Photographic observations of a low-density iron artificial meteoroid
Photographic observations of low density iron artificial meteoroid
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Photographic observations of low density iron artificial meteoroid
Meteoroid impact damage to Apollo and Gemini ablative heat shields
Scaling laws for predicting penetration of semiinfinite targets by particles traveling at meteoroid velocities - simulation techniques for low velocity and hypervelocity impacts
Electron irradiation from 20 keV to 1 MeV used to study effects on polyethylene terephthalate capacitor-type meteoroid detector
Material and geometry aspects of meteoroid armor protection for space radiator tubes, discussing bumper-fin concept
Model of near-earth meteoroid environment from satellite observation data
Satellite instrumentation and data retrieval procedures for collecting meteoroid penetration data from Pegasus satellite
Data collection and analysis of meteoroid penetration recorded on Pegasus flights, and derived flux figures
Statistical analysis of Pegasus satellite measurements of meteoroid penetration
Meteoroid hazards to solid propellant rocket motors
Mathematical model for determining ballistic limit of double-walled meteoroid bumper systems
Impact effects applied to meteoroid hazard
Meteoroid flux and puncture models for cislunar space
Meteoroid and hypervelocity impact criteria for spacecraft design study
Meteoroid penetration measurements by Explorer XVI and XXIII satellites and Pegasus satellites for application to spacecraft design
Meteoroid protection system designs for optimum orbital space laboratories and manned interplanetary spacecraft
Astronomical and satellite measurements of meteoroid environment of spacecraft in solar system
Comets lose mass primarily in the form of large particles that form meteoroid streams in the comets orbits. At visible wavelengths, comets often have long dust tails directed away from the Sun, consisting of small dust particles being blown away by solar radiation pressure.