cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Sonnenfleckenzeichnung Nr. 26570.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 01.01.1983, erstellt von Hans Ulrich Keller
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1983

description: Bleistiftzeichnung mit Tinte und Farbstift überschrieben, erstellt als Projektionsbildzeichnung in der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss Coudé-Refraktor (150/2250 mm).
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden mit Bleistift auf einem Vordruck eingetragen. Zusätzlich notiert: Tabelle mit den statistischen Angaben, für die Werte g, f sowie Gr (Anzahl g) und darüber hinaus einer Spalte für A: mit Hilfe eines korrekt-reduzierenden optischen Filters von blossem Auge sichtbare Flecken
Pipistrellus anthonyi Tate 1942
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus anthonyi

description: Pipistrellus anthonyi Tate, 1942. Bull. Am. Mus. Nat. Hist., 80:252. TYPE LOCALITY: Burma, Changyinku, 7,000 ft. (2,134 m). DISTRIBUTION: Known only from the type locality. COMMENTS: Subgenus Hypsugo. May be referrable to Nyctalus or even Philetor. Known only by the holotype.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on pages 219-220, DOI: 10.5281/zenodo.7353060
There's a crocodile in the house : symbol formation and its relation to symptoms in a four year old girl
Creators: name: Re, Jennifer M.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
A study of large fringe and non-fringe subtrees in conditional Galton-Watson trees
Creators: name: Cai, Xing Shi
name: Devroye, Luc
Publisher: name: arXiv
Year: 2016
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60C05

description: We study the conditions for families of subtrees to exist with high probability (whp) in a Galton-Walton tree of size $n$. We first give a Poisson approximation of fringe subtree counts, which yields the height of the maximal complete $r$-ary fringe subtree. Then we determine the maximal $K_n$ such that every tree of size at most $K_n$ appears as fringe subtree whp. Finally, we study non-fringe subtree counts and determine the height of the maximal complete $r$-ary non-fringe subtree.
description: 40 pages, 7 figure
Pipistrellus arabicus Harrison 1979
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus arabicus

description: Pipistrellus arabicus Harrison, 1979. Mammalia, 43:575. TYPE LOCALITY: Oman, Wadi Sahtan (23°22'N, 57°18'E). DISTRIBUTION: Oman. COMMENTS: Subgenus Hypsugo.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
title: CMOS Camera-Type THz Compact Antenna Test Range for Far-Field Radiation Pattern Analysis
Creators: name: Zatta, Robin
name: Jagtap, Vishal S.
name: Grzyb, Janusz
name: Pfeiffer, Ullrich
Publisher: name: Bergische Universität Wuppertal
Year: 2021

description: This paper presents a CMOS camera-type THz compact antenna test range (CATR) to facilitate a convenient means to measure far-field radiation patterns of transmitters (TXs). For concept validation, we measured the far-field radiation pattern of a 26-dBi 0.852-THz standard gain horn antenna-type TX with known far-field characteristics with the THz CATR. With the help of geometrical multi-frame super-resolution imaging, the directivity determination accuracy achieved at a peak signal-to-noise ratio (PSNR) of 34.8 dB is 0.2 dB. Further, we investigated a THz continuous-wave (CW) photomixer TX with unknown far-field characteristics at 0.852 THz. It emits a higher-order mode far-field radiation pattern, and its directivity is 25.4 dBi, determined at a PSNR of 31.8 dB.
description: This document is the accepted manuscript version that has been published in final form in: 2020 45th International Conference on Infrared, Millimeter, and Terahertz Waves (IRMMW-THz). https://doi.org/10.1109/IRMMW-THz46771.2020.9370372
© 2020 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.
Can Green Media Be Accessible?
Creators: name: Orero, Pilar
Publisher: name: Zenodo
Year: 2023
Subjects: Education for sustainable development, eco-school, environmental education, sustainability, sustainability competences, GreenComp

