Coronal mass ejections and their sheath regions in interplanetary space
E Kilpua, HEJ Koskinen, TI Pulkkinen - Living Reviews in Solar Physics, 2017 - Springer
Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …
The evolution of the solar wind
AA Vidotto - Living reviews in solar physics, 2021 - Springer
How has the solar wind evolved to reach what it is today? In this review, I discuss the long-
term evolution of the solar wind, including the evolution of observed properties that are …
term evolution of the solar wind, including the evolution of observed properties that are …
Habitability and biosignatures of Hycean worlds
N Madhusudhan, AAA Piette… - The Astrophysical …, 2021 - iopscience.iop.org
We investigate a new class of habitable planets composed of water-rich interiors with
massive oceans underlying H 2-rich atmospheres, referred to here as Hycean worlds. With …
massive oceans underlying H 2-rich atmospheres, referred to here as Hycean worlds. With …
Magnetic fields of M dwarfs
O Kochukhov - The Astronomy and Astrophysics Review, 2021 - Springer
Magnetic fields play a fundamental role for interior and atmospheric properties of M dwarfs
and greatly influence terrestrial planets orbiting in the habitable zones of these low-mass …
and greatly influence terrestrial planets orbiting in the habitable zones of these low-mass …
The population of M dwarfs observed at low radio frequencies
Coherent low-frequency (≲ 200 MHz) radio emission from stars encodes the conditions of
the outer corona, mass-ejection events and space weather,,,–. Previous low-frequency …
the outer corona, mass-ejection events and space weather,,,–. Previous low-frequency …
New observational constraints on the winds of M dwarf stars
BE Wood, HR Müller, S Redfield, F Konow… - The Astrophysical …, 2021 - iopscience.iop.org
High-resolution UV spectra of stellar H i Lyα lines from the Hubble Space Telescope (HST)
provide observational constraints on the winds of coronal main-sequence stars, thanks to an …
provide observational constraints on the winds of coronal main-sequence stars, thanks to an …
Modeling repeated M dwarf flaring at an Earth-like planet in the habitable zone: atmospheric effects for an unmagnetized planet
Understanding the impact of active M dwarf stars on the atmospheric equilibrium and
surface conditions of a habitable zone Earth-like planet is key to assessing M dwarf planet …
surface conditions of a habitable zone Earth-like planet is key to assessing M dwarf planet …
Evolved climates and observational discriminants for the TRAPPIST-1 planetary system
The TRAPPIST-1 planetary system provides an unprecedented opportunity to study
terrestrial exoplanet evolution with the James Webb Space Telescope (JWST) and ground …
terrestrial exoplanet evolution with the James Webb Space Telescope (JWST) and ground …
Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1
Ultracool dwarfs (UCD; T eff<∼ 3000 K) cool to settle on the main sequence after∼ 1 Gyr.
For brown dwarfs, this cooling never stops. Their habitable zones (HZ) thus sweeps inward …
For brown dwarfs, this cooling never stops. Their habitable zones (HZ) thus sweeps inward …
The habitability of proxima centauri bI. irradiation, rotation and volatile inventory from formation to the present
Proxima b is a planet with a minimum mass of 1.3M⊕ orbiting within the habitable zone (HZ)
of Proxima Centauri, a very low-mass, active star and the Sun's closest neighbor. Here we …
of Proxima Centauri, a very low-mass, active star and the Sun's closest neighbor. Here we …