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Journal articles on the topic 'Atmospheric Science'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Chyba, C. F. "ATMOSPHERIC SCIENCE: Rethinking Earth's Early Atmosphere." Science 308, no. 5724 (2005): 962–63. http://dx.doi.org/10.1126/science.1113157.

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2

Pawson, S. "Atmospheric science." Earth-Science Reviews 30, no. 3-4 (1991): 319–20. http://dx.doi.org/10.1016/0012-8252(91)90002-w.

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3

CICERONE, R. J. "Atmospheric Chemistry: The Photochemistry of Atmospheres." Science 233, no. 4766 (1986): 896–97. http://dx.doi.org/10.1126/science.233.4766.896-a.

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4

Hartmann, D. L., and H. H. Hendon. "ATMOSPHERIC SCIENCE: Resolving an Atmospheric Enigma." Science 318, no. 5857 (2007): 1731–32. http://dx.doi.org/10.1126/science.1152502.

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5

Jarvis, M. J. "ATMOSPHERIC SCIENCE: Bridging the Atmospheric Divide." Science 293, no. 5538 (2001): 2218–19. http://dx.doi.org/10.1126/science.1064467.

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6

Habib, Namrah, and Raymond T. Pierrehumbert. "Modeling Noncondensing Compositional Convection for Applications to Super-Earth and Sub-Neptune Atmospheres." Astrophysical Journal 961, no. 1 (2024): 35. http://dx.doi.org/10.3847/1538-4357/ad04e2.

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Abstract Compositional convection is atmospheric mixing driven by density variations caused by compositional gradients. Previous studies have suggested that compositional gradients of atmospheric trace species within planetary atmospheres can impact convection and the final atmospheric temperature profile. In this work, we employ 3D convection-resolving simulations using Cloud Model 1 (CM1) to gain a fundamental understanding of how compositional variation influences convection and the final atmospheric state of exoplanet atmospheres. We perform 3D initial value problem simulations of nonconde

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7

Kockarts, G. "Aeronomy, a 20th Century emergent science: the role of solar Lyman series." Annales Geophysicae 20, no. 5 (2002): 585–98. http://dx.doi.org/10.5194/angeo-20-585-2002.

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Abstract. Aeronomy is, by definition, a multidisciplinary science which can be used to study the terrestrial atmosphere, as well as any planetary atmosphere and even the interplanetary space. It was officially recognized in 1954 by the International Union of Geodesy and Geophysics. The major objective of the present paper is to show how aeronomy developed since its infancy. The subject is so large that a guide-line has been chosen to see how aeronomy affects our atmospheric knowledge. This guideline is the solar Lyman alpha radiation which has different effects in the solar system. After a sho

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8

Law, Cliff S., Emilie Brévière, Gerrit de Leeuw, et al. "Evolving research directions in Surface Ocean - Lower Atmosphere (SOLAS) science." Environmental Chemistry 10, no. 1 (2013): 1. http://dx.doi.org/10.1071/en12159.

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Environmental context Understanding the exchange of energy, gases and particles at the ocean–atmosphere interface is critical for the development of robust predictions of, and response to, future climate change. The international Surface Ocean–Lower Atmosphere Study (SOLAS) coordinates multi-disciplinary ocean–atmosphere research projects that quantify and characterise this exchange. This article details five new SOLAS research strategies – upwellings and associated oxygen minimum zones, sea ice, marine aerosols, atmospheric nutrient supply and ship emissions – that aim to improve knowledge in

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9

Vega, Anthony J. "Inventing Atmospheric Science." AAG Review of Books 4, no. 3 (2016): 153–55. http://dx.doi.org/10.1080/2325548x.2016.1187501.

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10

Sy, Lloyd Alimboyao. "Hans Pfaall's Breath: Edgar Allan Poe and Antebellum Atmospheres." Poe Studies 57, no. 1 (2024): 129–52. http://dx.doi.org/10.1353/poe.2024.a939002.