description: In her presentation, Pilar aims to address the question of whether green media can be made accessible. She aims to enhance the understanding of this topic and explore the potential for ensuring widespread accessibility to environmentally conscious media content.
Si K Edge Structure and Variability in Galactic X-Ray Binaries
Creators: name: Schulz, Norbert S.
name: Corrales, Lia
name: Canizares, Claude R.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We survey the Si K edge structure in various absorbed Galactic low-mass X-ray binaries (LMXBs) to study states of silicon in the inter- and circum-stellar medium. The bulk of these LMXBs lie toward the Galactic bulge region and all have column densities above $10^{22}$ cm$^{-2}$. The observations were performed with the \emph{Chandra} High Energy Transmission Grating Spectrometer. The Si K edge in all sources appears at an energy value of 1844$\pm$0.001 eV. The edge exhibits significant substructure which can be described by a near edge absorption feature at 1849$\pm$0.002 eV and a far edge absorption feature at 1865$\pm$0.002 eV. Both of these absorption features appear variable with equivalent widths up to several mÅ. We can describe the edge structure with several components: multiple edge functions, near edge absorption excesses from silicates in dust form, signatures from X-ray scattering optical depths, and a variable warm absorber from ionized atomic silicon. The measured optical depths of the edges indicate much higher values than expected from atomic silicon cross sections and ISM abundances, and appear consistent with predictions from silicate X-ray absorption and scattering. A comparison with models also indicates a preference for larger dust grain sizes. In many cases we identify \sixiii\ resonance absorption and determine ionization parameters between log $ξ$ = 1.8 and 2.8 and turbulent velocities between 300 and 1000 \kms. This places the warm absorber in close vicinity of the X-ray binaries. In some data we observe a weak edge at 1.840 keV, potentially from a lesser contribution of neutral atomic silicon.
description: 14 pages, 10 figues, accepted by ApJ Main
Pipistrellus ariel Thomas 1904
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus ariel

description: Pipistrellus ariel Thomas, 1904. Ann. Mag. Nat. Hist., ser. 7, 14:157. TYPE LOCALITY: Sudan, Kassala Province, Wadi Alagi (22°N, 35°E), 2,000 ft. (610 m). DISTRIBUTION: Egypt, N Sudan. COMMENTS: Subgenus Hypsugo.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
An experience of persecutory anxiety in a latency aged girl in psychoanalytic psychotherapy
Creators: name: Lowry, Marita.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Generalised T-duality and Integrable Deformations
Creators: name: Thompson, Daniel C.
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: We review some recent developments in the construction of integrable $η$- and $λ$-deformations of the $AdS_5 \times S^5$ superstring. We highlight their link with Poisson-Lie T-duality.
description: Proceedings of a talk at The String Theory Universe, 21st European String Workshop and 3rd COST MP1210 Meeting
Multiple operator integrals, Haagerup and Haagerup-like tensor products, and operator ideals
Creators: name: Aleksandrov, Alexei
name: Peller, Vladimir
Publisher: name: arXiv
Year: 2016
Subjects: subject: Functional Analysis (math.FA)
subject: Classical Analysis and ODEs (math.CA)
subject: Complex Variables (math.CV)
subject: Spectral Theory (math.SP)
subject: FOS: Mathematics

