The Cosmic-Ray Electron and Positron Spectra Measured at 1 AU during Solar Minimum Activity

By M. Boezio, P. Carlson, T. Francke, N. Weber, M. Suffert, M. Hof, W. Menn, M. Simon, S. A. Stephens, R. Bellotti and 25 more. 2000

211 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Pulmonary and Respiratory Medicine

View Paper: https://www.semanticscholar.org/paper/8a52bb08fb0f0b3a19fc406b3e84a4246cf18716

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In Astronomy and Astrophysics

1. E. Orlando
2. A. Strong
3. T. Jaffe
4. N. Fornengo
5. R. Lineros
6. J. Lavalle
7. T. Delahaye
8. F. Donato

In Nuclear and High Energy Physics

1. E. Orlando
2. A. Strong
3. N. Fornengo
4. T. Jaffe
5. R. Lineros
6. J. Lavalle
7. T. Delahaye
8. F. Donato

Citations in the corpus

• History of dark matter (2018, unknown): “Building upon earlier measurements (Mueller and Tang, 1987; Golden et al., 1996; Boezio et al., 2000), the balloon-bourne HEAT experiment observed in 1994, 1995, and 2000 indications of an excess of cosmic-ray positrons at energies above ∼10 GeV, relative to the rate predicted from standard…”
• The Most Likely Sources of High-Energy Cosmic-Ray Electrons in Supernova Remnants (2003, background): “As positrons are produced by this process, we can estimate the intensity of secondaries relative to primaries to be ∼ 10% at 10 GeV from the observed ratio of e+ to e− + e+ ∼ 5% at 10 GeV (Barwick et al. 1997; Boezio et al. 2000).”
• Observation of an anomalous positron abundance in the cosmic radiation (2008, result): “The low energy difference between the PAMELA results and those from CAPRICE94[32], HEAT95[31] and AMS-01[33] are interpreted as a consequence of solar modulation effects.”
• Galactic electrons and positrons at the Earth: new estimate of the primary and secondary fluxes (2010, methodology): “For electrons, we see that the data of CAPRICE and AMS-01 are barely consistent, but we can identify a median configuration.”
• Prospects for indirect detection of neutralino dark matter (2000, unknown): “HEAT94/95 [108] Balloon 1994/95 29/26 hr 495 50 — — CAPRICE94/98 [109] Balloon 1994/98 18/21 hr 163 10/30 — —”
• A database of charged cosmic rays (2013, unknown): “…BESS-TeV (2002/08): Haino et al. (2004, 2005); Shikaze et al. (2007) – BESS-PolarI (2004/12): BESS Collaboration et al. (2008) – BESS-PolarII (2007/12-2008/01): Abe et al. (2012b) – BETS – BETS97&98 (1997/06+1998/05): Torii et al. (2001) – BETS04 (2004/01): Yoshida et al. (2008) – CAPRICE –…”