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Photochemical Haze Formation on Titan and Uranus: A Comparative Review. [PDF]
Dubois D.
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Autonomous, miniature research station (lab-payload) for the nanosatellite biological mission: LabSat. [PDF]
Śniadek P +5 more
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MiRNAs shape mouse age-independent tissue adaptation to spaceflight via ECM and developmental pathways. [PDF]
Grandke F +16 more
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Secure and scalable dual blockchain and IPFS driven IoT ecosystem for next gen healthcare systems. [PDF]
Mallick SR, Lenka RK, Sobhanayak S.
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Enhancing the Thermoelectric Properties and Delaying Their Attenuation in n‑Type SiGe Alloy through SiC Nanoparticle Doping. [PDF]
Zhao T, Li X, Wu W, Gu J, Han Y, Tang X.
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Smart Contracts and Shared Platforms in Sustainable Health Care: Systematic Review.
Marino CA, Diaz Paz C.
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The Interplanetary Medium Family
Astronomers' Universe, 2019Like the interstellar medium, the interplanetary medium is composed of gas and dust (P 15), as well as energetic particles from the solar wind (P 16) and cosmic rays (S 30). The solar wind creates the heliosphere, a bubble within the more general interstellar wind, and while most of the material in the heliosphere emanates from the Sun itself, a small ...
S. Dick
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Interplanetary medium – A dusty plasma
Advances in Space Research, 2008The average mass of dust per volume in space equals that of the solar wind so that the interplanetary medium should provide an obvious region to study dust plasma interactions. While dust collective behavior is typically not observed in the interplanetary medium, the dust component rather consists of isolated grains screened by and interacting with the
Ingrid Mann
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Energetic Solar Electrons in the Interplanetary Medium
Solar Physics, 1985ISEE-3 measurements extending down to 2 keV energy have provided a new perspective on energetic solar electrons in the interplanetary medium. Impulsive solar electron events are observed, on average, several times a day near solar maximum, with ~40% detected only below ~ 15 keV.
R. Lin
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