO-G. Both models were driven by the same reconstructions of several external forcing factors. The high spatial resolution of the regional model allows climatologists to realistically simulate many aspects of the climate in the IP, as compared to an observational data set in the reference period 1961–1990. Although the spatial-averaged values developed

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17

Díaz-Giménez, E., A. Zandivarez, R. Proctor, C. Mendes de Oliveira, and L. R. Abramo. "Fossil groups in the Millennium simulation." Astronomy & Astrophysics 527 (February 10, 2011): A129. http://dx.doi.org/10.1051/0004-6361/201015347.

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18

Kanagusuku, María José, Eugenia Díaz-Giménez, and Ariel Zandivarez. "Fossil groups in the Millennium simulation." Astronomy & Astrophysics 586 (January 25, 2016): A40. http://dx.doi.org/10.1051/0004-6361/201527269.

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19

Díaz-Giménez, E., H. Muriel, and C. Mendes de Oliveira. "Fossil groups in the Millennium Simulation." Astronomy & Astrophysics 490, no. 3 (2008): 965–73. http://dx.doi.org/10.1051/0004-6361:200809760.

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20

Sundberg, R., A. Moberg, and A. Hind. "Statistical framework for evaluation of climate model simulations by use of climate proxy data from the last millennium – Part 1: Theory." Climate of the Past 8, no. 4 (2012): 1339–53. http://dx.doi.org/10.5194/cp-8-1339-2012.

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Abstract. A statistical framework for comparing the output of ensemble simulations from global climate models with networks of climate proxy and instrumental records has been developed, focusing on near-surface temperatures for the last millennium. This framework includes the formulation of a joint statistical model for proxy data, instrumental data and simulation data, which is used to optimize a quadratic distance measure for ranking climate model simulations. An essential underlying assumption is that the simulations and the proxy/instrumental series have a shared component of variability t

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21

Hind, A., A. Moberg, and R. Sundberg. "Statistical framework for evaluation of climate model simulations by use of climate proxy data from the last millennium." Climate of the Past Discussions 8, no. 1 (2012): 263–320. http://dx.doi.org/10.5194/cpd-8-263-2012.

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Abstract. A statistical framework for comparing the output of ensemble simulations from global climate models with networks of climate proxy and instrumental records is developed, focusing on near-surface temperatures for the last millennium. This framework includes the formulation of a joint statistical model for proxy data, instrumental data and simulation data, which is used to optimize a quadratic distance measure for ranking climate model simulations. An essential underlying assumption is that the simulations and the proxy/instrumental series have a shared component of variability that is

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22

Hameau, Angélique, Juliette Mignot, and Fortunat Joos. "Assessment of time of emergence of anthropogenic deoxygenation and warming: insights from a CESM simulation from 850 to 2100 CE." Biogeosciences 16, no. 8 (2019): 1755–80. http://dx.doi.org/10.5194/bg-16-1755-2019.

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Abstract. Marine deoxygenation and anthropogenic ocean warming are observed and projected to intensify in the future. These changes potentially impact the functions and services of marine ecosystems. A key question is whether marine ecosystems are already or will soon be exposed to environmental conditions not experienced during the last millennium. Using a forced simulation with the Community Earth System Model (CESM) over the period 850 to 2100, we find that anthropogenic deoxygenation and warming in the thermocline exceeded natural variability in, respectively, 60 % and 90 % of total ocean

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23

Colose, C. M., A. N. LeGrande, and M. Vuille. "The influence of tropical volcanic eruptions on the climate of South America during the last millennium." Climate of the Past Discussions 11, no. 4 (2015): 3375–424. http://dx.doi.org/10.5194/cpd-11-3375-2015.