description: We study Schatten--von Neumann properties of multiple operator integrals with integrands in the Haagerup tensor product of $L^\infty$ spaces. We obtain sharp, best possible estimates. This allowed us to obtain sharp Schatten--von Neumann estimates in the case of {\it Haagerup-like} tensor products.
description: 19 pages. arXiv admin note: text overlap with arXiv:1505.07173
Constancy of the Cluster Gas Mass Fraction in the R_h=ct Universe
Creators: name: Melia, Fulvio
Publisher: name: arXiv
Year: 2016
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The ratio of baryonic to dark matter densities is assumed to have remained constant throughout the formation of structure. With this, simulations show that the fraction f_gas(z) of baryonic mass to total mass in galaxy clusters should be nearly constant with redshift z. However, the measurement of these quantities depends on the angular distance to the source, which evolves with z according to the assumed background cosmology. An accurate determination of f_gas(z) for a large sample of hot (kT_e > 5 keV), dynamically relaxed clusters could therefore be used as a probe of the cosmological expansion up to z < 2. The fraction f_gas(z) would remain constant only when the "correct" cosmology is used to fit the data. In this paper, we compare the predicted gas mass fractions for both LCDM and the R_h=ct Universe and test them against the 3 largest cluster samples. We show that R_h=ct is consistent with a constant f_gas in the redshift range z < 2, as was previously shown for the reference LCDM model (with parameter values H_0=70 km/s/Mpc, Omega_m=0.3 and w_de=-1). Unlike LCDM, however, the R_h=ct Universe has no free parameters to optimize in fitting the data. Model selection tools, such as the Akaike Information Criterion (AIC) and the Bayes Information Criterion (BIC), therefore tend to favour R_h=ct over LCDM. For example, the BIC favours R_h=ct with a likelihood of ~95% versus ~5% for LCDM.
description: 17 Pages, 6 Figures, 1 Table. Accepted for publication in Proc. R. Soc. A
Frequency stability of a wavelength meter and applications to laser frequency stabilization
Creators: name: Saleh, Khaldoun
name: Millo, Jacques
name: Didier, Alexandre
name: Kersalé, Yann
name: Lacroûte, Clément
Publisher: name: arXiv
Year: 2015
Subjects: subject: Optics (physics.optics)
subject: Atomic Physics (physics.atom-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Interferometric wavelength meters have attained frequency resolutions down to the MHz range. In particular, Fizeau interferometers, which have no moving parts, are becoming a popular tool for laser characterization and stabilization. In this article, we characterize such a wavelength meter using an ultra-stable laser in terms of relative frequency instability $σ_y(τ)$ and demonstrate that it can achieve a short-term instability $σ_y(1 s) \approx 2{\times}10^{-10}$ and a frequency drift of order $10$ MHz/day. We use this apparatus to demonstrate frequency control of a near-infrared laser, where a frequency instability below $3{\times}10^{-10}$ from 1 s to 2000 s is achieved. Such performance is for example adequate for ions trapping and atoms cooling experiments.
description: 5 pages, 4 figures
Ferroelectricity in corundum derivatives
Creators: name: Ye, Meng
name: Vanderbilt, David
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The search for new ferroelectric (FE) materials holds promise for broadening our understanding of FE mechanisms and extending the range of application of FE materials. Here we investigate a class of ABO3 and A2BB'O6 materials that can be derived from the X2O3 corundum structure by mixing two or three ordered cations on the X site. Most such corundum derivatives have a polar structure, but it is unclear whether the polarization is reversible, which is a requirement for a FE material. In this paper, we propose a method to study the FE reversal path of materials in the corundum derivative family. We first categorize the corundum derivatives into four classes and show that only two of these allow for the possibility of FE reversal. We then calculate the energy profile and energy barrier of the FE reversal path using first-principles density functional methods with a structural constraint. Furthermore, we identify several empirical measures that can provide a rule of thumb for estimating the energy barriers. Finally, the conditions under which the magnetic ordering is compatible with ferroelectricity are determined. These results lead us to predict several potentially new FE materials.
description: 7 pages, 6 figures
Homologous prominence non-radial eruptions: A case study
Creators: name: Duchlev, P.
name: Koleva, K.
name: Madjarska, M. S.
name: Dechev, M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The present study provides important details on homologous eruptions of a solar prominence that occurred in active region NOAA 10904 on 2006 August 22. We report on the preeruptive phase of the homologous feature as well as the kinematics and the morphology of a forth from a series of prominence eruptions that is critical in defining the nature of the previous consecutive eruptions. The evolution of the overlying coronal field during homologous eruptions is discussed and a new observational criterion for homologous eruptions is provided. We find a distinctive sequence of three activation periods each of them containing preeruptive precursors such as a brightening and enlarging of the prominence body followed by small surge- like ejections from its southern end observed in the radio 17 GHz. We analyse a fourth eruption that clearly indicates a full reformation of the prominence after the third eruption. The fourth eruption although occurring 11 hrs later has an identical morphology, the same angle of propagation with respect to the radial direction, as well as similar kinematic evolution as the previous three eruptions. We find an important feature of the homologous eruptive prominence sequence that is the maximum height increase of each consecutive eruption. The present analysis establishes that all four eruptions observed in Hα are of confined type with the third eruption undergoing a thermal disappearance during its eruptive phase. We suggest that the observation of the same direction of the magnetic flux rope (MFR) ejections can be consider as an additional observational criterion for MFR homology. This observational indication for homologous eruptions is important, especially in the case of events of typical or poorly distinguishable morphology of eruptive solar phenomena.
description: 19 pages, 6 figures, 2 figures in Appendix, accepted in New Astronomy
Pipistrellus babu Thomas 1915
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus babu

description: Pipistrellus babu Thomas, 1915. J. Bombay Nat. Hist. Soc., 24:30. TYPE LOCALITY: Pakistan, Punjab, Rawalpindi, Murree, 8,000 ft. (2,438 m). DISTRIBUTION: Afghanistan, Pakistan, N India, Nepal, Bhutan, Burma, SW China. COMMENTS: Subgenus Pipistrellus.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
Large deviations for the branching Brownian motion in presence of selection or coalescence
Creators: name: Derrida, Bernard
name: Shi, Zhan
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mathematical Physics (math-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The large deviation function has been known for a long time in the literature for the displacement of the rightmost particle in a branching random walk (BRW), or in a branching Brownian motion (BBM). More recently a number of generalizations of the BBM and of the BRW have been considered where selection or coalescence mechanisms tend to limit the exponential growth of the number of particles. Here we try to estimate the large deviation function of the position of the rightmost particle for several such generalizations: the $L$-BBM, the $N$-BBM, and the CBRW (coalescing branching random walk) which is closely related to the noisy FKPP equation. Our approach allows us to obtain only upper bounds on these large deviation functions. One noticeable feature of our results is their non analytic dependence on the parameters (such as the coalescence rate in the CBRW).
description: submitted to Journal of Statistical Physics
Pipistrellus bodenheimeri Harrison 1960
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus bodenheimeri

