179,574 research outputs found
Musgrave, R A, 2790823
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/407057Surname: MUSGRAVE. Given Name(s) or Initials: R A. Military Service Number or Last Known Location: 2790823. Missing, Wounded and Prisoner of War Enquiry Card Index Number: SEA-3978.243092
Item: [2016.0049.39332] "Musgrave, R A, 2790823
The Musgrave Province - NT's most underexplored terrane
No full textMost mineral exploration within the Palaeo- to Mesoproterozoic of the Northern Territory has been focused on the Palaeoproterozoic basement terranes of the North Australian Craton and on Northern Australian platform cover rocks such as the McArthur Basin. In comparison, the more juvenile Proterozoic crust that lies to the south of the North Australian Craton, including the Warumpi Province (southwestern Arunta) and Musgrave Province3, has received little attention from explorers. The Musgrave Province within the NT is one of the most underexplored Proterozoic terranes on the Australian continent, with an average of 1 drillhole for every 210 km2. The geological framework of the Musgrave Province was a focus of NTGS studies in the 1990s (see List of selected NTGS publications in the Musgrave Province) and a summary of the geology of the Musgrave Province has recently been published (Edgoose et al 2004). Recent flying of the 2001 Eromanga and 2004 Simpson airborne surveys have completed high-resolution airborne magnetic coverage of the Musgrave Province at exploreable depths. NTGS is continuing its investigations in the Musgrave Province through collaborative research programs with the University of Adelaide.Ian R Scrimgeour, Christine J Edgoose, Dorothy F Close and Ben P Wad
Coronation medley march
No full textPublisher's advertisement on back cover. [note]Musgrave Bros, Toronto. [dealer stamp]British soldier on horse with sword, British flag and maple leaves. [illustration]March [form/genre]Dublin Fusiliers. [tempo]C major [key]Piano [instrumentation
Desudaboides fuscomaculata Musgrave
No full text<i>Desudaboides fuscomaculata</i> Musgrave <p>Figs 1I –J, 2, 5.</p> <p> <i>Desudaboides fuscomaculata</i> Musgrave, 1927: 47</p> <p> <b>Etymology.</b> <i>fuscomaculata</i> (adj., Latin): from <i>fuscus</i>, brown, and <i>maculatus</i>, spotted. Literally “spotted with brown”, the name refers to the colouration of the tegmina.</p> <p> <b>Type material examined:</b> Holotype 3: [Holotype <i>Desudaboides flavomaculata</i> Musgrave Ƥ] [Chilla, Jan 24] [Male, stated in error as Ƥ in paper, Det. by A. Musgrave.] [k55909] [Holotype 3 <i>Desudaboides fuscomaculata</i> Musgrave, 1927, Jérôme Constant det. 2009] (AMS).</p> <p> Allotype Ƥ: [Allotype <i>Desudaboides flavomaculata</i> Musgrave 3] [Chilla, Jan 24] [Female, stated in error as male in paper, Det. by A. Musgrave.] [k55910] [Paratype Ƥ <i>Desudaboides fuscomaculata</i> Musgrave, 1927, Jérôme Constant det. 2009] (AMS).</p> <p>Coordinates of Chinchilla (= Chilla): 26°45'S 150°38'E.</p> <p> <b>Notes:</b> The species has been described under the name <i>fuscomaculata</i> (Musgrave, 1927) but both type specimens bear labels indicating <i>flavomaculata</i>. The other labels on the specimens do not allow any doubt that they are the types. Additional labels with the right name have been attached to both specimens to avoid future confusion.</p> <p> Nagai & Porion (1996) provide a <i>habitus</i> illustration of the species but erroneously stated that the type specimens of <i>D. fuscomaculata</i> are deposited in the collections of the Macleay Museum, University of Sydney.