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280 results for “MESA”
FIGURES 10–19. Adelosgryllus similis n in Two new species of crickets Adelosgryllus Mesa & Zefa, 2004 (Orthoptera, Grylloidea, Phalangopsidae) from the Araripe-Apodi National Forest, State of Ceará, Brazil
FIGURES 10–19. Adelosgryllus similis n. sp., appendages. 10—leg I, inner view; 11—leg II, inner view; 12—leg III, inner view; 13—leg I, outer view; 14—leg II, outer view; 15—leg III, outer view; 16—auditory tympanum, inner view, arrow = filiform bristle; 17—tibia III, subapical spurs (S.S) and apical spurs (a, b, c, d, e, f, g); 18—antennae, dorsal; 19—cerci, dorsal.
FIGURES 39–46. Adelosgryllus cruscastaneus n in Two new species of crickets Adelosgryllus Mesa & Zefa, 2004 (Orthoptera, Grylloidea, Phalangopsidae) from the Araripe-Apodi National Forest, State of Ceará, Brazil
FIGURES 39–46. Adelosgryllus cruscastaneus n. sp. 39—holotype, habitus dorsal view; 40—holotype, habitus ventral view; 41—holotype, habitus lateral view; 42—paratype, head, frontal view; 43—holotype, head and pronotum, dorsal view; 44— holotype, head and pronotum, lateral view; 45—holotype, supranal plate, dorsal view; 46—holotype, subgenital plate, ventral view.
FIGURES 47–55. Adelosgryllus cruscastaneus n in Two new species of crickets Adelosgryllus Mesa & Zefa, 2004 (Orthoptera, Grylloidea, Phalangopsidae) from the Araripe-Apodi National Forest, State of Ceará, Brazil
FIGURES 47–55. Adelosgryllus cruscastaneus n. sp., paratype legs I to III. 47—Leg I, inner view; 48—Leg II, inner view; 49—Leg III, inner view; 50—Leg I, outer view; 51—Leg II, outer view; 52—Leg III, outer view; 53—inner auditory tympanum, filiforme bristle (arrow); 54—tibia III, inner apical spurs a, b, c and d, and outer apical spurs e, f and g; 55—tibia III inner and outer subapical spurs (S.S), and tarsomeres.
Input files and data for paper "Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation"
<p>This entry contains input files to reproduce the results of the paper:</p> <p>Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation.</p> <p>Each zip archive corresponds to a section of the paper, and includes README files in ASCII format with a description. Raw output data and plotting tools are also provided for some of the results.</p>
Exploring Stellar Evolution Models of sdB Stars using MESA
<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2015ApJ...806..178S">Exploring Stellar Evolution Models of sdB Stars using MESA</a></p>
Evolutionary Analysis of Gaseous Sub-Neptune-mass Planets with MESA
<p>MESA work directory, data, and ruby scripts associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2016ApJ...831..180C">Evolutionary Analysis of Gaseous Sub-Neptune-mass Planets with MESA</a></p>
MESA files for "She's Got Her Mother's Hair: End-to-End Collapsar Simulations Unveil the Origin of Black Holes' Magnetic Field"
<p>MESA input files, output, and scripts to reproduce Fig. 1 and the appendix figure in <a href="https://ui.adsabs.harvard.edu/abs/2024arXiv240716745G/abstract">Gottlieb, Renzo, et al. 2024</a><br><br></p>
Anemometer data from NSF NCAR Mesa Lab
<p>WXT instrument Sep 24,1996 through March 25, 2024, 5 minute data, unfiltered data, netcdf, from EOL , NSF NCAR</p> <p>Gill instrument Nov 29, 2021- March 25, 2024, 1 minute data, unfiltered data, netcdf, from EOL, NSF NCAR</p> <p>BAMS: Earth, wind and fire: Are Boulder’s hurricane-force downslope winds changing? Authors: Gerald A. Meehl*, Christine A. Shields, Brendan M. Myers, McKenzie L. Larson, Dale Durran, Muntaha Pasha, Annareli Morales, Aneesh Subramanian, Andrew C. Winters, Paul Schlatter, and Morris Weisman</p>
FIGURE 15 in Eleventh Annual Report of Historic Properties at the Phoenix-Mesa Gateway Airport, Mesa, Arizona
FIGURE 15. Brevipalpus phoenicis female dorsum, venter and deutonymph (after Baker & Tuttle 1987).
