cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25911/5c36da3ee4787
title: Upland Heath Swamps Plot Network: Plot Details - Spatial Coordinates, Dharawal National Park, Sydney Basin, NSW, Australia
title: Upland Heath Swamps Plot Network: Spatial data Dharawal National Park

description: This dataset contains spatial information for plots established in the Dharawal National Park. Sampling of soil is stratified along the soil moisture gradient and across the range of structural variability in the vegetation. 

A synopsis of related data packages which have been collected as part of the Upland Heath Swamps Plot Network’s full program is provided at https://doi.org/10.25911/5c1313b2b2644.
description: Abstract: This dataset contains spatial information for plots established in the Dharawal National Park. Sampling of soil is stratified along the soil moisture gradient and across the range of structural variability in the vegetation. Thus three categories of soil moisture and three categories of vegetation structure (based on the height and form of shrubs) are sampled in a factorial design at 60 sites in upland swamps scattered throughout the study area (Keith and Myerscough 1993). Each permanent swamp monitoring site consists of a belt transect of 30 contiguous 0.5x0.5 metre quadrats. Quadrats 1 and 30 are marked with steel star pickets, extending approximately 1.5 m above ground surface. 

This spatial data complements data collected from soil moisture, soil properties, vegetation and hydrological climate surveys conducted at these sites. 

A synopsis of related data packages which have been collected as part of the Upland Heath Swamps Plot Network’s full program is provided at https://doi.org/10.25911/5c1313b2b2644.

Between 2012 and 2018 this project was part of, and funded through the Long Term Ecological Research Network (LTERN) a facility within the Terrestrial Ecosystem Research Network (TERN) and supported by the Australian Government through the National Collaborative Research Infrastructure Strategy.
DOI: 10.25919/5c36da4546509
title: Current and future storm tide risks for Samoa.

description: Current and future storm tide risk study for Samoa.  These risks are quantified by estimating 20, 50 and 100 year maximum storm tide height return intervals under a variety of climate conditions and sea levels using a combined statistical/dynamical method.

Access to this data is restricted and relies on scripts.

This data collection comprises ~50 GB &gt;10000 files Tropical Cyclone Tracks, Storm tide model runs, other input information, derived statistical gridded data.
DOI: 10.25919/5c36da5047914
title: Parkes observations for project P737 semester 2014OCTS

description: Pulsar observations using the Parkes radio telescope have led to some of the most exciting astronomical results in the last few years.  The aim of this proposal is to carry out tests of the new backend instruments which cannot be carried out during standard maintenance periods. High precision pulsar timing experiments require cross-coupling in the feed to be measured.  This can only be done using observations of PSR J0437-4715 from rise-to-set.  We propose to undertake such observations and make the results available for any users of the telescope.
DOI: 10.25919/5c36da5966cd7
title: Parkes observations for project P456 semester 2014OCTS

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on gravitational waves until they are finally detected. Continued Parkes observations will remain valuable until the first stage of the SKA is able to offer the same sensitivity as Parkes and the same observing time. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5c36da62b575b
title: Phreeqc model for MARSUO infrastructure and water quality impact assessment

description: Model input and output files used in equilibrium modelling to evaluate the potential for pipe scale, corrosion and water quality changes due to interaction between various water sources and pipe materials.
DOI: 10.25919/5c36da7e9449b
title: Gascoyne Airborne Electromagnetic (AEM) Project Survey Data: Borehole Data

description: This Collection contains borehole data used in the Gascoyne AEM Project prior to the drilling campaign launched in 2014.  All borehole information is contained in xml structures.
DOI: 10.25919/5c36da8ea0418
title: Gascoyne Airborne Electromagnetic (AEM) Project Survey Data: Ground-based TEM

description: This Collection contains the dbdt data collected by CSIRO as part of a ground-based TEM survey conducted along selected boreholes in the Gascoyne AEM Project Survey Area.
DOI: 10.25919/5c36da997be5b
title: Gascoyne Airborne Electromagnetic (AEM) Project Survey Data: Processing and Inversion

description: Internal processing and inversion data files for the Gascoyne River AEM Project.  The data was processed and inverted using the Arhus workbench program.  Here we provide the final processed and inverted data that was used in the  Project.  Data is in ASCII format.  This Collection includes:
Point located data for low moment and high moment SkyTEM 304 data used in the inversions;
Inverted data;
A text file that shows which channels and fiducials have been culled from the dataset.
DOI: 10.25919/5c36daa377583
title: Lower Limestone Coast Prescribed Wells Area wetland-groundwater interaction model, version 1.0