description: Pipistrellus bodenheimeri Harrison, 1960. Durban Mus. Novit., 5:261. TYPE LOCALITY: Israel, 40 km N Eilat, Wadi Araba, Yotwata. DISTRIBUTION: Israel, S Yemen, Oman, perhaps Socotra Isl (Yemen). COMMENTS: Subgenus Hypsugo.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
Energy Efficient Downlink Transmission for Multi-cell Massive DAS with Pilot Contamination
Creators: name: Zuo, Jun
name: Zhang, Jun
name: Yuen, Chau
name: Jiang, Wei
name: Luo, Wu
Publisher: name: arXiv
Year: 2016
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: In this paper, we study the energy efficiency (EE) of a downlink multi-cell massive distributed antenna system (DAS) in the presence of pilot contamination (PC), where the antennas are clustered on the remote radio heads (RRHs). We employ a practical power consumption model by considering the transmit power, the circuit power, and the backhaul power, in contrast to most of the existing works which focus on co-located antenna systems (CAS) where the backhaul power is negligible. For a given average user rate, we consider the problem of maximizing the EE with respect to the number of each RRH antennas $n$, the number of RRHs $M$, the number of users $K$, and study the impact of system parameters on the optimal $n$, $M$ and $K$. Specifically, by applying random matrix theory, we derive the closed-form expressions of the optimal $n$, and find the solution of the optimal $M$ and $K$, under a simplified channel model with maximum ratio transmission. From the results, we find that to achieve the optimal EE, a large number of antennas is needed for a given user rate and PC. As the number of users increases, EE can be improved further by having more RRHs and antennas. Moreover, if the backhauling power is not large, massive DAS can be more energy efficient than massive CAS. These insights provide a useful guide to practical deployment of massive DAS.
description: 12 pages,10 figures. Accepted by the IEEE Transactions on Vehicular Technology
Betwixt and between
Creators: name: Aston, Carolyn.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Non-equilibrium helium ionization in an MHD simulation of the solar atmosphere
Creators: name: Golding, Thomas Peter
name: Leenaarts, Jorrit
name: Carlsson, Mats
Publisher: name: arXiv
Year: 2015
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The ionization state of the gas in the dynamic solar chromosphere can depart strongly from the instantaneous statistical equilibrium commonly assumed in numerical modeling. We improve on earlier simulations of the solar atmosphere that only included non-equilbrium hydrogen ionization by performing a 2D radiation-magneto-hydrodynamics simulation featuring non-equilibrium ionization of both hydrogen and helium. The simulation includes the effect of hydrogen Lyman-$α$ and the EUV radiation from the corona on the ionization and heating of the atmosphere. Details on code implementation are given. We obtain helium ion fractions that are far from their equilibrium values. Comparison with models with LTE ionization shows that non-equilibrium helium ionization leads to higher temperatures in wave fronts and lower temperatures in the gas between shocks. Assuming LTE ionization results in a thermostat-like behaviour with matter accumulating around the temperatures where the LTE ionization fractions change rapidly. Comparison of DEM curves computed from our models shows that non-equilibrium ionization leads to more radiating material in the temperature range 11-18 kK compared to models with LTE helium ionization. We conclude that non-equilbrium helium ionization is important for the dynamics and thermal structure of the upper chromosphere and transition region. It might also help resolve the problem that intensities of chromospheric lines computed from current models are smaller than those observed.
description: Accepted for publication in Astrophysical Journal
Pipistrellus cadornae Thomas 1916
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus cadornae