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Abstract. Currently, little is known on how volcanic eruptions impact large-scale climate phenomena such as paleo-ITCZ position or South American summer monsoon behavior. In this paper, an analysis of observations and model simulations is employed to assess the influence of large volcanic eruptions on the climate of South America. This problem is considered both for historically recent volcanic episodes, for which more comprehensive global observations exist, as well as reconstructed volcanic events for the period 850 C.E. to present that are incorporated into the NASA GISS ModelE2-R simulatio

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24

Lehner, F., F. Joos, C. C. Raible, et al. "Climate and carbon cycle dynamics in a CESM simulation from 850–2100 CE." Earth System Dynamics Discussions 6, no. 1 (2015): 351–406. http://dx.doi.org/10.5194/esdd-6-351-2015.

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Abstract. Under the protocols of the Paleoclimate and Coupled Modelling Intercomparison Projects a number of simulations were produced that provide a range of potential climate evolutions from the last millennium to the end of the current century. Here, we present the first simulation with the Community Earth System Model (CESM), which includes an interactive carbon cycle, that continuously covers the last millennium, the historical period, and the twenty-first century. Besides state-of-the-art forcing reconstructions, we apply a modified reconstruction of total solar irradiance to shed light

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Darg, D. W., S. Kaviraj, C. J. Lintott, et al. "Galaxy Zoo: multimergers and the Millennium Simulation." Monthly Notices of the Royal Astronomical Society 416, no. 3 (2011): 1745–55. http://dx.doi.org/10.1111/j.1365-2966.2011.18964.x.

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26

Wilking, P., R. Röseler, and P. Schneider. "Constrained correlation functions from the Millennium Simulation." Astronomy & Astrophysics 582 (October 2015): A107. http://dx.doi.org/10.1051/0004-6361/201525906.

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27

Pyrina, Maria, Eduardo Moreno-Chamarro, Sebastian Wagner, and Eduardo Zorita. "Surface and Tropospheric Response of North Atlantic Summer Climate from Paleoclimate Simulations of the Past Millennium." Atmosphere 12, no. 5 (2021): 568. http://dx.doi.org/10.3390/atmos12050568.

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We investigate the effects of solar forcing on the North Atlantic (NA) summer climate, in climate simulations with Earth System Models (ESMs), over the preindustrial past millennium (AD 850–1849). We use one simulation and a four-member ensemble performed with the MPI-ESM-P and CESM-LME models, respectively, forced only by low-scaling variations in Total Solar Irradiance (TSI). We apply linear methods (correlation and regression) and composite analysis to estimate the NA surface and tropospheric climatic responses to decadal solar variability. Linear methods in the CESM ensemble indicate a wea

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28

Gómez-Navarro, J. J., J. P. Montávez, P. Jiménez-Guerrero, et al. "Internal and external variability in regional simulations of the Iberian Peninsula climate over the last millennium." Climate of the Past 8, no. 1 (2012): 25–36. http://dx.doi.org/10.5194/cp-8-25-2012.

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Abstract. In this study we analyse the role of internal variability in regional climate simulations through a comparison of two regional paleoclimate simulations for the last millennium. They share the same external forcings and model configuration, differing only in the initial condition used to run the driving global model simulation. A comparison of these simulations allows us to study the role of internal variability in climate models at regional scales, and how it affects the long-term evolution of climate variables such as temperature and precipitation. The results indicate that, althoug

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29

Servonnat, J., P. Yiou, M. Khodri, D. Swingedouw, and S. Denvil. "Influence of solar variability, CO<sub>2</sub> and orbital forcing between 1000 and 1850 AD in the IPSLCM4 model." Climate of the Past 6, no. 4 (2010): 445–60. http://dx.doi.org/10.5194/cp-6-445-2010.

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Abstract. Studying the climate of the last millennium gives the possibility to deal with a relatively well-documented climate essentially driven by natural forcings. We have performed two simulations with the IPSLCM4 climate model to evaluate the impact of Total Solar Irradiance (TSI), CO2 and orbital forcing on secular temperature variability during the preindustrial part of the last millennium. The Northern Hemisphere (NH) temperature of the simulation reproduces the amplitude of the NH temperature reconstructions over the last millennium. Using a linear statistical decomposition we evaluate

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Servonnat, J., P. Yiou, M. Khodri, D. Swingedouw, and S. Denvil. "Influence of solar variability, CO<sub>2</sub> and orbital forcing during the last millennium in the IPSLCM4 model." Climate of the Past Discussions 6, no. 2 (2010): 421–60. http://dx.doi.org/10.5194/cpd-6-421-2010.

