Add to ORKGProcess of energy dissipation through radiation and evaporation, deceleration by drag, and ablation through evaporation of spherical stony micrometeorites in earth atmospher
We evaluate the heating of extraterrestrial particles entering the atmosphere using the comprehensiv...
Low energy solar wind (SW) and solar energetic particles (SEP) interact with material exposed on the...
Micrometeorites (MMs) provide constraints on the flux and sources of extraterrestrial dust falling o...
Aims. Micrometeoroids (cosmic dust with size between a few μm and ~1 mm) dominate the an...
Aims: Micrometeoroids (cosmic dust with size between a few μm and ~1 mm) dominate the annual extrate...
Ablation properties and luminosity of artificial meteoroid materials determined in plasma jet test
Physics of atmospheric entry of meteoroids was an active area of research at NASA ARC up to the earl...
Micrometeorite trajectory, composition, mass distribution, particle flux, and structure of cosmic du...
Evaluation of meteor flight parameters taking into account surface radiation and vapor ablatio
The vast majority of meteoroids either fall to the ground as meteorites or ablate completely in the ...
The problem of formation of the aerosol of space origin in Earth s atmosphere is examined. Meteoroid...
INTRODUCTION Micrometeoroids (MMs) represent the largest mass flux of extraterrestrial matter to ...
Each year 40,000 tons of extra-terrestrial material reaches the Earth's surface as micrometeorites. ...
The materials with vulnerability to micrometeoroids and space debris are discussed. It is concluded ...
Interplanetary particle study involving zodiacal clouds, meteoritic complex, and radio meteor
We evaluate the heating of extraterrestrial particles entering the atmosphere using the comprehensiv...
Low energy solar wind (SW) and solar energetic particles (SEP) interact with material exposed on the...
Micrometeorites (MMs) provide constraints on the flux and sources of extraterrestrial dust falling o...
Aims. Micrometeoroids (cosmic dust with size between a few μm and ~1 mm) dominate the an...
Aims: Micrometeoroids (cosmic dust with size between a few μm and ~1 mm) dominate the annual extrate...
Ablation properties and luminosity of artificial meteoroid materials determined in plasma jet test
Physics of atmospheric entry of meteoroids was an active area of research at NASA ARC up to the earl...
Micrometeorite trajectory, composition, mass distribution, particle flux, and structure of cosmic du...
Evaluation of meteor flight parameters taking into account surface radiation and vapor ablatio
The vast majority of meteoroids either fall to the ground as meteorites or ablate completely in the ...
The problem of formation of the aerosol of space origin in Earth s atmosphere is examined. Meteoroid...
INTRODUCTION Micrometeoroids (MMs) represent the largest mass flux of extraterrestrial matter to ...
Each year 40,000 tons of extra-terrestrial material reaches the Earth's surface as micrometeorites. ...
The materials with vulnerability to micrometeoroids and space debris are discussed. It is concluded ...
Interplanetary particle study involving zodiacal clouds, meteoritic complex, and radio meteor
We evaluate the heating of extraterrestrial particles entering the atmosphere using the comprehensiv...
Low energy solar wind (SW) and solar energetic particles (SEP) interact with material exposed on the...
Micrometeorites (MMs) provide constraints on the flux and sources of extraterrestrial dust falling o...