description: Pipistrellus cadornae Thomas, 1916. J. Bombay Nat. Hist. Soc., 24:416. TYPE LOCALITY: India, Darjeeling, Pashok, 3,500 ft (1,067m). DISTRIBUTION: NE India, Burma, Thailand. COMMENTS: Subgenus Hypsugo. Listed as a subspecies of savii by Ellerman and MorrisonScott (1951:170), but see Hill (19626:133).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
The JCMT Gould Belt Survey: Evidence for radiative heating and contamination in the W40 complex
Creators: name: Rumble, D.
name: Hatchell, J.
name: Pattle, K.
name: Kirk, H.
name: Wilson, T.
name: Buckle, J.
name: Berry, D. S.
name: Broekhoven-Fiene, H.
name: Currie, M. J.
name: Fich, M.
name: Jenness, T.
name: Johnstone, D.
name: Mottram, J. C.
name: Nutter, D.
name: Pineda, J. E.
name: Quinn, C.
name: Salji, C.
name: Tisi, S.
name: Walker-Smith, S.
name: Di Francesco, J.
name: Hogerheijde, M. R.
name: Ward-Thompson, D.
name: Bastien, P.
name: Bresnahan, D.
name: Butner, H.
name: Chen, M.
name: Chrysostomou, A.
name: Coude, S.
name: Davis, C. J.
name: Drabek-Maunder, E.
name: Duarte-Cabral, A.
name: Fiege, J.
name: Friberg, P.
name: Friesen, R.
name: Fuller, G. A.
name: Graves, S.
name: Greaves, J.
name: Gregson, J.
name: Holland, W.
name: Joncas, G.
name: Kirk, J. M.
name: Knee, L. B. G.
name: Mairs, S.
name: Matthews, B. C.
name: Moriarty-Schieven, G.
name: Mowat, C.
name: Rawlings, J.
name: Richer, J.
name: Robertson, D.
name: Rosolowsky, E.
name: Sadavoy, S.
name: Thomas, H.
name: Tothill, N.
name: Viti, S.
name: White, G. J.
name: Wouterloot, J.
name: Yates, J.
name: Zhu, M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present SCUBA-2 450μm and 850μm observations of the W40 complex in the Serpens-Aquila region as part of the James Clerk Maxwell Telescope (JCMT) Gould Belt Survey (GBS) of nearby star-forming regions. We investigate radiative heating by constructing temperature maps from the ratio of SCUBA-2 fluxes using a fixed dust opacity spectral index, β = 1.8, and a beam convolution kernel to achieve a common 14.8" resolution. We identify 82 clumps ranging between 10 and 36K with a mean temperature of 20{\pm}3K. Clump temperature is strongly correlated with proximity to the external OB association and there is no evidence that the embedded protostars significantly heat the dust. We identify 31 clumps that have cores with densities greater than 105cm{^{-3}}. Thirteen of these cores contain embedded Class 0/I protostars. Many cores are associated with bright-rimmed clouds seen in Herschel 70 μm images. From JCMT HARP observations of the 12CO 3-2 line, we find contamination of the 850μm band of up to 20 per cent. We investigate the free-free contribution to SCUBA-2 bands from large-scale and ultracompact H ii regions using archival VLA data and find the contribution is limited to individual stars, accounting for 9 per cent of flux per beam at 450 μm or 12 per cent at 850 μm in these cases. We conclude that radiative heating has potentially influenced the formation of stars in the Dust Arc sub-region, favouring Jeans stable clouds in the warm east and fragmentation in the cool west.
description: 27 pages, 25 figures, 7 tables, 3 online catalogues
Karakterisasi Parameter Fisik-Kimia Airtanah dan Analisis Infiltrasi Daerah Citatah-Cipangeran dan Sekitarnya, Kabupaten Bandung Barat, Provinsi Jawa Barat
Creators: name: Ericson, David
Publisher: name: Zenodo
Year: 2020
Subjects: padalarang
citatah
geologi
hidrogeologi