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Abstract. Studying the climate of the last millennium gives the possibility to deal with a relatively well-documented climate essentially driven by natural forcings. We have performed two simulations with the IPSLCM4 climate model to evaluate the impact of Total Solar Irradiance (TSI), CO2 and orbital forcing on secular temperature variability during the preindustrial part of the last millennium. The Northern Hemisphere (NH) temperature of the simulation reproduces the amplitude of the NH temperature reconstructions over the last millennium. Using a linear statistical decomposition we evaluate

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31

Gómez-Navarro, J. J., J. P. Montávez, P. Jiménez-Guerrero, et al. "Internal and external variability in regional simulations of the Iberian Peninsula climate over the last millennium." Climate of the Past Discussions 7, no. 4 (2011): 2579–607. http://dx.doi.org/10.5194/cpd-7-2579-2011.

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Abstract. In this study we analyse the role of internal variability in regional climate simulations through a comparison of two regional paleoclimate simulations for the last millennium. They share the same external forcings and model configuration, differing only in the initial condition used to run the driving global model simulation. A comparison of these simulations allows us to study the role of internal variability in climate models at regional scales, and how it affects the long-term evolution of climate variables such as temperature and precipitation. The results indicate that, althoug

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32

Korty, Robert L., Suzana J. Camargo, and Joseph Galewsky. "Variations in Tropical Cyclone Genesis Factors in Simulations of the Holocene Epoch." Journal of Climate 25, no. 23 (2012): 8196–211. http://dx.doi.org/10.1175/jcli-d-12-00033.1.

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Abstract The thermodynamic factors related to tropical cyclone genesis are examined in several simulations of the middle part of the Holocene epoch when the precession of Earth’s orbit altered the seasonal distribution of solar radiation and in one transient simulation of the millennium preceding the industrial era. The thermodynamic properties most crucial for genesis display a broad stability across both periods, although both orbital variations during the mid-Holocene (MH) 6000 years ago (6ka) and volcanic eruptions in the transient simulation have detectable effects. It is shown that the d

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33

RAOUF, MOJTABA, and HABIB G. KHOSROSHAHI. "AGE DATING GALAXY GROUPS IN THE MILLENNIUM SIMULATION." Publications of The Korean Astronomical Society 30, no. 2 (2015): 363–65. http://dx.doi.org/10.5303/pkas.2015.30.2.363.

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Smith, Alex, Shaun Cole, Carlton Baugh, et al. "A lightcone catalogue from the Millennium-XXL simulation." Monthly Notices of the Royal Astronomical Society 470, no. 4 (2017): 4646–61. http://dx.doi.org/10.1093/mnras/stx1432.

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Cohn, J. D., A. E. Evrard, M. White, D. Croton, and E. Ellingson. "Red-sequence cluster finding in the Millennium Simulation." Monthly Notices of the Royal Astronomical Society 382, no. 4 (2007): 1738–50. http://dx.doi.org/10.1111/j.1365-2966.2007.12479.x.

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36

Seeger, P. A., L. L. Daemen, T. G. Thelliez, and R. P. Hjelm. "Neutron instrument simulations in the next millennium." Physica B: Condensed Matter 283, no. 4 (2000): 433–35. http://dx.doi.org/10.1016/s0921-4526(00)00382-3.

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37

Kay, Scott T., Michael W. Peel, C. J. Short, et al. "Sunyaev-Zel’dovich clusters in Millennium gas simulations." Monthly Notices of the Royal Astronomical Society 422, no. 3 (2012): 1999–2023. http://dx.doi.org/10.1111/j.1365-2966.2012.20623.x.