description: This model demonstrates a methodology for simulating interactions between wetlands and underlying shallow groundwater in the Lower Limestone Coast Prescribed Wells Area. Specifically, the model simulates changes in wetland water levels to variations in water tables. A variant of the industry standard groundwater flow simulation code MODFLOW (i.e. MODFLOW-OWHM) was used as the basis for this approach. Significant components of the water mass balances for both wetland and groundwater domains were included. Of particular novelty was the use of a combined approach to simultaneously represent recharge and evapotranspiration. Model files also include Python language post-processing scripts, which may be used to produce statistical summaries of wetland surface water persistence.
The model was demonstrated using a synthetic input dataset. Results of the synthetic demonstration, including the calculated salinisation risk metric, indicated the potential for managed surface water additions to negate the effects of long-term water table decline on the persistence of wetland surface water levels.
DOI: 10.25919/5c36daaf46683
title: Coastal bank erosion and river load data, Western Port Bay

description: This data was collected as part of two research projects commissioned by Melbourne Water that investigate the rates and processes of coastal bank erosion in Western Port Bay, Victoria. 
Most of the timeseries data commences in Nov or Dec 2012 and extends to the date of upload (currently October 2015 or earlier for some parameters). The initial project ceased in December 2013. A phase 2 project continues until December 2016, and coastal bank erosion monitoring continues until ~June 2016 as part of that project.

The data includes: 
*GIS layers and air photos that were used to determine long term changes in the position of the coastline. The photos start from 1947 and cover an 8.6 km stretch of banks near Lang Lang.
*15-minute tide and groundwater peizometer data collected from the monitoring site near Lang Lang
*30-minute climate data recorded by the Davis weather station installed at the monitoring site.
*Photos of the site at high and low tide each day until Nov 2013.
*Total Suspended Solids loads for monitoring sites on four streams draining to Western Port. Loads were calculated from available discharge, TSS concentration and turbidity monitoring data

Further information on the data is provided in the supporting attachment (Information.pdf)
DOI: 10.25919/5c36dab991fb8
title: Water Level Climatologies for Pacific Island Countries

description: Components of total hourly sea level signal, monthly exceedance probabilities, and gridded tides and sea level anomaly.

Access to this data collection is restricted and relies on scripts.

The data collection comprises ~4 GB, &gt;10000 files comprising processed hourly sea level files, weekly averaged altimetry files, and derived gridded products.
DOI: 10.25919/5c36dad071098
title: Gascoyne Airborne Electromagnetic (AEM) Pjoject Survey Data: Grids

description: This Collection holds the grids used in the Gasoynce AEM Project for the planned drilling campaign.
DOI: 10.25919/5c36dad97444f
title: Acquisition and Processing Report SkyTEM Helicopter EM Survey Gascoyne Area Project, Western Australia

description: This collection contains the raw and processed data from a helicopter-borne airborne electromagnetic (AEM) survey over the lower reaches of the Gascoyne River near Carnarvon, Western Australia.  It contains information about the survey statistics, aqcuisition parameters and processing that was completed by Groundprobe Geophysics for the Department of Agriculture and Food, Western Australia (DAFWA) and CSIRO.
DOI: 10.25919/5c36dae2b2d69
title: Gascoyne Airborne Electromagnetic (AEM) Project Survey Data: Workbench Workspace

description: This is the complete workspace for the Gascoyne AEM Project.  The workspace is only able to be open in the Arhus Workbench program, a propietary program for processing and inverting AEM data.
DOI: 10.25919/5c36daf16a531
title: Parkes observations for project P887 semester 2015APRS

description: Searches for radio pulsations from Fermi sources have been astonishingly fruitful, both in discovering new pulsars and in probing the physics of high-energy emission.  We propose observations of members of two promising Fermi source classes: (1) candidate enshrouded millisecond pulsars (2) new "blind search" gamma-ray pulsars.  The former are fascinating systems in which the wind of an energetic recycled millisecond pulsar is disintegrating its companion; detecting pulsations turns them into laboratories for this process.  The latter are pulsars recently discovered in computational tour de force trawls of the Fermi data.  Radio pulsations greatly add to the information we can obtain; conversely, deep upper limits constrain emission models.
DOI: 10.5061/dryad.646v2r1/1
title: systox.tar

