Zobrazeno 1 - 10
of 250
pro vyhledávání: '"Hakeem, M A"'
Autor:
Hakeem, M. J., Sulphey, M. M.
Publikováno v:
Transforming Government: People, Process and Policy, 2024, Vol. 18, Issue 4, pp. 785-802.
Externí odkaz:
http://www.emeraldinsight.com/doi/10.1108/TG-06-2024-0136
Autor:
Smith, D., Hakeem, M. A., Parisiades, P., Maynard-Casely, H. E., Foster, D., Eden, D., Bull, D. J., Marshall, A. R. L., Adawi, A. M., Howie, R., Sapelkin, A., Brazhkin, V. V., Proctor, J. E.
Publikováno v:
Phys. Rev. E 96, 052113 (2017)
We report experimental evidence for a crossover between a liquid-like state and a gas-like state in fluid methane (CH4). This crossover is observed in all of our experiments, up to 397 K temperature; 2.1 times the critical temperature of methane. The
Externí odkaz:
http://arxiv.org/abs/1710.04212
Autor:
Gleissner, J., Errandonea, D., Segura, A., Pellicer-Porres, J., Hakeem, M. A., Proctor, J., Raju, S. V., Kumar, R. S., Rodriguez-Hernandez, P., Munoz, A., Lopez-Moreno, S., Bettinelli, M.
Publikováno v:
Phys. Rev. B 94, 134108 (2016)
We report a high-pressure study of monoclinic monazite-type SrCrO4 up to 26 GPa. Therein we combined x-ray diffraction, Raman and optical-absorption measurements with ab initio calculations, to find a pressure-induced structural phase transition of S
Externí odkaz:
http://arxiv.org/abs/1610.06738
Autor:
Johnston, Kyle B, Oluseyi, Hakeem M
With the advent of digital astronomy, new benefits and new problems have been presented to the modern day astronomer. While data can be captured in a more efficient and accurate manor using digital means, the efficiency of data retrieval has led to a
Externí odkaz:
http://arxiv.org/abs/1601.03769
Solar variability investigations that include magnetic energy coupling are paramount to solving many key solar/stellar physics problems, particularly for understanding the temporal variability of magnetic energy redistribution and heating processes.
Externí odkaz:
http://arxiv.org/abs/1601.02986
Increasing evidence for coronal heating contributions from cooler solar atmospheric layers, notably quiet Sun (QS) conditions, challenges standard solar atmospheric descriptions of bright transition region (TR) emission. As such, questions to the rol
Externí odkaz:
http://arxiv.org/abs/1501.05211
Autor:
Orange, N. Brice, Oluseyi, Hakeem M., Chesny, David L., Patel, Maulik, Champey, Patrick, Hesterly, Katie, Anthony, Dylan, Treen, Robert
Achieving sub-arcsecond co-registration across varying time-lines of multi-wavelength and instrument images is not trivial, and requires accurate characterization of instrument pointing jitter. In this work we have investigated internal pointing erro
Externí odkaz:
http://arxiv.org/abs/1501.05000
Autor:
Orange, N. Brice, Oluseyi, Hakeem M., Chesny, David L., Patel, Maulik, Hesterly, Katie, Preuss, Lauren, Neira, Chantale, Turner, Niescja E.
Since their discovery twenty year ago, transition region bright points (TRBPs) have never been observed spectroscopically. Bright point properties have not been compared with similar transition region and coronal structures. In this work we have inve
Externí odkaz:
http://arxiv.org/abs/1501.04997
Autor:
Oluseyi, Hakeem M., Walker, II, A. B. C., Santiago, David I., Hoover, Richard B., Barbee, Jr, Troy W.
Publikováno v:
Astrophys.J. 527 (1999) 992-999
In the present work we undertake a study of the quasi-static loop model and the observational consequences of the various solutions found. We obtain the most general solutions consistent with certain initial conditions. Great care is exercised in cho
Externí odkaz:
http://arxiv.org/abs/astro-ph/9904063
Akademický článek
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