Ohmic Heating Archives

Qmax (Eq. 14) for the population of exoplanets from the exoplanet.eu database, as a function of the orbital distance and the stellar mass. A given rotation rate has been assumed for all stars in each panel, to estimate their magnetic field and the ambient magnetic field strength at the orbit of the planet. Trappist-1 b and π men c are highlighted by the red square in the left and right panels, respectively. -- astro-ph.EP

Atmospheres, Climate, Weather, Exoplanets, -moons, -comets, Magnetic Fields, Electromagnetism, bioelectricity,, Space Weather & Heliophysics, Status Report

Ohmic Heating In The Upper Atmosphere of Hot Exoplanets The Influence of a Time-varying Magnetic Field

by Keith CowingDecember 22, 2024December 22, 2024

Exoplanets on close-in orbit are subject to intense X-ray and ultraviolet (XUV) irradiation from their star. Their atmosphere therefore heats up, sometimes to the point where it thermally escapes from […]

Ohmic Heating

Ohmic Heating In The Upper Atmosphere of Hot Exoplanets The Influence of a Time-varying Magnetic Field

ALMA Central Molecular Zone Exploration Survey (ACES) I: Overview

RNA And Proteins Joined Up At The Origins Of Life: Persistence Is The Point

Selection For Growth Drives The Emergence Of Genetic Heredity In Protocells

NASA SMD ROSES-25 Amendment 65: New Opportunity: C.4 Planetary Science Enabling Facilities

TESS Photometry and Radial Velocity Analysis of the sub-Neptune Exoplanet π Mensae c and the Wider π Mensae Planetary System