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Space and Earth Observations from Stratospheric Balloons

Author(s)
Ibba, Roberto  
Peterzen, Steven
Ubertini, Pietro
Masi, Silvia
Date Issued
2008-01-01
Abstract
Stratospheric balloons are rapidly becoming the vehicle of choice for near space investigations and earth observations by a variety of science disciplines. With the ever increasing research into climatic change, instruments suspended from stratospheric balloons offer the science team a unique, stable and reusable platform that can circle the Earth in the polar region or equatorial zone for thirty days or more. The Italian Space Agency (ASI) in collaboration with Andoya Rocket Range (Andenes, Norway) has opened access in the far northern latitudes above 78o N from Longyearbyen, Svalbard. In 2006 the first Italian UltraLite Long Duration Balloon was launched from Baia Terra Nova, Mario Zuchelli station in Antarctica and now ASI is setting up for the their first equatorial stratospheric launch from their satellite receiving station and rocket launch site in Malindi, Kenya. For the equatorial missions we have analysed the statistical properties of trajectories considering the biennal oscillation and the seasonal effects of the stratospheric winds. Maintaining these launch sites offer the science community 3 point world coverage for heavy lift balloons as well as the rapidly deployed Ultralight payloads and TM system ASI developed to use for test platforms, micro experiments, as well as a comprehensive student pilot program
URI
https://hdl.handle.net/20.500.13025/2643
Journal
37th COSPAR Scientific Assembly. Held 13-20 July 2008, in Montreal, Canada.
URL
http://adsabs.harvard.edu/abs/2008cosp...37.2419P
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