Benchmark Results: We wanted to check out the File Benchmark test in HD Tune Pro, so we fired up HD Tune Pro 5.50 and found that the drive had a sequential read speed of 1701MB/s and a write speed of 1230MB/s according to this utility. The HD Tune 4K Random Multi test with a QD of 32 showed that the drive had 145,000 IOPS read and 5,300 IOPS write.
Hd tune pro 5.50 serial key
To test the performance of the Silicon Power Armor A30, I ran a series of benchmarks using CrystalDiskMark 3.0.3, HD Tach RW 3.0.4.0, ATTO Disk Benchmark 2.46 and HD Tune Pro 5.50. To get a feel for the "real world" performance, I also copied and pasted 500MB of random files and directories in Windows Explorer.
Gather information and tune your hard drive to function at peak performance with this handy utility.Your hard drive is the life blood of your computer. When it goes bad, the whole thing goes down. Keeping it healthy can be an involved and painful process without the right tools. HDTune is the right tool for that job.HDTune works with all kinds of drives, internal or external, spinning media or SSD, USB sticks, etc. With it, you get a complete picture of how your PC's hard drive is performing, and can even check its S.M.A.R.T. status as well as perform various maintenance activities on it.With information comes power, and the ability to act, HDTune gives you the ability to monitor, view and benchmark your drives performance. You can scan for errors and repair them, as well as see which folders on your drive contain the most information.Pros: Small, easy to use, informative screens.Cons: Doesn't give all information in virtual environments, not a lot of preventative or utility options to prevent or fix errors.Conclusion: While the screens provide a lot of information, we had trouble with the application when it ran on a virtual hard drive. It crashed more than once. HDTune provides a great deal of information, but doesn't offer a lot in terms of actual tuning capabilities or even preventive utilities or tools to keep your hard drive from failing. Though it says it supports SSD's, we found no evidence of any SSD specific data or tuning options as opposed to regular HDD options. The application provides a great deal of information, but doesn't give you many options for fixing problems once they are discovered. The application's website also has little to no information regarding the application's capabilities, though it does have a lot of drive performance data on it.
Test system: AMD FX-8320 8-core CPU, 32GB DDR3 SDRAM, 1x WD 2TB Black (WD2002FAEX) drive, 1x Samsung 840 PRO Series 512GB SSD, Ubuntu 12.04.2-LTS fully updated, Windows Server 2008 R2 guest OS, HD Tune Pro 5.50 Windows disk benchmark suite.
HD Tune Pro 5.50 was used to run a number of tests on the unformatted drive. The gallery below presents some interesting numbers for various access types, and how the location of the data in the platter can affect the performance.
HD Tune is a hard disk utility that includes drive info, benchmarking, and drive health. Information includes partitions, firmware version, serial number, etc. while benchmarking covers transfer rate, access time, burst rate, and more. Health parameters include the S.M.A.R.T details as well as temperature and a whole disk surface scan.Functional with SSD and flash memory.Note: this is the last freeware version. A "pro" version with additional features is available from the website.
hd tune pro 5.70 serial é um programa de HDD e SSD de disco rígido de benchmark/monitoramento com várias funcionalidades. Ele pode ser usado para testar o desempenho da unidade, verificar falhas, verificar o status de integridade (SMART), limpar com segurança todos os dados e muito mais. O HD Tune Pro é uma versão expandida do HD Tune que contém muitos recursos adicionais, como: benchmark de gravação, apagamento seguro, configuração AAM, visualização de uso de pasta, monitor de disco, argumentos de linha de comando e benchmark de arquivo. Essa solicitação também pode aumentar a atividade do seu próprio gadget. Você também pode fazer uso deles para verificar as falhas. Isso é extremamente espetacular combinado com equipamentos de PC gratificantes por você normalmente convenientemente acessível ao sistema operacional.
Requisitos de hardware: disco rígido (interno ou externo), SSD, pendrive, leitor de cartão de memória. Devido a restrições de hardware, algumas unidades podem não oferecer todos os recursos. Após a instalação, você pode testar o aplicativo por 15 dias. Se você deseja usar o aplicativo além desse tempo, você deve adquirir um número de série. hd tune pro torrent é um aplicativo de disco rígido / SSD com várias funcionalidades. O HDtune Pro pode ser usado para avaliar o desempenho da unidade, verificar falhas, verificar o status de integridade (SMART), limpar com segurança todos os dados e muito mais. Também pode ajudá-lo em queda livre nos sons e melhorar a demonstração. Você pode até usá-lo para acessar o CD quadriculado. Da mesma forma, pode encorajá-lo a eliminar altamente suas próprias informações de CD.
hd tune pro download é uma ferramenta útil, desenvolvida para auxiliar os usuários a verificar o desempenho dos discos rígidos instalados em um computador, procurando informações essenciais como velocidade de transferência, estado de uso da tinta ou regiões. disco está quebrado. O download do HD Tune tem acesso ao desempenho do dispositivo de armazenamento e fornece informações abrangentes sobre velocidades de transferência, execução de testes de medição de desempenho ou validação de taxas de transmissão com um único arquivo com volume personalizável.
hd tune pro completo é uma eficácia maravilhosa do PC que permite que alguém verifique e numere a demonstração operacional em seu PC. Você também pode aplicá-lo na posição quadriculada de saúde física de qualquer um de seus objetivos. Este programa é fácil de usar de verdade por uma pessoa casual.
