History
Althought civilian air activity was common in Alice Springs since 1920, the military buildup in the north of Australia in the late 1930s saw the need for the establishment of an airport that could receive larger and heavier aircraft. Thus, the Australian Department of Defence decided to built in 1940 the Seven Mile Aerodrome shifting the operations from the already established Town Site Drome. Altought civilian aircraft were allowed to use the airport, due to his strategic location, during World War II its primary purpose was military, being used primarily by the Royal Australian Air Force (RAAF) and the United States Air Force, as the main transit base for transport planes bringing troops and supplies into the Pacific Theater of Operations and as a refuelling and staging facility. At the end of the war, the military left the aerodrome and it returned to civilian use.
By 1946 several improvements were made including the installation of the first underground fuel tanks, a VHF radio range and meteorological facilities. In 1958 the aerodrome became officially known as Alice Springs Airport and in 1961 a major improvement was made with the reconstruction of part of the existing Runway 12/30 and its extension to 2,4 km of longitude. In 1965, the construction of a new passenger terminal and a fire station near the old installation marked the complete transfer of all activity to the current building area. The only facilities that remained active then at the original airfield site (referred even today as the "Seven Mile Area") were those devoted to maintenance tasks.
First uses of the airport to launch balloons
In 1960 was established on behalf the Departament of Supply (DOS) the first Australian Balloon Launch Station (ABLS) which was located at the Mildura airport in Victoria. The main activity there was to support an atmospheric sampling program carried out by the United States Atomic Comission under a first intergovernment agreement which lasted almost seven years and that allowed the launch of near 600 balloons from the station. Once finished a new document was signed reducing sharply the amount of missions devoted to the sampling effort but at the same time diversifying the research aims of the flights to other branches of Science as well to other users.
Scientific groups from around the world, realizing the potential of Australia as an excellent site for ballooning, became increasingly interested in performing flights from various locations within the continent. The southerly latitude, combined with the large land mass in the east-west direction could yield extended observation times for astrophysical sources not easily visible from the northern hemisphere. One of those locations was precisally the airport of Alice Springs from which were carried out many experiments in the field of Gamma Ray and X-Ray astronomy on those years.
Obviously in that times, the airport lacked of dedicated facilities so the balloon launches were performed under Mildura ABLS managment: generally all the necessary equipment and staff was transported by road and rail to Alice Springs during each campaign. There were three main reasons to make such an effort each year: Population, Winds and Location.
The very low population density over Central Australia allowed to use heavy payloads and big balloons with less security restrictions and with very safe termination process margins, though the prevalence of semi-desertic landscapes over most of this region difficulted somewhat the recovery operations.
On regard the wind pattern, Alice Springs has two features worth noting: a low wind velocity regime that dominates the altitude range of 90,000 ft. to 110,000 ft. between March and November, giving a long period when flights with payloads that not need extreme altitudes (i.e. infrared) can be carried out and two turnaround periods, one in the October-November window with a duration of three to five weeks of slow moving winds above 120,000 ft and the other in March-April with somewhat short duration. With careful preparation and timing, turnaround flights of over 60 hr duration can be achieved.
Finally, the site offered too better observing conditions than Mildura specially due to its latitude located nearer the declination of the Galactic Centre region along with a higher vertical cut-off rigidity.
All these factors led to the first era of scientific ballooning in Alice Spring, which would extend during the entire 70's decade.
Basic infrastructure
The launch of the balloons is carried out from two runways which are closed to air traffic during the operations. For inflation, Helium gas is used instead of Hydrogen as the extremely dry air of the zone can generate dangerous estatic discharges during balloon inflation.
As mentioned, the launch equipment available at the station is the same used for balloon operations at Mildura ABLS and allowed to launch balloons with a volume of up to 46.000.000 cubic feet, and payloads weighting up to 2 tons.
On regard telemetry, the LOS (Line of Sight) hardware is composed of receivers for downlink telemetry channels operating on 234.4, 253.8 and 255.1 MHz, with standard IRIG channels up to F, and transmitters with a power of 2 Watts feeding a quarter-wave ground plane antenna together with a quad-helical receiving antenna system with a gain of 21 dB. The uplink system is composed of a transmiter of 50 w operating on 148.46 MHz coupled to two vertical and horizontal plane multi-element yagis antennas, allowing a reliable control of the payload in flight.
Two downrange stations were used, one located in Newman (West) and the other in Longreach (East) each one with a coverage of 700 kms in all directions. Good telephone links were available between the two stations and Alice Spring with the possibility of data transfer at up to 9.6 kbs.
Althought the tracking of the balloons was performed visually using locally hired aircrafts, almost real time positional information was also available by the use of on-board Omega receivers or Argos transmitters. Termination was also performed from aircrafts with the balloon in sight.
Due to the desertic and rough terrain, in addition to the 4-wheel drive vehicles owned by the station, recovery operations often requires the use of helicopters which are also hired.
