The RAN Australian Hydrographic Service conducted hydrographic survey HI514 at Mawson, February to March 2012. The areas surveyed were the entrance to Horseshoe Harbour and the western side of West Arm. There is also a single line of soundings east of Evans Island. The survey dataset, which includes the Report of Survey, was provided to the Australian Antarctic Data Centre by the Australian Hydrographic Office and is available for download (see a Related URL). The vertical datum of the soundings is Lowest Astronomical Tide, 0.83 metres below Mean Sea Level. The survey was lead by LT C.E.Diplock. The data are not suitable for navigation.

A high resolution bathymetric grid of the nearshore area at Casey station, Antarctica was produced by Geoscience Australia by combining data from two multibeam hydrographic surveys: 1) A survey conducted by the Royal Australian Navy in 2013/14. Refer to the metadata record 'Hydrographic survey HI545 by the RAN Australian Hydrographic Service at Casey, December 2013 to January 2014' with ID HI545_hydrographic_survey. 2) A survey conducted by Geoscience Australia and the Royal Australian Navy in 2014/15. Refer to the metadata record 'Hydrographic survey HI560 by the RAN Australian Hydrographic Service at Casey, December 2014 to February 2015' with ID HI560_hydrographic_survey and the metadata record 'Seafloor Mapping Survey, Windmill Islands and Casey region, Antarctica, December 2014 - February 2015' with ID AAS_3326_seafloor_mapping_casey_2014_15. The grid has a cell size of one metre and is stored in a UTM Zone 49S projection, based on WGS84. Further information is available from the Geoscience Australia website (see a Related URL).

This dataset (provided as a series of CF-compatible netcdf file) consists of 432 consecutive maps of Antarctic landfast sea ice, derived from NASA MODIS imagery. There are 24 maps per year, spanning the 18 year period from March 2000 to Feb 2018. The data are provided in a polar stereographic projection with a latitude of true scale at 70 S (i.e., to maintain compatibility with the NSIDC polar stereographic projection).

Imagery of Aurora Australis and sea ice captured by a 'quadcopter' (Inspire) drone launched from the ship

In January 2005 a multi-parametric international experiment was conducted that encompassed both Deception Island and its surrounding waters. This experiment used as main platforms the Spanish Oceanographic vessel 'Hesperides', the Spanish Scientific Antarctic base 'Gabriel de Castilla' at Deception Island and four temporary camps deployed on the volcanic island. This experiment allowed us to record active seismic signals on a large network of seismic stations that were deployed both on land and on the seafloor. In addition other geophysical data were acquired, such as: bathymetric high precision multi-beam data, and gravimetric and magnetic profiles. During the whole period of the experiment a multi-beam sounding EM120 was used to perform bathymetric surveys. The characteristic of this sensor permitted to reach up to 11.000 m b.s.l. In table 2 we provide some of its main characteristics. During the experiment different bathymetric profiles were performed with this equipment outside of Port Foster. Some of these images already have provide an accurate vision of the region, and were used to estimate the real size of the water column locate below each shoot. Additional information of these data could be found in the Lamont-Doherty Earth Observatory at IEDA Marine Geoscience Data System (http://www.marine-geo.org/). It is possible to access the summary of downloads that were made of these data and documents at http://www.marine-geo.org/about/downloadreport/person/Ibanez_Jesus/2016A.

Taken from sections of the report: Introduction This report details the survey work carried out on Macquarie Island during January of 1996 by AUSLIG on behalf of Australian Antarctic Divisions Mapping Program. The principle aim of this work was to acquire aerial photography of the island so that a new topographic map of the island can be produced. A number of other tasks were also carried out. In the following pages each task will be dealt with in terms of the technique employed and the results achieved. The survey work was carried out by the following people : Paul Boland Tasmania Department of Environment and Land Management, Troy Lee Antarctic Division Volunteer, Stuart Smith Antarctic Division Volunteer, Roger Handsworth Platypus Engineering, Noel Ward AUSLIG. This report does not cover the specifics of the work carried out by Paul Boland or Roger Handsworth, that being the subject of separate reports to be submitted by them. Time Frame The Macquarie Island survey field party departed Hobart at 3pm on Thursday 4th of January 1996 aboard MV Polar Bird, voyage 3.1 of the Antarctic re-supply season. Voyage 3.1 arrived at Macquarie island at about 5am eastern summer time (UT+11) on Sunday 7th of January 1996. The survey party departed Macquarie Island on 12th of January aboard MV Polar Bird, voyage 3.1, at about 0:50am local time. Voyage 3.1 returned to Hobart on Sunday the 14th of January. All passengers where disembarked at about 6pm that day. Aim and Project Brief The survey program, as detailed by Antarctic Division in its Brief to Surveyors, comprised the following tasks, this document is included as Appendix A 1. Attempt aerial photography of the whole island, 2. Mark the boundaries of the Historic Zone and Zone A in the vicinity of the Isthmus, 3. Field check the new station facilities information system, including the location of all masts, antennae, guys and walkways. 4. Positioning of ERS-1 and 2 corner cube reflectors, 5. Precise levelling, 6. Fix, by GPS, survey marks AUS 157 and AUS 158. 7. Precise GPS connection from the ARGN site to the Hurd Point Tide Gauge site.