description: All necessary code and data is housed within this archive. The archive should have an md5 checksum d56eabd45e46af9f28d7936bd7390899. 
The code is version controlled and any updates can be found at https://github.com/pvtodorov/systox .
The data is also stored on synapse.org as syn11697964.
The code and data within this repo are released under the CC Zero license.
DOI: 10.25919/5c36db2a9afed
title: Parkes observations for project P892 semester 2015OCTS

description: SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Recent results show that there is a strong latitude dependence to FRB detectability so SUPERBx will search above 25 degrees in Galactic latitude. It will use optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (Molonglo, GMRT, MWA) to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors.
DOI: 10.25919/5c36db33039fd
title: GFLOWS Hydrogeological Framework Model

description: Derived hydrogeology dataset of the Eyre Peninsula region in South Australia
DOI: 10.25919/5c36db3fc389f
title: Parkes observations for project P888 semester 2015OCTS

description: Erratically-emitting neutron stars like Rotating Radio Transients (RRATs), represent approximately 3% (and increasing) of radio-emitting pulsars as they are found via searches of archival and current pulsar surveys. The sporadic emission from these sources makes them difficult to study and nearly all information about the properties of the objects is the result of dedicated monitoring and timing programs at Parkes telescope. This project represents an effort to obtain accurate timing solutions and polarization profiles of a sample of sparse-emitting pulsars. We will monitor and time 6 sources to determine basic RRAT properties including spin period, spin period derivative, and polarization properties. Thus enabling us to identify physical causes for the extreme emission, enable high-energy follow-up observations, deduce how these pulsars are related to the general pulsar and magnetar populations, and explore the distribution of extreme radio intermittence in neutron stars.
DOI: 10.25919/5c36db4b82fae
title: RV Investigator Voyage IN2015_E01 End of Voyage (EOV) Archive

description: This record describes the End of Voyage (EOV) archive from the Marine National Facility RV Investigator trial voyage IN2015_E01 - Cold Water Trial voyage (including Atmospherics). This voyage took place from Hobart to Hobart from the 29th January to 18th February 2015 and went to 65 degrees south. 

The voyage objectives included testing the cold water and atmospheric operations; the collection and processing of data and samples to test laboratories, facilities and on board systems; specific testing and checks of aerosol sampling mast, aerosol laboratory and air-chemistry laboratory. Geophysical Survey Mapping data collection, including instrument calibrations, testing of equipment and deployments of XBTs. Data Acquisition operations including the integration and test of underway instruments, new atmospheric instruments and drop keel instrumentation.

Data collected included Acoustic Doppler Current Profiler (ADCP)(75, 150 KHz), Underway (UWY), Gravity, SST Radiometer, Atmospheric data (Absorption Photometer, Nephelometer, Ozone and Radon), Greenhouse data (Aerodyne and Picarro), Underway pCO2, Echosounders (12, 18, 38, 70, 120, 200, 333, Bridge 200 KHz), Multibeam (EM122, EM710, ME70 and SBP120) and XBT. 

Additional Aerosol data collected included TSI 3772 Condensation Particle Counter (CPC), 3787, Time of flight aerosol chemical speciation monitor (ToF-ACSM), Cloud Condensation Nuclei Counter (CCN), Spectronus - trace gas analyser based on Fourier Transform Infrared spectrometry (FTIR), Long Scanning Mobility Particle Size (longSMPS), Nano Scanning Mobility Particle Size (nanoSMPS), Neutral Cluster Air Ion Spectrometer (NAIS), Proton Transfer Reaction Mass Spectrometer (PTR-MS), PTRMS_AUX, Radiosondes_balloons, Sequencer (SEQ) and Volatility Hygroscopicity Tandem Differential Mobility Analyser (VHTDMA).
    
The EOV paper documentation - Multibeam (EM122, EM710, ME70 and SBP120), Gravity Meter and XBT logs are scanned, archived and entered in the records management system TRIM, reference "in2015_e01". ELOG files are generated as .csv and archived. All voyage documentation is archived c/o the Data Centre in Hobart available electronically to MNF support via the local network "global_docs". Access to voyage documentation for non CSIRO participants can be made via DataLibrariansOAMNF@csiro.au.