FIGURE 36. A in Eleventh Annual Report of Historic Properties at the Phoenix-Mesa Gateway Airport, Mesa, Arizona
FIGURE 36. A) Phyllotetranychus aegyptium female dorsum (after Sayed 1938); B) Phyllotetranychus romaine female dorsum and palp (after Pritchard & Baker 1958).
FIGURE 33 in Eleventh Annual Report of Historic Properties at the Phoenix-Mesa Gateway Airport, Mesa, Arizona
FIGURE 33. Crossipalpus verticillatae female dorsum, venter of gnathosoma and palpi (after Smiley et al. 1996).
FIGURE 27 in Eleventh Annual Report of Historic Properties at the Phoenix-Mesa Gateway Airport, Mesa, Arizona
FIGURE 27. Obdulia tamaricis female dorsum (original), venter and palps (after Pritchard & Baker 1958).
FIGURE 3.2 in Diversity of Leguminosae in the Chapada das Mesas National Park, Maranhão, Brazil: new occurrences for Maranhão and the Brazilian Cerrado
FIGURE 3.2 (Continued) Diversity of Leguminosae from Chapada das Mesas National Park, Maranhão, Brazil.
FIGURE 3.3 in Diversity of Leguminosae in the Chapada das Mesas National Park, Maranhão, Brazil: new occurrences for Maranhão and the Brazilian Cerrado
FIGURE 3.3 (Continued) Diversity of Leguminosae from Chapada das Mesas National Park, Maranhão, Brazil.
FIGURE 4 in Diversity of Leguminosae in the Chapada das Mesas National Park, Maranhão, Brazil: new occurrences for Maranhão and the Brazilian Cerrado
FIGURE 4. Distribution of genera and species according to Subfamilies of Leguminosae recorded for Chapada das Mesas National Park, Maranhão, Brazil.
FIGURE 2 in Diversity of Leguminosae in the Chapada das Mesas National Park, Maranhão, Brazil: new occurrences for Maranhão and the Brazilian Cerrado
FIGURE 2. Vegetation diversity of Chapada das Mesas National Park. A. and B. Canopy view of Cerradão vegetation; C. and D. Cerrado sensu stricto areas; E. and F. Waterfalls associated with gallery forests. Image authors: A-D: Guilherme Silva; E-F: Regigláucia Rodrigues.
FIGURE 3.4 in Diversity of Leguminosae in the Chapada das Mesas National Park, Maranhão, Brazil: new occurrences for Maranhão and the Brazilian Cerrado
FIGURE 3.4 (Continued) Diversity of Leguminosae from Chapada das Mesas National Park, Maranhão, Brazil.
FIGURE 6 in Diversity of Leguminosae in the Chapada das Mesas National Park, Maranhão, Brazil: new occurrences for Maranhão and the Brazilian Cerrado
FIGURE 6. Distribution of life habits of Leguminosae species recorded for Chapada das Mesas National Park, Maranhão, Brazil.
Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure
<p>We update the capabilities of the open-knowledge software instrument Modules for Experiments in Stellar Astrophysics (MESA). The new auto_diff module implements automatic differentiation in MESA, an enabling capability that alleviates the need for hard-coded analytic expressions or finite difference approximations. We significantly enhance the treatment of the growth and decay of convection in MESA with a new model for time-dependent convection, which is particularly important during late-stage nuclear burning in massive stars and electron degenerate ignition events. We strengthen MESA's implementation of the equation of state, and we quantify continued improvements to energy accounting and solver accuracy through a discussion of different energy equation features and enhancements. To improve the modeling of stars in MESA we describe key updates to the treatment of stellar atmospheres, molecular opacities, Compton opacities, conductive opacities, element diffusion coefficients, and nuclear reaction rates. We introduce treatments of starspots, an important consideration for low-mass stars, and modifications for superadiabatic convection in radiation-dominated regions. We describe new approaches for increasing the efficiency of calculating monochromatic opacities and radiative levitation, and for increasing the efficiency of evolving the late stages of massive stars with a new operator split nuclear burning mode. We close by discussing major updates to MESA's software infrastructure that enhance source code development and community engagement.</p>
MESA input/output for Evolutionary and Observational Consequences of Dyson Sphere Feedback
<p>MESA inlists, extras, and output for <a href="https://iopscience.iop.org/article/10.3847/1538-4357/ac3421">Evolutionary and Observational Consequences of Dyson Sphere Feedback,</a> published in the Astrophysical Journal, 2022.</p> <p>Paper DOI: 10.3847/1538-4357/ac3421</p> <p>Files included for Irradiated star experiments (recreating the work of Tout et al. (1989) in MESA) in irradiatedstar.zip:</p> <ul> <li>src/ <ul> <li>run_star_extras.f: MESA extension allowing for a constant temperature bath to irradiate a star.</li> </ul> </li> <li>inlists/ <ul> <li>inlist_zams: Create a zero age main sequence star.</li> <li>inlist_irrad_tams: Evolve a star from ZAMS to TAMS in a constant temperature irradiation bath.</li> <li>inlist_irrad_hefl: Attempt to evolve a star from TAMS to the helium flash in a constant temperature irradiation bath. Note: This model crashes before the helium flash for many parameter choices.</li> </ul> </li> <li>plots/ <ul> <li>tout_recreation_plot.ipynb: Python Jupyter notebook for generating the Figure 1 in the paper.</li> <li>lifetimes.pdf: My MESA recreation of Figure 5 from Tout et al. (1989).</li> </ul> </li> <li>LOGS/ <ul> <li>*_history: MESA output for the evolution of a given stellar mass to a given age in a given temperature bath.</li> </ul> </li> </ul> <p>Files included for Dyson Sphere Feedback experiments in dsfeedback.zip:</p> <ul> <li>src/ <ul> <li>run_star_extras.f: MESA extension allowing for a fraction of a star's luminosity to be dumped back onto the outer layer as extra heat.</li> </ul> </li> <li>inlists/ <ul> <li>inlist_sphere_tams: Evolve a selected model to the end of the main sequence with a given DS feedback fraction.</li> <li>inlist_zams: Create a zero age main sequence star.</li> <li>inlist_zams_lowmass: Create a zero age main sequence star with a timestep limit that helps with lower mass stars.</li> <li>inlist_zamstoage: Evolve a star normally from ZAMS to a selected age (0.6Gyr used here for 2Msun).</li> <li>inlist_zamstosolarage: Evolve a star normally from ZAMS to 4.6 Gyr (used before DS application for 1Msun and lower stars).</li> </ul> </li> <li>plots/ <ul> <li>ds_feedback_plots.ipynb: Python Jupyter notebook for generating the figures 2-9 in the paper.</li> <li>newplots/*: Plots generated from the notebook</li> </ul> </li> <li>LOGS/ <ul> <li>*_history: MESA output for the evolution of a given stellar mass, to a given age, and DS feedback level</li> <li>*_profile: MESA output for the structure of a given stellar mass, at one given age, and DS feedback level</li> </ul> </li> </ul> <p>Email me at mhuston@berkeley.edu if you have any comments or questions!</p> <p>MESA version: 12778</p> <p>MESA SDK version: x86_64-macos-20.4.1</p>
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