Taken from sections of the report: Introduction This report describes aspects of the fieldwork completed for the Australian Antarctic Division (AAD) mapping program during the Austral summer 2003-04. The mapping program was undertaken in harmony and collaboration with the Geoscience Australia geodesy program in Antarctica, between 16th November 2003 and 2nd February 2004. Surveyors from both organisations, including Henk Brolsma (Mapping Officer, AAD) and A. Corvino (author), teamed up to successfully complete a wide range of goals. The principal objective of the Geoscience Australia geodesy program was to install three remotely located continuous GPS stations in the southern Prince Charles Mountains (PCM) and Grove Mountains (Corvino, 2004). That project is not discussed further in this report. The main objectives of the AAD mapping program were to survey ground control points (GCPs) for geo-referencing new satellite imagery and to complete terrestrial survey work in the vicinity of Davis station. The following tasks were completed: - Downloading of the tide gauges at the Larsemann Hills and Davis station; - Transfer of local sea level at the Davis tide gauge to an absolute height datum using GPS; - Establishing a new survey mark at Beaver Lake and connecting it to the existing survey marks; - Conducting GPS surveys of selected ground features for geo-referencing satellite imagery at Beaver Lake, Marine Plain, the Grove Mountains and Wilson Bluff; - Establishing new survey marks at Marine Plain in the Vestfold Hills; - Computing the alignment of the UWOSCR instrument in the Space and Atmospheric Sciences (SAS) building at Davis station; - Surveying lake levels in the Vestfold Hills; and - Various local surveying tasks at Davis station. A few aspects of the fieldwork that were completed exclusively by surveyor Brolsma are not included in this report. In particular the report is concerned with the tasks that were undertaken using GPS survey methods, which includes the tide gauge surveys, image control surveys and the fieldwork at Beaver Lake and Marine Plain. Photographs that document the fieldwork and support the text are included throughout. GPS processing reports and photographs showing the locations of the GCPs are provided as Appendices.

Digital Elevation Model of the Amery Ice Shelf derived from ERS satellite radar altimetry elevation data. Generated on a 1-km polar stereographic grid using kriging in four sections by Helen Amanda Phillips, Antarctic CRC/IASOS. Three files are available for download: Amery Ice Shelf DEM from satellite altimeter data version relative to WGS-84 ellipsoid, Amery Ice Shelf DEM from satellite altimeter data version relative to EGM96 geoid, A thickness dataset that was derived from the AIS-DEM. Each file constitutes 122,385 lines of data (+ 4 lines of header information). The fields in this dataset are: Latitude Longitude Geodial Height in metres above sea level (WGS-84 and EGM-96) Thickness

