Hea Brand
University College London
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Featured researches published by Hea Brand.
Journal of Applied Crystallography | 2007
Ad Fortes; Ig Wood; L Vocadlo; Hea Brand; Kevin S. Knight
Detailed neutron powder diffraction measurements have been carried out on two polymorphs of anhydrous magnesium sulfate, alpha-MgSO4 and beta-MgSO4. alpha-MgSO4 is orthorhombic, space group Cmcm (Z = 4); at 4.2 K the unit-cell dimensions are a = 5.16863 (3), b = 7.86781 (5), c = 6.46674 (5) angstrom, V = 262.975 (2) angstrom(3) [rho(calc) = 3040.16 (2) kg m(-3)], and at 300 K, a = 5.17471 (3), b = 7.87563 (5), c = 6.49517 (5) angstrom, V = 264.705 (2) angstrom(3) [rho(calc) = 3020.29 (2) kg m(-3)]. The axial and volumetric thermal expansion coefficients are positive at all temperatures and exhibit no unusual behaviour. Structures were refined at 4.2 and 300 K to R-P < 3%; less precise structural parameters were determined during warming from 4.2 to 300 K. beta-MgSO4 has a more complex structure, crystallizing in space group Pbnm (Z = 4); the unit-cell dimensions at 4.2 K are a = 4.73431 (8), b = 8.58170 (12), c = 6.67266 (11) angstrom, V = 271.100 (5) angstrom(3) [rho(calc) = 2949.04 (5) kg m(-3)], and at 300 K, a = 4.74598 (7), b = 8.58310 (10), c = 6.70933 (10) angstrom, V = 273.306 (4) angstrom(3) [rho(calc) = 2925.42 (4) kg m(-3)]. The thermal expansivities of the a and c axes, and the volumetric thermal expansion coefficient, are positive at all temperatures and normally behaved. However, the thermal expansion of the b axis is both very small and negative below similar to 125 K. Structural and thermal motion parameters for beta-MgSO4 as a function of temperature are also reported.
High Pressure Research | 2006
Hea Brand; David P. Dobson; L Vocadlo; Ig Wood
The melting temperature, T m, of copper has been determined from ambient pressure to 16 GPa using multi-anvil techniques. The melting curve obtained (T m=1355(5)+44.5(31)P−0.61(21)P 2, with T m in Kelvin and P in GPa) is in good agreement with both the previous experimental studies and with recent ab initio calculations.
Physics and Chemistry of Minerals | 2009
Hea Brand; Ad Fortes; Ig Wood; Kevin S. Knight; L Vocadlo
In: (pp. 1310-). Lunar and Planetary Institue: Houston, US. (2006) | 2006
Hea Brand; Ad Fortes; Ig Wood; Maria Alfredsson; L Vocadlo
In: Lunar and Planetary Institute: Houston, US. (2006) | 2006
Ad Fortes; Ig Wood; L Vocadlo; Hea Brand; Peter Grindrod; Kh Joy; Matthew G. Tucker
In: Lunar and Planetary Science XXXIX: papers presented at the Thirty-ninth Lunar and Planetary Science Conference: March 10-14, 2008. (pp. 1641 - 1641). Lunar and Planetary Institute: Houston, US. (2008) | 2008
Hea Brand; Ca Middleton; Peter Grindrod; Ad Fortes; Ig Wood; L Vocadlo
JOURNAL OF APPLIED CRYSTALLOGRAPHY , 46 pp. 448-460. (2013) | 2013
Ad Fortes; Hea Brand; L Vocadlo; Alex Lindsay-Scott; F. Fernandez-Alonso; Ig Wood
Presented at: The Science of Solar System Ices (ScSSI): A Cross-Disciplinary Workshop 2008, Oxnard, California. (2008) | 2008
Hea Brand; Ad Fortes; Kevin S. Knight; Ig Wood; L Vocadlo
In: (Proceedings) EOS Transactions of the American Geophysical Union Fall Meeting. (pp. MR11A-08-). (2007) | 2007
Ad Fortes; L Vocadlo; Ig Wood; Peter Grindrod; Hea Brand; El Gromnitskaya; Ag Lyapin; Of Yagaforov
(ISIS Experimental Reports RB20047 ). CCLRC: Didcot, UK. | 2005
Ad Fortes; Ig Wood; L Vocadlo; Hea Brand