BARREL 2013 Operations have officially ended.
For more information on the 2013 campaign, science updates, and preparations for our 2014 campaign, check out the BARREL blog!
BARREL Fact Sheet
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BARREL has a webpage on the NASA website.
Click here to visit the BARREL page on the NASA website
David Smith (one of the BARREL Co-I's) was featured on KQED in California, talking
Click here to listen
to the audio and read the article.
BARREL I&T in progress
Balloon Array for Radiation Belt Relativistic Electron Losses
BARREL (Balloon Array for RBSP Relativistic Electron Losses) is a
multiple-balloon investigation that will study Earth's Radiation Belts. Atmospheric losses of relativistic electrons
play an important role in radiation belt dynamics; precipitation into the atmosphere may even completely deplete the
radiation belts in some cases. BARREL is the first NASA Living with a Star Geospace Mission of Opportunity, and
will support NASA's RBSP (Radiation Belt Storm Probes) mission.
BARREL will consist of two Antarctic balloon campaigns conducted in Austral summers of 2012 and 2013. During each
campaign, a total of 20 small (~20 kg) balloon payloads will be launched to an altitude of 30-35 km to maintain an array
of 5-8 payloads. Each balloon will carry a NaI scintillator to measure the bremsstrahlung X-rays produced by
precipitating relativistic electrons as they collide with neutrals in Earth's atmosphere, and a DC magnetometer. The
balloons will be launched from the South African
Antarctic Station (SANAE IV) and the British station, Halley Bay.
We will combine the measurements of precipitation with the RBSP spacecraft measurements of waves and energetic particles,
achieving the following specific science objectives during the RBSP mission:
Determine the total electron loss rate during RBSP relativistic electron events by simultaneously measuring the
precipitating flux of relativistic electrons over a wide range of local times. The loss rate will be compared with
changes in the trapped flux for specific relativistic electron events to help quantify relativistic electron
acceleration, and determine whether pitch-angle scattering is occurring in the strong-diffusion limit.
Directly test models of wave-particle interactions in order to differentiate among different loss processes by combining
precipitation measurements with simultaneous RBSP in situ wave and energetic particle measurements. We will
quantitatively test whether EMIC waves and chorus are responsible for duskside MeV events and microburst precipitation
respectively. This will be crucial for validating the models that will be used to calculate losses based only on in-situ
RBSP measurements, for example during times when global precipitation measurements are not available.
Determine the relative importance of duskside MeV events and microburst precipitation and their associated precipitation
mechanisms for different magnetic activity levels. This will be achieved by comparing the precipitation loss rates due to
both types of precipitation. BARREL will detect 120 duskside MeV events, allowing us to produce the first magnetic local
time/L-value distribution of these events, which can then be compared to the distribution for microbursts measured by
Characterize the spatial extent and spatial structure of precipitation, which has been addressed previously only in a
statistical sense. The region over which waves scatter electrons is a critical parameter for modeling electron loss
timescales. This is particularly important when direct precipitation measurements are not available. BARREL will
simultaneously measure precipitation at 5-8 different locations in correlation with wave measurements made by RBSP.
BARREL is one balloon project carried out by the Dartmouth Balloon Group. Click here to
learn about other projects carried out by the group.