This dataset comprises oblique aerial photographs of multiple Adelie penguin breeding sites in East Antarctica. The photographs were taken using hand-held digital cameras from fixed-wing aircraft and helicopters used by the Australian Antarctic Program. The aircraft flew at or above the minimum wildlife approach altitude of 750 m with a horizontal offset distance from the site of approximately 500-600m. The date and exact location of the aircraft when each photo was taken is embedded in the EXIF data of each photo. All photographs that were taken are included despite varying image quality due to environmental conditions, camera type and altitude. Generally an attempt was made to photograph the entire breeding site (usually an island, occasionally an outcrop of continental rock) with a series of zoomed, overlapping photos. Sometimes this was not possible when the site was large, and in these cases the overlapping photos covered the locations where colonies were known to exist from previous survey work. In some cases a site was over-flown at an altitude of 1200m so that a single photo of the entire site could be taken. These photos are useful in piecing together the detailed photos. The database of potential Adelie penguin breeding habitat in Southwell et al. (2016a) was used to associate photos to a particular breeding site and structure how the photos are stored. The breeding site database has a unique identifying code of every site of potential breeding habitat in East Antarctica, and the sites are aggregated into sub-groups and then groups. The file structure in which the photos are stored has a combination of ‘group’ and ‘split-year breeding season’ at the top level (eg VES 2015-16 contains all photos in group VES (Vestfold Hills and islands) taken in the 2015-16 breeding season). Within each group-year folder are sub-folders for each breeding site where photos were taken (eg IS_72276 is Gardner Island in the VES group). If an overview photo was taken there are separate sub-folders for overview and detailed photos in the site sub-folder. These data also superseded an earlier dataset of 2009-2016 data - https://data.aad.gov.au/metadata/records/AAS_4088_Adelie_oblique_photos Please refer to the Seabird Conservation Team Data Sharing Policy for use, acknowledgement and availability of data prior to downloading data.

Introduction The purpose of the 97/98 Antarctic survey season was to provide survey control and vertical and oblique aerial photography around Mawson, Davis, Beaver Lake, and the Prince Charles Mountains in support of the ANARE mapping program as well as providing survey support for other ANARE science programs. The following team carried out this survey work: Christopher Watson - Antarctic Division Volunteer Surveyor, John Hyslop - LANDINFO Surveyor. Project Outline The Antarctic Division's Brief to Surveyors which outlines the details of the program is included in Appendix A. The survey program for Antarctica 97/8 was divided into two main areas of interest. Mawson station from Voyage 2 to 4 which included photo control of offshore islands, aerial photography of penguin colonies with the Linhof camera, Mawson tide gauge network and updating the station map. Davis station from Voyage 4 to 5 which included aerial photography of the Rauer Group and Larsemann Hills, aerial photography and tide gauge work at Beaver Lake, and vertical and oblique aerial photography in the Southen Prince Charles Mountains. Also photo control at Scullin and Murray Monoliths and photography at Mount Brown, Mirny offshore island and features between Mirny and Davis. At Davis station surveys included Station detail surveys tide gauge connections and lake water levels in the Vestfold Hills. At Casey station during V2 stop over survey work was requested at the wharf area, levelling and detail survey updates. Recommendations: Aerial photography. The following suggestions are made. 1. The flight program be upgraded to allow a digital map to be shown on the screen. 2. The pilots display did not work in the helicopter and the problem needs to be fixed. I suspect it may have been due to the setting in the flight program. I had difficulty understanding what all the settings meant and perhaps more documentation may help. 3. Because of 2. more reliance was placed on the air crew navigating from the monitor and hence felt the need for more control over the display eg. Zooming in and out and run selection. 4. A video drift sight would be a great advantage. If this were somehow attached directly to the camera there would be more room and less leads involved. 5. Some of the film spools were too tight on the cogged drive shaft. At Beaver Lake when loading film in a black camera bag in the helicopter I had to wind the new film onto another spool that would fit. The spools need to be checked. Logistics. The need to return the helicopter to Davis each day seems to me to be an extremely expensive requirement. To get to the Southern Prince Charles Mountains is an eight hour return trip. 11 hour flying is about all the pilots can do in a day which does not leave much time for productive work. We did have an opportunity to do aerial photography on the way but on the two days we went to the PCMs we decided to make the first priority the main destination and hope for time on the return trip, but each occasion we were too late and returned by the most direct route. I could not help thinking how much more work we could have done if the helicopters had been based at Beaver Lake for a few days. There were also days when the weather was fine and suitable for flying in the PCMs but we could not leave Davis through bad weather on the way. This method of operation also understandably placed pressures on using the helicopters to the fullest. The last days flying in the PCMs was done with 4 people in the back of the S76. We then were asked if we could take 300kg of equipment back from a Mawson Escarpment camp. That made photographic operation a bit cramped but by then the weather was against further photography. I felt that through Joe Johnson, station leader and Jim Wilson, chief pilot we got excellent support for the photographic program but with the S76 deployed in the area of operation we could have achieved a lot more.