</p> <p> <b>Other material examined:</b> 2 3: 40 Mile Scrub near Mt. Garnet, N. Qld, 9.i.1973, M.S. & B.J. Moulds (AMS) coordinates of 40 Mile Scrub: 18°5’S 144°50’E; 1 3: 40 Mile Scrub, 65 km SW of Mt. Garnet, N. Qld, 19.xii.1974, M.S. Moulds (AMS); 2 3: idem, 15.iii.1982 (ASCU); 2 3, 1 Ƥ: 40 Mile Scrub, 40 mi SW of Mt. Garnet, N. Qld, 19.xii.1974, M.S. Moulds (ASCU); 1 Ƥ: 40 Miles Scrub, 64 km SW of Ravenshoe, N. Qld, 7.i.1976, mv lamp, D.K. McAlpine (AMS); 2 3, 2 Ƥ: Chillagoe, GPS 300, 11-12.iii.1997, light trap, Th. Bourgoin (1 3, 1 Ƥ: MNHN; 1 3, 1 Ƥ: RBINS) coordinates of Chillagoe: 17°9'S 144°32'E</p> <p> <b>Additional data:</b> Mareeba (Nagai et Porion, 1996). Coordinates of Mareeba: 17°0'S 145°26'E.</p> <p> - specimens in ANIC (<i>pers. comm.</i> Tom Weir, 2008): 1 ex.: Emu Ck, 27 km SW of Dimbulah, QLD, 25- 26.xi.1981, J. Balderson, coordinates of Emu Creek: 17°20’S 144°57’E; 1 ex.: Lolworth Station, N.</p> <p>Queensland, 29.vi.1907, Mrs Black, coordinates of Lolworth Station: 20°11’S 145°1’E; 2 ex.: 40 Mile Scrub, 40 miles SW of Mt Garnet, NQ, 9.i.1973, G.J. Brooks; 4ex.: idem, 26.ii.1974; 1 ex.: 40 Mile Scrub, 55 miles SW by S of Mt Garnet, 8.xii.1985, J. Balderson; 5 ex.: 40 Mile Scrub, 4.x.1989, L. Ring; 3 ex: idem, 12.iii.1994, L.R. Ring; 6 ex.: Mt. Garnet, 14.iv.1944, coordinates of Mt. Garnet: 17°41’S 145°7’E.</p> <p> <b>Diagnosis.</b> The species is immediately recognized by the following combination of characters: (<b>1</b>) frons pale yellow to red with 4 black spots on disc (Fig. 1 J), (<b>2</b>) hind wings with base red (Fig. 1 I), (<b>3</b>) abdominal tergites 3 to 8 bright orange (Fig. 1 I), (<b>4</b>) tegmina with numerous black-brown spots, with base rosy red and with apex hyaline (Fig. 1 I).</p> <p> <i>Genitalia</i> 3: see Figs. 2A–C.</p> <p> <b>Biology.</b> Nothing is known except that five of the 15 examined specimens have been caught by light trap.</p> <p> <b>Distribution</b> (Fig. 5). Eastern Queensland. The distribution seems to roughly follow the Great Dividing Range.</p>Published as part of <i>Constant, Jerome, 2010, Review of the Australian genus Desudaboides Musgrave with descriptions of four new species (Hemiptera: Fulgoromorpha: Fulgoridae), pp. 39-48 in Zootaxa 2351</i> on pages 42-43, DOI: <a href="http://zenodo.org/record/193465">10.5281/zenodo.193465</a>
Appropriate Similarity Measures for Author Cocitation Analysis
No full textWe provide a number of new insights into the methodological discussion about author cocitation analysis. We first argue that the use of the Pearson correlation for measuring the similarity between authors’ cocitation profiles is not very satisfactory. We then discuss what kind of similarity measures may be used as an alternative to the Pearson correlation. We consider three similarity measures in particular. One is the well-known cosine. The other two similarity measures have not been used before in the bibliometric literature. Finally, we show by means of an example that our findings have a high practical relevance.information science;Pearson correlation;cosine;similarity measure;author cocitation analysis
Musgrave Block, SA, 1967 (P338), magnetic line data, AWAGS levelled
No full textMaintenance and Update Frequency: notPlannedStatement: This Musgrave Block, SA, 1967 (P338), magnetic line data, AWAGS levelled is an airborne-derived magnetic line dataset for the Musgrave Block, SA, 1967 survey. The data was acquired under the project No. 338 for the geological survey of SA. A total of 30860 line-kilometres of data at a line spacing of 1600m and 150m terrain clearance were acquired during this survey. To constrain long wavelengths in the data, an independent data set, the Australia-wide Airborne Geophysical Survey (AWAGS) airborne magnetic data, was used to control the base levels of the survey data (Milligan et al., 2009). This survey data is essentially levelled to AWAGS. Details of the specifications of individual airborne surveys can be found in the Fourteenth Edition of the Index of Airborne Geophysical Surveys (Percival, 2014). This Index is also available online at http://pid.geoscience.gov.au/dataset/79134.
