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Because the solar luminosity increases over geological timescales, Earth climate is expected to warm, increasing water evaporation which, in turn, enhances the atmospheric greenhouse effect. Above a certain critical insolation, this…

Earth and Planetary Astrophysics · Physics 2015-06-18 Jérémy Leconte , François Forget , Benjamin Charnay , Robin Wordsworth , Alizée Pottier

We investigate atmospheric responses of modeled hypothetical Earth-like planets in the habitable zone of the M-dwarf AD Leonis to reduced oxygen (O2), removed biomass (dead Earth), varying carbon dioxide (CO2) and surface relative humidity…

Earth and Planetary Astrophysics · Physics 2021-03-17 Stefanie Gebauer , Iva Vilović , John Lee Grenfell , Fabian Wunderlich , Franz Schreier , Heike Rauer

The South and East Asian summer monsoons are globally significant meteorological features, creating a strongly seasonal pattern of precipitation. The stability of the monsoon is of extreme importance for a vast range of ecosystems and for…

Atmospheric and Oceanic Physics · Physics 2023-10-27 Lucy Recchia , Valerio Lucarini

We model the temperature and chemical structure of molecular clouds as a function of depth into the cloud, assuming a cloud of constant density n illuminated by an external FUV (6 eV < E < 13.6 eV) flux G_0 (scaling factor in multiples of…

Astrophysics · Physics 2011-02-11 David Hollenbach , Michael J. Kaufman , Edwin A. Bergin , Gary J. Melnick

The rotational transitions of carbon monoxide (CO) are the primary means of investigating the density and velocity structure of the molecular interstellar medium. Here we study the lowest four rotational transitions of CO towards…

Astrophysics · Physics 2009-10-31 James G. Ingalls , T. M. Bania , Adair P. Lane , Matthias Rumitz , Antony A. Stark

Carbon is an essential element for life on Earth, and the relative abundances of major carbon species (CO2, CO, and CH4) in the atmosphere exert fundamental controls on planetary climate and biogeochemistry. Here, we employed a theoretical…

Earth and Planetary Astrophysics · Physics 2024-11-06 Yasuto Watanabe , Kazumi Ozaki

On their way through the heliosphere, Galactic Cosmic Rays (GCRs) are modulated by various effects before they can be detected at Earth. This process can be described by the Parker equation, which calculates the phase space distribution of…

Space Physics · Physics 2017-11-28 Jan Gieseler , Bernd Heber , Konstantin Herbst

Motivated by the theoretical hypotheses on the existence of heretofore unobserved stable elementary particles and exotic nuclear states, we searched for doubly-charged particles, as anomalously heavy isotopes of helium, in the Earth's…

Nuclear Experiment · Physics 2009-11-10 P. Mueller , L. -B. Wang , R. J. Holt , Z. -T. Lu , T. P. O'Connor , J. P. Schiffer

The Great Oxidation Event was a period during which Earth's atmospheric oxygen (O$_2$) concentrations increased from $\sim 10^{-5}$ times its present atmospheric level (PAL) to near modern levels, marking the start of the Proterozoic…

Earth and Planetary Astrophysics · Physics 2022-09-28 Gregory Cooke , Dan Marsh , Catherine Walsh , Sarah Rugheimer , Geronimo Villanueva

We present an experimental study of the absorption, between 40 and 640 cm$^{-1}$, by CO$_2$, CH$_4$ and H$_2$ gases as well as by H$_2$+CO$_2$ and CH$_4$+CO$_2$ mixtures at room temperature. A Fourier transform spectrometer associated to a…

Earth and Planetary Astrophysics · Physics 2018-12-05 Martin Turbet , Ha Tran , Olivier Pirali , Francois Forget , Christian Boulet , Jean-Michel Hartmann

Global warming arises from 'temperature forcing', a net imbalance between energy fluxes entering and leaving the climate system and arising within it. Humanity introduces temperature forcing through greenhouse gas emissions, agriculture,…

Atmospheric and Oceanic Physics · Physics 2008-12-12 Nick E. B. Cowern , Chihak Ahn

We study the abundances of complex carbon-bearing molecules in the oxygen-rich dust- forming atmospheres of Brown Dwarfs and giant gas planets. The inner atmospheric re- gions that form the inner boundary for thermochemical gas-phase models…

Solar and Stellar Astrophysics · Physics 2015-06-16 Camille Bilger , Paul Rimmer , Christiane Helling

An old conceptual physics-based back-of-the-envelope model for greenhouse effect is revisited and validated against state-of-the-art reanalyses. Untraditional diagnostics show a physically consistent picture, for which the state of earth's…

Atmospheric and Oceanic Physics · Physics 2013-03-05 Rasmus E. Benestad

Forbush decreases (FDs) are depletions in the galactic cosmic ray (GCR) count rate that last typically for about a week and can be caused by coronal mass ejections (CMEs) or corotating interacting regions (CIRs). Fast CMEs that drive shocks…

Space Physics · Physics 2020-02-24 Anamarija Kirin , Bojan Vršnak , Mateja Dumbović , Bernd Heber

The effect of ionisation quenching for ions is critical for experiments relying on the measurement of low energy recoils, such as direct Dark Matter searches. We present ionisation quenching factor estimates over a range of energies for…

High Energy Physics - Experiment · Physics 2022-05-12 Ioannis Katsioulas , Patrick Knights , Konstantinos Nikolopoulos

Laser cooling and magneto-optical trapping of molecules typically involves multiple transitions driven by several laser frequencies. We analyze how magneto-optical trapping forces depend on the angular momenta, $F_l$ and $F_u$, and the…

Atomic Physics · Physics 2015-06-22 M. R. Tarbutt

One of the greatest challenges to theoretical models of massive galaxy formation is the regulation of star formation at early times. The relative roles of molecular gas expulsion, depletion, and stabilization are uncertain as direct…

Drylands forestation offers the potential for significant long-term sequestration of atmospheric CO$_2$. We consider sequestration of organic and inorganic carbon by a planted semi-arid forest, based on carbon that originates from…

Geophysics · Physics 2025-12-25 Murray Moinester , Joel Kronfeld

Emission from high-dipole moment molecules such as HCN allows determination of the density in molecular clouds, and is often considered to trace the "dense" gas available for star formation. We assess the importance of electron excitation…

Astrophysics of Galaxies · Physics 2017-08-28 Paul F. Goldsmith , Jens Kauffmann

Aims: Our aims are threefold: a) To compare the $uv$ and mm-wave results; b) to interpret 13CO and 12CO abundances in terms of the physical processes which separately and jointly determine them; c) to interpret observed J=1-0 rotational…

Astrophysics · Physics 2009-11-13 H. S. Liszt
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