A new era of cooperation
Scientific ballooning in Australia would suffer two major changes during the 80's decade. The first one was a direct consequence of severe funding troubles started at the end of the 70's decade: the closure of the Mildura ABLS in December 1980. The station equipment was then moved to Alice Springs and the responsability for running the facility was transferred to the Physics Department at the University of Melbourne under direction of Prof. Ravi K. Sood.
The second change would occur in late 1981, with the entrance in the scene of NASA. Between November and December that year the National Scientific Balloon Facility (now Columbia Scientific Balloon Facility) in charge of the managment of the NASA balloon program, succesfully launched the first six balloons from Alice Spring under a campaign fully managed and supported by NSBF.
This marked the start of some sort of dual mode balloon campaigns, some of them managed by the Australians launching their own payloads as well third part experiments offered by international collaborations and the others carried out by the Americans, launching mainly US scientific payloads and in some occasions Australian payloads as well.
Since the change of management in 1980 all flight operations at the station under Australian managment have been carried out by amateurs, mainly academics, researchers, technicians and students of the University.
Past, present and future
Great part of the activity at the site took place in the 80's decade being launched dozens of missions in the field of Infrared, X-Ray and Gamma Ray astronomy as well were performed several others to measure high energy particles of galactic and cosmic origin. This activity was focused mainly in campaigns performed in the summer that lasted several months. Notably, a few missions on that decade were performed using a concept known as radiation controlled balloon or RACOON. This development allowed to flight large, low-cost polyethylene balloons for several weeks without the need of use great amounts of ballast. Those balloons made at the time crossings of the Pacific Ocean to Southamerica where the payload was recovered and even a few succeded in performing circumglobal flights with diverse results.
By the end of the decade a flood of scientists were looking to perform balloon missions in Australia to perform observations in all the high energy domain. The reason was that after the discovery in 1987 of the SN1987A supernova in the Large Magellanic Cloud, soon was realized that Alice Spring offered a first class seat to analyze the event, only visible in the southern hemisphere. Thus several missions were performed with this objective in the remainder of the 80's decade and the first years of the next, when the amount of launches started again to decrease.
In the first years of the XXI century, Alice Spring was choosen as the site to perform the first global flights of the NASA Ultra Long Duration Balloon (ULDB), a superpressure craft devoted to perform circumglobal flights of up to 100 days carrying a payload weighting a ton. Nevertheless, none global flight was achieved due to several design flaws of the model used at that time.
Since those launches in 2003 an "impasse" took place in the activity of the station. On one hand the intergovernmental agreement between Australia and the US for the accomplishment of these activities ended. In the other, the NASA's balloon program decided to cancel the missions from Australia initially until 2007, to balance its accounts after extraordinary expenses that demanded the works of improvement of the Antarctic balloon facilities at the McMurdo base.
After the renewal of the agreement, NASA's balloon program started in 2008 an important upgrading to the launching facilities in the Seven Miles Area of the airport by constructing an additional Integration and Staging Building adjacent to the existing one as can be seen in the image at right (click to enlarge). The new construction is a 60-foot by 60-foot building with enough space to allocate four integration bays for big payloads. The older building will be used for the Electronics Shop and Ground Telemetry Station as well as integration building for up to two small payloads. Much of the existing structures were also improved.
The main construction ended in October 2009, and currently the only lasting tasks are the internal outfitting of the buildings, expected to be completed before the start of the first campaign planned for the southern hemisphere fall in 2010, when five big balloons would be launched.
Balloon launched list
