Observations of High Energy Primary Electrons and Their Astrophysical Significance
Vela as the most likely source for the primary electrons in TeV region
Plastic Balloons with Thin Polyethylene Films for High Altitude Observations
A Micro Segment Chamber for the cosmic-ray balloon experiment
CHAPTER 2 -- BALLOON DESIGN - Overpressurized Balloon
CHAPTER 2 -- BALLOON DESIGN - Feasibility Study of EVAL Balloons
New measurement of the electron flux from 10 GeV to 100 GeV with the bets instrument
Cosmic-ray electron flux from 10 to 100 GeV measured by the bets instrument