References:
Milligan, P.R., Minty, B.R.S., Richardson, M. & Franklin, R., 2009. The Australia-wide Airborne Geophysical Survey accurate continental magnetic coverage. Preview, No. 138, p. 1-128,
Percival, P.J., 2014. Index of airborne geophysical surveys (Fourteenth Edition).Total magnetic intensity (TMI) data measures variations in the intensity of the Earth's magnetic field caused by the contrasting content of rock-forming minerals in the Earth crust. Magnetic anomalies can be either positive (field stronger than normal) or negative (field weaker) depending on the susceptibility of the rock. The data are processed via standard methods to ensure the response recorded is that due only to the rocks in the ground. The results produce datasets that can be interpreted to reveal the geological structure of the sub-surface. The processed data is checked for quality by GA geophysicists to ensure that the final data released by GA are fit-for-purpose.<br/> These line dataset from the Musgrave Block, SA, 1967 survey were acquired in 1967 by the SA Government, and consisted of 30860 line-kilometres of data at 1600m line spacing and 150m terrain clearance. To constrain long wavelengths in the data, an independent data set, the Australia-wide Airborne Geophysical Survey (AWAGS) airborne magnetic data, was used to control the base levels of the survey data. This survey data is essentially levelled to AWAGS
Financial feasibility of sustainable events
No full textContributions to event sustainability are a fundamental step for the global success of any initiative: nevertheless, this can directly and indirectly affect markets and institutions (‘brand’ in particular). Enterprises will need to contribute financially to event sustainability, in a perspective not of bearing further costs, but as a real investment, capable of delivering multiple benefits. The financial contribution will also be considered in terms of a portion of the value created by the event. In this context, dealing opportunely with CRM concepts and tools would enable firms to monitor their investment carefully
The burning heart - the Proterozoic geology and geological evolution of the west Musgrave Region, central Australia
No full textGR focus review - this article has a corrigendum at 10.1016/j.gr.2015.06.002 Due to an error during revisions, the captions for Figs. 5 through to 10 in Howard et al. (2015) are out of order.The Musgrave Province is one of the most geodynamically significant of Australia's Proterozoic orogenic belts, lying at the intersection of the continent's three cratonic elements - the West, North and South Australian Cratons. While remoteness and cultural sensitivity have slowed geological research into this region, recent collaborative programs in Western Australia (the west Musgrave Province) have done much to address this. This Focus Review provides a synthesis of this, and previous, work investigating the Mesoproterozoic to Neoproterozoic geological evolution of the province. The Musgrave Province is a Mesoproterozoic to Neoproterozoic belt dominated by granites formed and deformed during several major events. A cryptic juvenile basement is exposed mainly in the east Musgrave Province as c. 1600-1550. Ma orthogneiss and in the west Musgrave Province as isolated outcrops of granulite-facies metagranites of the c. 1575. Ma Warlawurru Supersuite. Zircon Hf-isotopic data suggest an earlier major juvenile crust-forming event at c. 1950-1900. Ma. There is, however, no evidence that the province evolved over Archean crust. The c. 1600-1550. Ma period probably involved evolution within a primitive arc setting, perhaps developed on c. 1950-1900. Ma oceanic or oceanic-arc crust. Voluminous calc-alkaline plutonism was accompanied by clastic and volcaniclastic basin formation during the 1345-1293. Ma Mount West Orogeny. This stage traced the evolution of a continental arc reflecting the final amalgamation of the combined North and West Australian Craton with the South Australian Craton. The intervening c. 1400. Ma primitive crust - the Madura Province - on which the proto-Musgrave Province had evolved, was consumed during amalgamation. The thickened crust resulting from this accretion was drastically thinned at the beginning of the c. 1220-1150. Ma Musgrave Orogeny as this central part of the new combined craton entered an extraordinary period of high heat flow characterised by c. 100. m.y. of ultrahigh-temperature metamorphism and high-temperature, anhydrous, alkali-calcic magmatism sourced from MASH chambers developed at the base of the thinned crust. The ridged cratonic architecture and a massive accumulation of high radiogenic heat producing granites within the mid crust perpetuated a thin crustal regime. Voluminous magmatism was again triggered during the c. 1090-1040. Ma Giles Event with the evolution of the magmatism-dominated, Ngaanyatjarra Rift. This event was likely initiated through renewed movement along translithospheric faults that intersected the thermally perturbed Musgrave Province, pinned at a cratonic junction. Mantle-derived bimodal magmatism extended more or less continuously for 50. m.y., producing one of the world's largest layered mafic intrusions and supervolcano-sized additions of juvenile felsic crust, in the form of alkali-calcic to alkali, A-type, rhyolite deposits. Together, the Albany-Fraser Orogen, which developed over the southern margin of the West Australian Craton, and the Musgrave Province mark the preserved edge of the North and West Australian Craton. These two belts show remarkable chronological links between c. 1345 and 1150. Ma but contrasting histories before and after that period. Their period of shared evolution reflects collision and accretion of the South Australian Craton, but their tectonic setting and basement geology throughout that event were very different.H.M. Howard, R.H. Smithies, C.L. Kirkland, D.E. Kelsey, A. Aitken, M.T.D. Wingate, R. Quentin de Gromard, C.V. Spaggiari, W.D. Maie
"Closing the R&D Gap, Evaluating the Sources of R&D Spending"
No full textBoth spending and tax policies have been implemented in the United States with the goal of stimulating private sector research and development (R&D). Karier questions whether current R&D policy, especially the research and experimentation tax credit, can contribute to closing the gap between nondefense expenditures on R&D in the United States and such expenditures in other countries, such as Japan and Germany. He also explores possible changes to our current R&D policy to make it more effective.
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