| Date | Hour | Flight Duration | Experiment | Payload landing place |
|---|---|---|---|---|
| 10/15/1970 | 10 h | High Energy X-ray Balloon Observatory | --- No Data --- | |
| 4/4/1972 | 26h 55m | --- NO DATA --- | --- NO DATA --- | |
| 4/5/1972 | 27 h | CONTROLLABLE X-RAY TELESCOPE | --- No Data --- | |
| 4/15/1972 | --- | -- No Data -- | --- No Data --- | |
| 4/19/1972 | --- | CONTROLLABLE X-RAY TELESCOPE | --- No Data --- | |
| 10/26/1977 | F 8 h 15 m | X-RAY OBSERVATIONS | --- No Data --- | |
| 11/11/1977 | F 55 h 45 m | GAMMA RAY EXPERIMENT | --- No Data --- | |
| 11/21/1977 | F 9 h 30 m | X-RAY OBSERVATIONS | --- No Data --- | |
| 11/22/1977 | F 47 h 45 m | GAMMA RAY EXPERIMENT | --- No Data --- | |
| 11/22/1978 | ~ 55 hr | X-RAY EXPERIMENT | --- No Data --- | |
| 4/4/1979 | 2 h | GAMMA RAY EXPERIMENT | --- No Data --- | |
| 4/15/1979 | F 16 h 10 m | GERMANIUM GAMMA RAY TELESCOPE | --- No Data --- | |
| 4/18/1979 | F 13 h 10 m | DOUBLE SCATTER GAMMA RAY TELESCOPE | --- No Data --- | |
| 11/12/1980 | 30 h | AGLAE | In an aborigin reserve 600 km from Alice Spring | |
| 11/10/1981 | 24 h 30 m | GAMMA RAY EXPERIMENT | --- No Data --- | |
| 11/20/1981 | 19 h | GAMMA RAY EXPERIMENT | --- No Data --- | |
| 11/21/1981 | 30 h 5 m | GAMMA RAY EXPERIMENT | --- No Data --- | |
| 12/1/1981 | 14 h 15 m | COSMIC RAY EXPERIMENT | --- No Data --- | |
| 12/2/1981 | F 12 h | COSMIC RAY EXPERIMENT | --- No Data --- | |
| 12/3/1981 | F 10 h 10 m | X-RAY EXPERIMENT | --- No Data --- | |
| 12/14/1982 | --- | ---No Data--- | Ground Abort | |
| 1/19/1983 | 20:41 | 22 d | EOSCOR III (Extended Observation of Solar COsmic Radiation) | Lost over the Indian Ocean |
| 5/4/1983 | 34 h | COSMIC RAY HEAVIES | --- No Data --- | |
| 5/8/1983 | 11 h | INFRARED ASTRONOMY | --- No Data --- | |
| 5/10/1983 | 29 h | COSMIC RAY HEAVIES | --- No Data --- | |
| 5/13/1983 | 25 h | ATMOSPHERIC ELECTRICITY | --- No Data --- | |
| 5/18/1983 | 13 h | INFRARED ASTRONOMY | --- No Data --- | |
| 11/7/1983 | 34 h | COSMIC RAY IRON NUCLEI | --- No Data --- | |
| 2/21/1985 | 12 h | INFRARED ASTRONOMY | --- No Data --- | |
| 2/27/1985 | 2 h | INFRARED ASTRONOMY | --- No Data --- | |
| 3/8/1985 | 8 h | INFRARED ASTRONOMY | --- No Data --- | |
| 8/27/1986 | 11 h | INFRARED ASTRONOMY | --- No Data --- | |
| 9/4/1986 | 2 h | INFRARED ASTRONOMY | --- No Data --- | |
| 9/13/1986 | 6 h | INFRARED ASTRONOMY | --- No Data --- | |
| 11/20/1986 | 12 h | PULSAR EMISSION SPECTRA OBSERVATION. | --- No Data --- | |
| 2/9/1987 | ~ 21:00 | 12 d | Observation of the sun corona. | Over Brazil. |
| 4/13/1987 | 2 h | X-RAY / GAMMA RAY ASTRONOMY | --- No Data --- | |
| 4/19/1987 | 9 h | X-RAY / GAMMA RAY ASTRONOMY | --- No Data --- | |
| 11/10/1987 | 15 m | X-RAY ASTRONOMY | --- No Data --- | |
| 11/19/1987 | 20 h | X-RAY ASTRONOMY | --- No Data --- | |
| 5/1/1988 | 24 h | GRIS (Gamma-Ray Imaging Spectrometer) | --- No Data --- | |
| 5/18/1988 | --- | EXITE (Energetic X-ray Imaging Telescope Experiment) | --- No Data --- | |
| 10/28/1988 | 44 h | GRIS (Gamma-Ray Imaging Spectrometer) | --- No Data --- | |
| 5/8/1989 | 30 h | EXITE (Energetic X-ray Imaging Telescope Experiment) | --- No Data --- | |
| 4/26/1992 | 14 h | GRIS (Gamma-Ray Imaging Spectrometer) | --- No Data --- | |
| 5/7/1992 | 24 h | GRIS (Gamma-Ray Imaging Spectrometer) | --- No Data --- | |
| 9/27/1995 | 7:44 local | 24 h | AXEL (Astrophysical X-Ray Experimental Laboratory) formed by a ultra high pressure proportional counter wich extract the position of the incoming X-ray and a phoswich detector | The flight was terminated just over the Western Australian border. The payload was parachuted to the ground, and impacted about 100 km north-west of the Giles weather station. |
| 10/4/1995 | 24 h | GRIS (Gamma-Ray Imaging Spectrometer) | --- No Data --- | |
| 10/7/1995 | 34 h | GRIP-2 (Gamma-Ray Imaging Payload) | --- No Data --- | |
| 10/17/1995 | 8:00 local | 32 h | GRATIS (Gamma Ray Arcminute Telescope Imaging System) | --- No Data --- |
| 10/24/1995 | 35 h | GRIS (Gamma-Ray Imaging Spectrometer) | --- No Data --- | |
| 11/14/1995 | 9 h 30 m | GRIS (Gamma-Ray Imaging Spectrometer) | --- No Data --- | |
| 2/25/2001 | 9:21 local | 4 h 17 m | NIGHTGLOW + ULDB (Ultra Long Duration Balloon) | 132 miles (212 kilometers) west-southwest of the launch site. |
| 3/10/2001 | 9:26 local | 24 h 42 m | ULDB (Ultra Long Duration Balloon) | Near the W coast line of Australia |
| 3/17/2003 | 8:38 local | 12 h 13 m | NIGHTGLOW + ULDB (Ultra Long Duration Balloon) | 241 kilometers west-southwest of Ayers Rock near the town of Uluru. |