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38

Smole, Majda, Miroslav Micic, and Nemanja Martinović. "SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations." Monthly Notices of the Royal Astronomical Society 451, no. 2 (2015): 1964–72. http://dx.doi.org/10.1093/mnras/stv1065.

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39

Rojas, Maisa, Paola A. Arias, Valentina Flores-Aqueveque, Anji Seth, and Mathias Vuille. "The South American monsoon variability over the last millennium in climate models." Climate of the Past 12, no. 8 (2016): 1681–91. http://dx.doi.org/10.5194/cp-12-1681-2016.

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Abstract. In this paper we assess South American monsoon system (SAMS) variability in the last millennium as depicted by global coupled climate model simulations. High-resolution proxy records for the South American monsoon over this period show a coherent regional picture of a weak monsoon during the Medieval Climate Anomaly and a stronger monsoon during the Little Ice Age (LIA). Due to the small external forcing during the past 1000 years, model simulations do not show very strong temperature anomalies over these two specific periods, which in turn do not translate into clear precipitation a

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40

Roldán-Gómez, Pedro José, Jesús Fidel González-Rouco, Camilo Melo-Aguilar, and Jason E. Smerdon. "Dynamical and hydrological changes in climate simulations of the last millennium." Climate of the Past 16, no. 4 (2020): 1285–307. http://dx.doi.org/10.5194/cp-16-1285-2020.

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Abstract. Simulations of climate of the last millennium (LM) show that external forcing had a major contribution to the evolution of temperatures; warmer and colder periods like the Medieval Climate Anomaly (MCA; ca. 950–1250 CE) and the Little Ice Age (LIA; ca. 1450–1850 CE) were critically influenced by changes in solar and volcanic activity. Even if this influence is mainly observed in terms of temperatures, evidence from simulations and reconstructions shows that other variables related to atmospheric dynamics and hydroclimate were also influenced by external forcing over some regions. In

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Rojas, M., P. A. Arias, V. Flores-Aqueveque, A. Seth, and M. Vuille. "The South American Monsoon Variability over the Last Millennium in CMIP5/PMIP3 simulations." Climate of the Past Discussions 11, no. 6 (2015): 5651–81. http://dx.doi.org/10.5194/cpd-11-5651-2015.

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Abstract. In this paper we assess South American Monsoon System (SAMS) variability throughout the Last Millennium as depicted by the Coupled Modelling Intercomparison Project version 5/Paleo Modelling Intercomparison Project version 3 (CMIP5/PMIP3) simulations. High-resolution proxy records for the South American monsoon over this period show a coherent regional picture of a weak monsoon during the Medieval Climate Anomaly period and a stronger monsoon during the Little Ice Age (LIA). Due to the small forcing during the past 1000 years, CMIP5/PMIP3 model simulations do not show very strong tem

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42

Landrum, Laura, Bette L. Otto-Bliesner, Eugene R. Wahl, et al. "Last Millennium Climate and Its Variability in CCSM4." Journal of Climate 26, no. 4 (2013): 1085–111. http://dx.doi.org/10.1175/jcli-d-11-00326.1.

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Abstract An overview of a simulation referred to as the “Last Millennium” (LM) simulation of the Community Climate System Model, version 4 (CCSM4), is presented. The CCSM4 LM simulation reproduces many large-scale climate patterns suggested by historical and proxy-data records, with Northern Hemisphere (NH) and Southern Hemisphere (SH) surface temperatures cooling to the early 1800s Common Era by ~0.5°C (NH) and ~0.3°C (SH), followed by warming to the present. High latitudes of both hemispheres show polar amplification of the cooling from the Medieval Climate Anomaly (MCA) to the Little Ice Ag

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Araya-Araya, Pablo, Marcelo C. Vicentin, Laerte Sodré, Roderik A. Overzier, and Hector Cuevas. "Protocluster detection in simulations of HSC–SSP and the 10-yr LSST forecast, using PCcones." Monthly Notices of the Royal Astronomical Society 504, no. 4 (2021): 5054–73. http://dx.doi.org/10.1093/mnras/stab1133.

