A gestational profile of placental exosomes in maternal plasma and their effects on endothelial cell migration
C Salomon, MJ Torres, M Kobayashi… - PloS one, 2014 - journals.plos.org
Studies completed to date provide persuasive evidence that placental cell-derived
exosomes play a significant role in intercellular communication pathways that potentially …
exosomes play a significant role in intercellular communication pathways that potentially …
Ion acceleration and outflow from Mars and Venus: An overview
R Lundin - The plasma environment of Venus, Mars, and Titan, 2012 - Springer
Solar wind forcing of Mars and Venus results in outflow and escape of ionospheric ions.
Observations show that the replenishment of ionospheric ions starts in the dayside at low …
Observations show that the replenishment of ionospheric ions starts in the dayside at low …
Observations and modeling of Martian auroras
SA Haider, KK Mahajan, SW Bougher… - Space Science …, 2022 - Springer
Observations of planetary auroras form a new area of planetary exploration from space,
especially for nonmagnetic planets since various kinds of auroras like Discrete, Proton and …
especially for nonmagnetic planets since various kinds of auroras like Discrete, Proton and …
The analyser of space plasmas and energetic atoms (ASPERA-4) for the Venus Express mission
The general scientific objective of the ASPERA-4 (Analyser of Space Plasmas and Energetic
Atoms) experiment is to study the solar wind–atmosphere interaction and characterise the …
Atoms) experiment is to study the solar wind–atmosphere interaction and characterise the …
Energetic neutral atoms as the explanation for the high-velocity hydrogen around HD 209458b
Absorption in the stellar Lyman-α (Lyα) line observed during the transit of the extrasolar
planet HD 209458b in front of its host star reveals high-velocity atomic hydrogen at great …
planet HD 209458b in front of its host star reveals high-velocity atomic hydrogen at great …
Two regimes of interaction of a hot Jupiter's escaping atmosphere with the stellar wind and generation of energized atomic hydrogen corona
IF Shaikhislamov, ML Khodachenko… - The Astrophysical …, 2016 - iopscience.iop.org
The interaction of escaping the upper atmosphere of a hydrogen-rich non-magnetized
analog of HD 209458b with a stellar wind (SW) of its host G-type star at different orbital …
analog of HD 209458b with a stellar wind (SW) of its host G-type star at different orbital …
Energetic neutral atoms around HD 209458b: estimations of magnetospheric properties
ABSTRACT HD 209458b is an exoplanet found to transit the disk of its parent star.
Observations have shown a broad absorption signature about the Lyα stellar line during …
Observations have shown a broad absorption signature about the Lyα stellar line during …
XUV-exposed, non-hydrostatic hydrogen-rich upper atmospheres of terrestrial planets. Part II: hydrogen coronae and ion escape
KG Kislyakova, H Lammer, M Holmström… - Astrobiology, 2013 - liebertpub.com
We studied the interactions between the stellar wind plasma flow of a typical M star, such as
GJ 436, and the hydrogen-rich upper atmosphere of an Earth-like planet and a “super-Earth” …
GJ 436, and the hydrogen-rich upper atmosphere of an Earth-like planet and a “super-Earth” …
First ENA observations at Mars: ENA emissions from the Martian upper atmosphere
The neutral particle detector (NPD) on board Mars Express has observed energetic neutral
atoms (ENAs) from a broad region on the dayside of the martian upper atmosphere. We …
atoms (ENAs) from a broad region on the dayside of the martian upper atmosphere. We …
Inversion of upstream solar wind parameters from ENA observations at Mars
An algorithm has been developed to invert the solar wind parameters from the hydrogen
energetic neutral atom (H-ENA) measured in near-Mars space. Supposing the H-ENA is …
energetic neutral atom (H-ENA) measured in near-Mars space. Supposing the H-ENA is …