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AESOP / LEE [Anti-Electron Sub Orbital Payload / Low Energy Electrons]
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ANITA [Antarctic Impulse Transient Array] (project for radio frequency neutrino shower detection) See also here.
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ATIC [Advanced Thin Ionization Calorimeter]
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BaBy [Background Bypass] (measuring atmospheric UV background for the EUSO project)
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BESS [Balloon-borne Experiment with a superconducting Solenoid Spectrometer] (see also here).
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BETS [Balloon borne Electron Telescope with Scintillating fibers]
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CAPRICE [Cosmic AntiParticle Ring Imaging Cherenkov Experiment] (see also CAPRICE-II)
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CREAM [Cosmic Ray Energetics and Mass Balloon Experiment] (see also here and here)
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GRATIS [Gamma-Ray Arcminute Telescope Imaging System]
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GRIP [Gamma Ray Imaging Payload]
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GRIS [Gamma-Ray Imaging Spectrometer]
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HEAT [High Energy Antimatter Telescope]
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HIREGS [High Resolution Gamma-Ray and Hard X-Ray Spectrometer]
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IMAX [Isotope Matter Antimatter Experiment] (see also here and here)
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ISOMAX [Isotope Magnet Experiment]
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JACEE [Japanese-American Collaborative Emulsion Experiment]
(mainly for cosmic-ray composition up to several hundred TeV)
隨著能量的增大宇宙射線質(zhì)量的測量越來越困難?!叭彰篮献魅槟z實(shí)驗(yàn)”(JACEE)的聯(lián)合高空氣球?qū)嶒?yàn)結(jié)果,提供了能量高達(dá)1015eV的有價值的重要資料。這項實(shí)驗(yàn)是在高空氣球浮升到含量不到0.5%的大氣頂層進(jìn)行的。得到的結(jié)論是,雖然大氣效應(yīng)仍待改正,這里能不受影響地在大氣中觀測到宇宙射線。JACEE實(shí)驗(yàn)是由日本、美國和波蘭研究人員協(xié)作進(jìn)行的,一系列的長期氣球飛行已經(jīng)積累了大量數(shù)據(jù)?;緦?shí)驗(yàn)由探測宇宙射線、測定其電荷和能量等幾項工作組成。由于能夠進(jìn)行研究的能量范圍寬,所以這些測量特別重要。因?yàn)樘綔y系統(tǒng)非常龐大,探測器能在多次飛行中反復(fù)利用,所以觀測的時間也很長。實(shí)驗(yàn)采用大面積和長時間就意味著,宇宙射線粒子雖然稀少,卻可以探測到相當(dāng)數(shù)量的高能宇宙射線。
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MASS.. [Matter Antimatter Superconducting Spectrometer] (flown in different configurations; for MASS2 see also here)
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RUNJOB [RUssian-Nippon JOint Balloon Experiment]
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SMILI [Superconducting Magnet Instrument for Light Isotopes]
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TIGRE [Tracking and Imaging Gamma Ray Experiment] (under development)
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TIGER [Trans Iron Galactic Element Recorder]
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TRACER [Transition Radiation Array for Cosmic Energetic Radiation]
See also the NASA links to balloon instruments.