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ABSTRACT The progenitors of present-day galaxy clusters give important clues about the evolution of the large-scale structure, cosmic mass assembly, and galaxy evolution. Simulations are a major tool for these studies since they are used to interpret observations. In this work, we introduce a set of ‘protocluster-light-cones’, dubbed PCcones. They are mock galaxy catalogues generated from the Millennium Simulation with the L-GALAXIES semi-analytic model. These light-cones were constructed by placing a desired structure at the redshift of interest in the centre of the cone. This approach allows

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Boylan-Kolchin, Michael, Volker Springel, Simon D. M. White, Adrian Jenkins, and Gerard Lemson. "Resolving cosmic structure formation with the Millennium-II Simulation." Monthly Notices of the Royal Astronomical Society 398, no. 3 (2009): 1150–64. http://dx.doi.org/10.1111/j.1365-2966.2009.15191.x.

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Nurmi, P., P. Heinämäki, T. Sepp, et al. "Groups in the Millennium Simulation and in SDSS DR7." Monthly Notices of the Royal Astronomical Society 436, no. 1 (2013): 380–94. http://dx.doi.org/10.1093/mnras/stt1571.

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Huang, Grace C., James A. Gordon, and Richard M. Schwartzstein. "Millennium Conference 2005 on Medical Simulation: A Summary Report." Simulation in Healthcare: The Journal of the Society for Simulation in Healthcare 2, no. 2 (2007): 88–95. http://dx.doi.org/10.1097/sih.0b013e318053e066.

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Sales, L. V., J. F. Navarro, D. G. Lambas, S. D. M. White, and D. J. Croton. "Satellite galaxies and fossil groups in the Millennium Simulation." Monthly Notices of the Royal Astronomical Society 382, no. 4 (2007): 1901–16. http://dx.doi.org/10.1111/j.1365-2966.2007.12507.x.

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Safonova, Sasha, Peder Norberg, and Shaun Cole. "Rosella: a mock catalogue from the P-Millennium simulation." Monthly Notices of the Royal Astronomical Society 505, no. 1 (2021): 325–38. http://dx.doi.org/10.1093/mnras/stab1286.

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ABSTRACT The scientific exploitation of the Dark Energy Spectroscopic Instrument Bright Galaxy Survey (DESI BGS) data requires the construction of mocks with galaxy population properties closely mimicking those of the actual DESI BGS targets. We create a high-fidelity mock galaxy catalogue, including information about galaxies and their host dark matter subhaloes. The mock catalogue uses subhalo abundance matching with scatter to populate the P-Millennium N-body simulation with galaxies at the median BGS redshift of ∼0.2, using formation redshift information to assign 0.1(g − r) rest-frame col

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Moberg, A., R. Sundberg, H. Grudd, and A. Hind. "Statistical framework for evaluation of climate model simulations by use of climate proxy data from the last millennium – Part 3: Practical considerations, relaxed assumptions, and using tree-ring data to address the amplitude of solar forcing." Climate of the Past 11, no. 3 (2015): 425–48. http://dx.doi.org/10.5194/cp-11-425-2015.

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Abstract. A statistical framework for evaluation of climate model simulations by comparison with climate observations from instrumental and proxy data (part 1 in this series) is improved by the relaxation of two assumptions. This allows autocorrelation in the statistical model for simulated internal climate variability and enables direct comparison of two alternative forced simulations to test whether one fits the observations significantly better than the other. The extended framework is applied to a set of simulations driven with forcings for the pre-industrial period 1000–1849 CE and 15 tre

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Widmann, Martin, and Simon FB Tett. "Simulating the Climate of the Last Millennium." PAGES news 11, no. 2-3 (2003): 21–23. http://dx.doi.org/10.22498/pages.11.2-3.21.

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