description: This presentation is based on David Ericson undergraduate final project in the Department of Geologi, Faculty of Earth Sciences and Technology, Institut Teknologi Bandung.
The Binggeli effect
Creators: name: Biernacka, Monika
name: Panko, Elena
name: Godlowski, Wlodzimierz
name: Bajan, Katarzyna
name: Flin, Piotr
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We found the alignement of elongated clusters of BM type I and III (the excess of small values of the Δθangles is observed), having range till about 60Mpc/h. The first one is probably connected with the origin of supergiant galaxy, while the second one with environmental effects in clusters, originated on the long filament or plane.
description: To appear as proceedings of the IAU Symposium 308 "The Zeldovich Universe, Genesis and Growth of the Cosmic Web"
Characterization of Saturn's bow shock: Magnetic field observations of quasi-perpendicular shocks
Creators: name: Sulaiman, A. H.
name: Masters, A.
name: Dougherty, M. K.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Collisionless shocks vary drastically from terrestrial to astrophysical regimes resulting in radically different characteristics. This poses two complexities. Firstly, separating the influences of these parameters on physical mechanisms such as energy dissipation. Secondly, correlating observations of shock waves over a wide range of each parameter, enough to span across different regimes. Investigating the latter has been restricted since the majority of studies on shocks at exotic regimes (such as supernova remnants) have been achieved either remotely or via simulations, but rarely by means of in-situ observations. Here we present the parameter space of MA bow shock crossings from 2004-2014 as observed by the Cassini spacecraft. We find that Saturn's bow shock exhibits characteristics akin to both terrestrial and astrophysical regimes (MA of order 100), which is principally controlled by the upstream magnetic field strength. Moreover, we determined the θBn of each crossing to show that Saturn's (dayside) bow shock is predominantly quasi-perpendicular by virtue of the Parker spiral at 10 AU. Our results suggest a strong dependence on MA in controlling the onset of physical mechanisms in collisionless shocks, particularly non-time stationarity and variability. We anticipate our comprehensive assessment will yield deeper insight into high MA collisionless shocks and provide a broader scope for understanding the structures and mechanisms of collisionless shocks.
description: Accepted in Journal of Geophysical Research: Space Physics
Adolescents' experience of psychoanalytically oriented psychotherapy
Creators: name: Mier, Carolyn.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Pipistrellus ceylonicus
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus ceylonicus

description: Pipistrellus ceylonicus (Kelaart, 1852). Prodr. Faun. Zeylanica, p. 22. TYPE LOCALITY: Sri Lanka, Trincomalee. DISTRIBUTION: Pakistan; India; Sri Lanka; Burma; Kwangsi and Hainan (China); Vietnam; Borneo. SYNONYMS: borneanus, chrysothrix, indicus, raptor, shanorum, subcanus, tonfangensis. COMMENTS: Subgenus Pipistrellus.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
Stability of superfluid vortices in dense quark matter
Creators: name: Alford, Mark G.
name: Mallavarapu, S. Kumar
name: Vachaspati, Tanmay
name: Windisch, Andreas
Publisher: name: arXiv
Year: 2016
Subjects: subject: Nuclear Theory (nucl-th)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Superfluid vortices in the color-flavor-locked (CFL) phase of dense quark matter are known to be energetically disfavored relative to well-separated triplets of "semi-superfluid" color flux tubes. However, the short-range interaction (metastable versus unstable) has not been established. In this paper we perform numerical calculations using the effective theory of the condensate field, mapping the regions in the parameter space of coupling constants where the vortices are metastable versus unstable. For the case of zero gauge coupling we analytically identify a candidate for the unstable mode, and show that it agrees well with the results of the numerical calculations. We find that in the region of the parameter space that seems likely to correspond to real-world CFL quark matter the vortices are unstable, indicating that if such matter exists in neutron star cores it is very likely to contain semi-superfluid color flux tubes rather than superfluid vortices.
description: 9 pages, 4 figures
Spin-orbit excitation energies, anisotropic exchange, and magnetic phases of honeycomb RuCl3
Creators: name: Yadav, Ravi
name: Bogdanov, Nikolay A.
name: Katukuri, Vamshi M.
name: Nishimoto, Satoshi
name: Brink, Jeroen van den
name: Hozoi, Liviu
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Using quantum chemistry calculations we shed fresh light on the electronic structure and magnetic properties of RuCl3, a proposed realization of the honeycomb Kitaev spin model. It is found that the nearest-neighbor Kitaev exchange K is weaker than in 5d5 Ir oxides but still larger than other effective spin couplings. The electronic-structure computations also indicate a ferromagnetic K in the halide, which is supported by a detailed analysis of the field-dependent magnetization. From exact-diagonalization calculations for extended Kitaev-Heisenberg Hamiltonians we additionally find that a transition from zigzag order to a spin-liquid ground state can be induced in RuCl3 with external magnetic field.
Limits in child psychoanalytic psychotherapy and their use as a technique for dealing with resistance
Creators: name: Rudd, Janice Elizabeth.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Stellar kinematics using a third integral of motion: method and application on the Andromeda galaxy
Creators: name: Kipper, Rain
name: Tenjes, Peeter
name: Tihhonova, Olga
name: Tamm, Antti
name: Tempel, Elmo
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We probe the feasibility of describing the structure of a multi-component axisymmetric galaxy with a dynamical model based on the Jeans equations while taking into account a third integral of motion. We demonstrate that using the third integral in the form derived by G. Kuzmin, it is possible to calculate the stellar kinematics of a galaxy from the Jeans equations by integrating the equations along certain characteristic curves. In cases where the third integral of motion does not describe the system exactly, the derived kinematics would describe the galaxy only approximately. We apply our method to the Andromeda galaxy, for which the mass distribution is relatively firmly known. We are able to reproduce the observed stellar kinematics of the galaxy rather well. The calculated model suggests that the velocity dispersion ratios $σ_z^2/σ_R^2$ of M31 decrease with increasing R. Moving away from the galactic plane, $σ_z^2/σ_R^2$ remains the same. The velocity dispersions $σ_θ^2$ and $σ_R^2$ are roughly equal in the galactic plane.
description: 12 pages, 8 figures, accepted to MNRAS
Pipistrellus circumdatus
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus circumdatus

