The results are a more efficient engine that could be used for interplanetary manned missions.
Based on this we suggest that the cyanophage-infected cyanobacteria may be more likely to survive the interplanetary transport than the cyanobacteria alone.
The divergence-free condition is trivially satisfied in numerical simulations for either parallel or antiparallel interplanetary magnetic and magnetospheric fields.
Volumes of air from the upper stratosphere collected via balloon-carried cryogenic equipment have been found to trap interplanetary microparticles (1).
This corresponds to the situation encountered with interplanetary magnetic clouds in the solar wind.
In the latter case, one can expect the proposed expansion to depend crucially on the interplanetary magnetic field conditions.
The fluffy nature of cometary material facilitates the degradation of these particles in the interplanetary medium.
The interplanetary shock is an important phenomenon, often observed by spacecrafts in interplanetary space.