The archive for the IN2015_E01 EOV data will be held temporarily within the CSIRO Oceans and Atmosphere Data Centre in Hobart with a permanent archive to be located at the CSIRO Data Access Portal (DAP), providing access to participants and processors of the data collected on the Marine National Facility RV Investigator IN2015_E01.
DOI: 10.25919/5c36db5917016
title: Parkes observations for project P427 semester 2015APRS

description: Timing of the dozen pulsars discovered in six globular clusters by us in the framework of P303 and timed in the context of P427 has ensured high quality results, which have been reported in several papers, three more of which are in preparation.  We now propose to continue our timing project, performing a small number of visits to the six globular clusters, in order to measure higher order derivatives of the rotational and/or of the orbital parameters of the pulsars and to safely keep coherence in the timing solutions. With a very limited investment of additional telescope time, that will enable studying some poorly constrained aspects of the inner dynamics of the observed globular clusters, as well as providing the ephemeris for the best possible searches for gamma-ray and/or gravitational wave emission from the targeted pulsars.
DOI: 10.25919/5c36db61ea6ce
title: Parkes observations for project P858 semester 2015APRS

description: SUPERB is a large-scale survey for pulsars and extragalactic radio bursts. It will uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The pulsars discovered will enable studies of the interstellar medium, allow us to more accurately constrain the MSP luminosity function (which informs estimates of the SKA yield of MSPs), tests of theories of gravity and several will contribute to the precision timing projects of the PPTA. The FRBs discovered will have much more associated information than all previous detections. Firstly the discovery lag will be ~1 second, rather than months/years. The Parkes observations will be shadowed by the Molonglo telescope to allow, for the first time, localisation of FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors. The survey will discover ~20 MSPs, ~100 slower pulsars and ~10 FRBs.
DOI: 10.25919/5c36db69ec18c
title: Parkes observations for project P887 semester 2015APRS

description: Searches for radio pulsations from Fermi sources have been astonishingly fruitful, both in discovering new pulsars and in probing the physics of high-energy emission.  We propose observations of members of two promising Fermi source classes: (1) candidate enshrouded millisecond pulsars (2) new "blind search" gamma-ray pulsars.  The former are fascinating systems in which the wind of an energetic recycled millisecond pulsar is disintegrating its companion; detecting pulsations turns them into laboratories for this process.  The latter are pulsars recently discovered in computational tour de force trawls of the Fermi data.  Radio pulsations greatly add to the information we can obtain; conversely, deep upper limits constrain emission models.
DOI: 10.25919/5c36db7523d0b
title: Parkes observations for project P427 semester 2015APRS

description: Timing of the dozen pulsars discovered in six globular clusters by us in the framework of P303 and timed in the context of P427 has ensured high quality results, which have been reported in several papers, three more of which are in preparation.  We now propose to continue our timing project, performing a small number of visits to the six globular clusters, in order to measure higher order derivatives of the rotational and/or of the orbital parameters of the pulsars and to safely keep coherence in the timing solutions. With a very limited investment of additional telescope time, that will enable studying some poorly constrained aspects of the inner dynamics of the observed globular clusters, as well as providing the ephemeris for the best possible searches for gamma-ray and/or gravitational wave emission from the targeted pulsars.
DOI: 10.25919/5c36db84f051d
title: Continental-scale spatial phylogenetics of Australian angiosperms

description: The data in this folder were used in the spatial phylogenetic study of the Australian angiosperm genera by Thornhill et al. 2016.
DOI: 10.25919/5c36db8d6e201
title: Parkes observations for project P456 semester 2015OCTS

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on gravitational waves until they are finally detected. Continued Parkes observations will remain valuable until the first stage of the SKA is able to offer the same sensitivity as Parkes and the same observing time. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.25919/5c36db9685bdb
title: Parkes observations for project P878 semester 2014OCTS

description: Measuring the magnetic field and electron density of the solar wind is essential in order to understand the properties of solar corona. Detection of dispersion measure (DM) and Faraday rotation measure (RM) of linearly polarized radio sources occulted by the solar wind provides a unique opportunity to measure these properties. Pulsars are therefore ideal sources for such study, especially for millisecond pulsars which can be used to obtain high timing precision to measure the DM variations caused by the solar wind.  Two millisecond pulsars, PSRs J1730-2304 and J1824-2452A with ecliptic latitude of only 0.19 and -1.55 degree are ideal for this work as the line-of-sight to these pulsars goes very close to the Sun; the closest approach is only 0.8 and 5.8 solar radii respectively. We can use these two pulsars detect the different regions of the solar coronal, such as solar equator and south pole region. We also propose a unique study of the solar corona on small physical scales using the lines-of-sight to multiple pulsars in the M28 globular cluster.