description: Pipistrellus circumdatus (Temminck, 1840). Monogr. Mamm., 2:214. TYPE LOCALITY: Indonesia, Java, Tapos. DISTRIBUTION: Java, W Malaysia, Burma, NE India, SW China. SYNONYMS: drungicus. COMMENTS: Subgenus Arielulus.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
Mixing of a passive scalar by the instability of a differentially rotating axial pinch
Creators: name: Paredes, A.
name: Gellert, M.
name: Rüdiger, G.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The mixing of a passive scalar like lithium, beryllium or temperature fluctuations due to the magnetic Tayler instability of a rotating axial pinch is considered. Our study is carried out within a Taylor-Couette setup for two rotation laws: quasi-Kepler and solid-body rotation. The minimum magnetic Prandtl number used is 0.05 while the molecular Schmidt number Sc of the fluid varies between 0.1 and 2. An effective diffusivity coefficient for the mixing is numerically measured by the decay process of a global concentration peak located between the cylinder walls. We find that only models with Sc>0.1 do provide finite eddy diffusivity values. We also find that for quasi-Kepler rotation at a magnetic Mach number Mm~2 the flow transits from the slow-rotation regime to the fast-rotation regime. For fixed Reynolds number the relation between the normalized eddy diffusivity and the Schmidt number of the fluid is always linear so that also a linear relation between the instability-induced diffusivity and the molecular viscosity results just in the sense proposed by Schatzman (1977). The numerical value of the coefficient in this relation will reach a maximum at Mm~2 and will decrease for Mm>>1 implying that only toroidal magnetic fields of order kG can exist in the solar tachocline.
description: 7 pages, 8 figures, subm. to AA
Pipistrellus coromandra
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus coromandra

description: Pipistrellus coromandra (Gray, 1838). Mag. Zool. Bot., 2:498. TYPE LOCALITY: India, Coromandel Coast, Pondicherry. DISTRIBUTION: Afghanistan, Pakistan, India (including Nicobar Isis), Sri Lanka, Nepal, Bhutan, Burma, S China, Thailand, Vietnam. SYNONYMS: afghanus, blythii, coromandelicus, micropus, parvipes, portensis, tramatus. COMMENTS: Subgenus Pipistrellus. Does not include aladdin; see Corbet (1978c:53). See comment under P. pipistrellus.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
description: {"references": ["Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp."]}
Direct measurement of topological numbers with spins in diamond
Creators: name: Kong, Fei
name: Ju, Chenyong
name: Liu, Ying
name: Lei, Chao
name: Wang, Mengqi
name: Kong, Xi
name: Wang, Pengfei
name: Huang, Pu
name: Li, Zhaokai
name: Shi, Fazhan
name: Jiang, Liang
name: Du, Jiangfeng
Publisher: name: arXiv
Year: 2016
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Topological numbers can characterize the transition between different topological phases, which are not described by Landau's paradigm of symmetry breaking. Since the discovery of quantum Hall effect, more topological phases have been theoretically predicted and experimentally verified. However, it is still an experimental challenge to directly measure the topological number of various predicted topological phases. In this paper, we demonstrate quantum simulation of topological phase transition of a quantum wire (QW) using a single nitrogen-vacancy (NV) center in diamond. Deploying quantum algorithm of finding eigenvalues, we can reliably extract both the dispersion relations and topological numbers.
The use of eroticised transference and countertransference in the psychodynamic treatment of a seven and a half year old boy
Creators: name: Carver, Jennifer Anne.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Pipistrellus crassulus Thomas 1904
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus crassulus

