Antarctica bess types

The Bess-Polar II Long Duration Flight Above Antarctica

BESS-Polar is an advanced program of the BESS collaboration to study these topics with much greater precision using long duration flights above Antarctica. The BESS-Polar spectrometer was successfully developed to accumulate much larger numbers of events during long duration flights around the South Pole.

BESS-Polar experiment: Progress and future prospects

The first scientific flight of the BESS-Polar balloon-borne experiment was successfully carried out in December 2004 from Antarctica with the primary scientific

Antarctica New Zealand 10-MWh BESS

Endless Energy, in partnership with ComAp and EIS, secured the contract to design and install a cutting edge 10 MWh Battery Energy Storage System (BESS) for the Scott Base redevelopment. The BESS will connect to three new 1MW wind turbines and a new microgrid system between Scott Base, the Crater Hill Wind Farm, and the American run

BESS

BESS-Polar has the largest geometry factor of any balloon-borne magnet spectrometer currently flying, and is ideally suited to statistics-limited studies of Z=1 and Z=2 components - identifying antiprotons, and searching for antihelium nuclei in the cosmic radiation.

Measurements of cosmic-ray proton and helium spectra from the BESS

We report new measurements of the energy spectra of cosmic-ray protons and helium made by the BESS-Polar Collaboration (Balloon-borne Experiment with a Superconducting Spectrometer-Polar) during long-duration balloon (LDB) flights over Antarctica in December 2004 (BESS-Polar I), prior to the last solar minimum, and in December 2007 (BESS-Polar

The results from BESS-Polar experiment

The first and second scientific flights called BESS-Polar I/II were successfully performed, over Antarctica in 2004 December and 2007 December respectively. We report the

Antarctica New Zealand 10-MWh BESS

Endless Energy, in partnership with ComAp and EIS, secured the contract to design and install a cutting edge 10 MWh Battery Energy Storage System (BESS) for the Scott

Measurement of the Cosmic-Ray Antiproton Spectrum at

BESS-Polar II data show no evidence of primary ¯p''s from evaporation of primordial black holes. Precise measurement of the cosmic-ray antiproton (¯p) spectrum is crucial to investigations of conditions in the early universe and cosmic-ray propagation. Most cosmic-ray ¯p''s are produced by interactions of cosmic-ray nuclei

The Bess-Polar II Long Duration Flight Above Antarctica

BESS-Polar is an advanced program of the BESS collaboration to study these topics with much greater precision using long duration flights above Antarctica. The BESS-Polar spectrometer

BESS: Present Results and the BESS-Polar Program

In nine flights between 1993 and 2002, the Balloon Borne Experiment with a Superconducting Spectrometer (BESS) has measured the spectrum of cosmic-ray antiprotons between 0.18 and 4.20 GeV, and the spectra of protons and

BESS-polar experiment

The BESS-polar detector is designed to meet the requirements of long duration balloon flights over Antarctica. The total weight of the payload will be about 1500 kg. A

Measurement of the Cosmic-Ray Antiproton Spectrum at

BESS-Polar II data show no evidence of primary ¯p''s from evaporation of primordial black holes. Precise measurement of the cosmic-ray antiproton (¯p) spectrum is crucial to investigations of

BESS-polar experiment

The BESS-polar detector is designed to meet the requirements of long duration balloon flights over Antarctica. The total weight of the payload will be about 1500 kg. A dedicated solar battery system providing 600 W electric power is also being developed for the front-end electronics and the data acquisition system.

(PDF) BESS-Polar II experiment

The BESS program has been extended to long duration balloon (LDB) flights in Antarctica (BESS-Polar) with the goal of achieving unprecedented sensitivity in the search for

The results from BESS-Polar experiment

The first and second scientific flights called BESS-Polar I/II were successfully performed, over Antarctica in 2004 December and 2007 December respectively. We report the scientific results, focusing on the long-duration flights of

(PDF) BESS-Polar II experiment

The BESS program has been extended to long duration balloon (LDB) flights in Antarctica (BESS-Polar) with the goal of achieving unprecedented sensitivity in the search for primordial

BESS-Polar experiment: Progress and future prospects

The first scientific flight of the BESS-Polar balloon-borne experiment was successfully carried out in December 2004 from Antarctica with the primary scientific objectives of searching for primordial antiparticles from the universe and making precision measurements of primary cosmic-ray fluxes.

Measurements of cosmic-ray proton and helium spectra from the

We report new measurements of the energy spectra of cosmic-ray protons and helium made by the BESS-Polar Collaboration (Balloon-borne Experiment with a

BESS: Present Results and the BESS-Polar Program

In nine flights between 1993 and 2002, the Balloon Borne Experiment with a Superconducting Spectrometer (BESS) has measured the spectrum of cosmic-ray antiprotons

Antarctica bess types [PDF]

Solar Pro.