Stink bugs (Hemiptera: Pentatomidae) have historically not been pests of soybean in Minnesota. In response to the invasion of Halyomorpha halys (Stål) and reports of increasing abundance of species native to North America, a state-wide survey of soybean was conducted over 3 yr in Minnesota to determine species composition, abundance, and seasonal dynamics of Pentatomidae associated with soybean. Fourteen species of Pentatomidae (12 herbivorous and two predatory) were collected from soybean. H. halys was not detected in this survey. Among the herbivorous species found, adults of Euschistus variolarius (Palisot de Beauvois) had the greatest relative abundance (60.51%) and frequency of detection (18.44%), followed by Euschistus servus euschistoides (Say) (19.37 and 3.04%, respectively) and Chinavia hilaris (Say) (5.50 and 1.69%, respectively). Abundance of herbivorous nymphs and adults exceeded an economic threshold (20 nymphs and adults per 100 sweeps) in 0.82% of fields in 2012 but not in 2011 or 2013. The frequency of detection of herbivorous species and ratio of nymphs to adults increased with increasing reproductive growth stage of soybean. In two of three years, herbivorous adults were more abundant in the edge compared with interior of fields. Two predatory Pentatomidae, Podisus maculiventris (Say) and Podisus placidus Uhler, comprised 5.95 and 1.62% of the pentatomid adults. Though the species composition of Pentatomidae in Minnesota soybean differs from that in eastern and southern states, the spatial (i.e., greater abundance near field edge) and seasonal dynamics (i.e., increasing abundance and reproduction with increasing reproductive maturity of soybean) in soybean appear similar.
The stability of water ice on Mars' surface is determined by its temperature and the density of water vapor at the bottom of the atmosphere. Multiple orbiting instruments have been used to study column-integrated water abundance in the martian atmosphere, resolving the global annual water cycle. However, poor knowledge of the vertical distribution of water makes constraining its abundance near the surface difficult. One must assume a mixing regime to produce surface vapor density estimates. More indirectly, one can use the appearance and disappearance of seasonal water frost, along with ice stability models, to estimate this value. Here, we use derived temperature and surface reflectance data from MGS TES to constrain a 1-D thermal diffusion model, which is coupled to an atmospheric water transport model. TES temperatures are used to constrain thermal properties of our modeled subsurface, while changes in TES albedo can be used to determine the timing of water frost. We tune the density of water vapor in the atmospheric model to match the observed seasonal water frost timing in the northern hemisphere, poleward of 45N. Thus, we produce a new estimate for the water abundance in the lower atmosphere of Mars and how it varies seasonally and geographically. The timing of water frost can be ambiguous in TES data, especially at lower latitudes where the albedo contrast between frosted and unfrosted surfaces is lower (presumably due to lesser areal coverage of water frost). The uncertainty in frost timing with our approach is
A time-variable 1D photochemical model is used to study the distribution of stratospheric hydrocarbons as a function of altitude, latitude, and season on Uranus and Neptune. The results for Neptune indicate that in the absence of stratospheric circulation or other meridional transport processes, the hydrocarbon abundances exhibit strong seasonal and meridional variations in the upper stratosphere, but that these variations become increasingly damped with depth due to increasing dynamical and chemical time scales. At high altitudes, hydrocarbon mixing ratios are typically largest where the solar insolation is the greatest, leading to strong hemispheric dichotomies between the summer-to-fall hemisphere and winter-to-spring hemisphere. At mbar pressures and deeper, slower chemistry and diffusion lead to latitude variations that become more symmetric about the equator. On Uranus, the stagnant, poorly mixed stratosphere confines methane and its photochemical products to higher pressures, where chemistry and diffusion time scales remain large. Seasonal variations in hydrocarbons are therefore predicted to be more muted on Uranus, despite the planet's very large obliquity. Radiative-transfer simulations demonstrate that latitude variations in hydrocarbons on both planets are potentially observable with future JWST mid-infrared spectral imaging. Our seasonal model predictions for Neptune compare well with retrieved C2H2 and C2H6 abundances from spatially resolved ground-based observations (no such observations currently exist for Uranus), suggesting that stratospheric circulation - which was not included in these models - may have little influence on the large-scale meridional hydrocarbon distributions on Neptune, unlike the situation on Jupiter and Saturn. 2ff7e9595c
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