description: Pipistrellus crassulus Thomas, 1904. Ann. Mag. Nat. Hist., ser. 7, 13:206. TYPE LOCALITY: Cameroon, Efulen. DISTRIBUTION: Cameroon, Zaire, S Sudan, N Angola. COMMENTS: Subgenus Pipistrellus.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
A Model for Lightcone Fluctuations due to Stress Tensor Fluctuations
Creators: name: Bessa, C. H. G.
name: De Lorenci, V. A.
name: Ford, L. H.
name: Ribeiro, C. C. H.
Publisher: name: arXiv
Year: 2016
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study a model for quantum lightcone fluctuations in which vacuum fluctuations of the electric field and of the squared electric field in a nonlinear dielectric material produce variations in the flight times of probe pulses. When this material has a non-zero third order polarizability, the flight time variations arise from squared electric field fluctuations, and are analogous to effects expected when the stress tensor of a quantized field drives passive spacetime geometry fluctuations. We also discuss the dependence of the squared electric field fluctuations upon the geometry of the material, which in turn determines a sampling function for averaging the squared electric field along the path of the pulse. This allows us to estimate the probability of especially large fluctuations, which is a measure of the probability distribution for quantum stress tensor fluctuations.
description: 9 pages, 2 figures
Building the Jupyter Community in Musculoskeletal Imaging Research - Proposal for the 3rd round of the Jupyter Community Workshop
Creators: name: Bonaretti, Serena
name: Burghardt, Andrew
name: Stok, Kathryn
name: Manske, Sarah
name: Barzegari, Mojtaba
name: Grassi, Lorenzo
name: Schileo, Enrico
name: Taddei, Fulvia
name: Carballido-Gamio, Julio
Publisher: name: Zenodo
Year: 2022

description: Accepted proposal for the 3rd round of Jupyter Community Workshop Find two documents in this repository: - Accepted proposal without budget - Accepter proposal with budget included Webpage of the workshop at: https://github.com/JCMSK/2022_JCW/blob/main/README.md
A new and simple model for magneto-optics uncovers an unexpected spin switching
Creators: name: Zhang, G. P.
name: Bai, Y. H.
name: George, Thomas F.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In magneto-optics the spin angular momentum $S_z$ of a sample is indirectly probed by the rotation angle and ellipticity, which are mainly determined by the off-diagonal susceptibility $χ^{(1)}_{xy}$. A direct and analytic relation between $S_z$ and $χ^{(1)}_{xy}$ is necessary and of paramount importance to the success of magneto-optics, but is often difficult to acquire since quantum mechanically the relation is hidden in the sum-over-states. Here we propose a new and simple model to establish such a much needed relation. Our model is based on the Hookean model, but includes spin-orbit coupling. Under cw excitation, we show that $χ^{(1)}_{xy}(ω)$ is indeed directly proportional to $S_z$ for a fixed photon frequency $ω$. Such an elegant relation is encouraging, and we wonder whether our model can describe spin dynamics as well. By allowing the spin to change dynamically, to our surprise, our model predicts that an ultrafast laser pulse can induce a spin precession; with appropriate parameters, the laser can even reverse spin from one direction to another. This works for both the circularly and linearly polarized light. The spin reversal window is narrow. These unexpected results closely resemble all-optical helicity-dependent magnetic switching found in much more complicated ferrimagnetic rare earth compounds. Therefore, we believe that our spin-orbit coupled model may find some important applications in spin switching processes, a hot topic in femtomagnetism.
description: 6 pages, 2 figures
Breastfeeding, ambivalence and the psyche-soma of the infant : a study based on an infant observation
Creators: name: Adler, Jacqueline.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Pipistrellus cuprosus Hill and Francis 1984
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus cuprosus

description: Pipistrellus cuprosus Hill and Francis, 1984. Bull. Brit. Mus. (Nat. Hist.) Zool., 47:312. TYPE LOCALITY: Borneo, Sabah, Sepilok. DISTRIBUTION: Borneo. COMMENTS: Subgenus Arielulus.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 220, DOI: 10.5281/zenodo.7353060
Pipistrellus dormeri
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Pipistrellus
Pipistrellus dormeri

description: Pipistrellus dormeri (Dobson, 1875). Proc. Zool. Soc. Lond., 1875:373. TYPE LOCALITY: India, Mysore, Bellary Hills. DISTRIBUTION: NW, S and E India, Pakistan, perhaps Taiwan. SYNONYMS: caurinus. COMMENTS: Subgenus Scotozous. Sometimes placed in a separate genus, Scotozous; see Tate (1942«:259) and Corbet and Hill (1980:68); but also see Ellerman and Morrison-Scott (1951:162-163) and Corbet (1978c:51).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on pages 220-221, DOI: 10.5281/zenodo.7353060
description: {"references": ["Corbet, G. B., and J. E. Hill. 1980. A world list of mammalian species. British Museum (Natural History), London, 226 pp.", "Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp.", "Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp."]}