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ABSTRACT: This essay examines the connections between Edgar Allan Poe's "The Unparalleled Adventure of One Hans Pfaall" and the scientific and political discourse of antebellum America, particularly insofar as it centered on atmospheric science. This essay argues that Poe's story should be read within an antebellum comprehension of atmospheric science that used the atmosphere as a metaphor to comment on freedom, revolution, and slavery. I read Hans's journey through the atmosphere as a thought experiment addressing the contemporary scientific challenge of measuring the upper atmosphere, while

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11

Radmilović-Radjenović, Marija, Martin Sabo, and Branislav Radjenović. "Transport Characteristics of the Electrification and Lightning of the Gas Mixture Representing the Atmospheres of the Solar System Planets." Atmosphere 12, no. 4 (2021): 438. http://dx.doi.org/10.3390/atmos12040438.

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Electrification represents a fundamental process in planetary atmospheres, widespread in the Solar System. The atmospheres of the terrestrial planets (Venus, Earth, and Mars) range from thin to thick are rich in heavier gases and gaseous compounds, such as carbon dioxide, nitrogen, oxygen, argon, sodium, sulfur dioxide, and carbon monoxide. The Jovian planets (Jupiter, Saturn, Uranus, and Neptune) have thick atmospheres mainly composed of hydrogen and helium involving. The electrical discharge processes occur in the planetary atmospheres leading to potential hazards due to arcing on landers an

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12

Smith, H. J. "ATMOSPHERIC SCIENCE: Vegetation Effects on Atmospheric Pollution." Science 302, no. 5643 (2003): 201a—201. http://dx.doi.org/10.1126/science.302.5643.201a.

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13

Yuan, Bao-Zhong, and Jie Sun. "Research trend the in meteorology and atmospheric sciences category based on essential science indicators during 2011–2021." Időjárás 127, no. 3 (2023): 299–319. http://dx.doi.org/10.28974/idojaras.2023.3.3.

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This study analyzed 1,636 top papers in the subject category of meteorology and atmospheric sciences about eleven years from 2011 to 2021, which included 1,636 highly cited papers and 24 hot papers in the field belonged to 20 Web of Science categories and 14 research areas. All top papers, written in English, were from 13,878 authors, 2,913 organizations, and 124 countries or territories, and published in 72 journals in the field. The top five journals are the Nature Climate Change (15.9% of the studied paper), Atmospheric Chemistry and Physics (12.1%), Journal of Climate (7.0%), Bulletin of t

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14

RICHMOND, A. D. "Atmospheric Physics: Atmospheric Electrodynamics." Science 228, no. 4699 (1985): 572–73. http://dx.doi.org/10.1126/science.228.4699.572-a.

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15

Ragossnig, Florian, Alexander Stökl, Ernst Dorfi, Colin P. Johnstone, Daniel Steiner, and Manuel Güdel. "Interaction of infalling solid bodies with primordial atmospheres of disk-embedded planets." Astronomy & Astrophysics 618 (October 2018): A19. http://dx.doi.org/10.1051/0004-6361/201832681.

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Context. Planets that form early enough to be embedded in the circumstellar gas disk accumulate thick atmospheres of nebular gas. Models of these atmospheres need to specify the surface luminosity (i.e. energy loss rate) of the planet. This luminosity is usually associated with a continuous inflow of solid bodies, where the gravitational energy released from these bodies is the source of energy. However, if these bodies release energy in the atmosphere instead of at the surface, this assumption might not be justified. Aims. Our aim is to explore the interactions of infalling planetesimals with

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16

Ridden-Harper, Andrew, Stevanus K. Nugroho, Laura Flagg, et al. "High-resolution Transmission Spectroscopy of the Terrestrial Exoplanet GJ 486b." Astronomical Journal 165, no. 4 (2023): 170. http://dx.doi.org/10.3847/1538-3881/acbd39.

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Abstract Terrestrial exoplanets orbiting M-dwarf stars are promising targets for transmission spectroscopy with existing or near-future instrumentation. The atmospheric composition of such rocky planets remains an open question, especially given the high X-ray and ultraviolet flux from their host M dwarfs that can drive atmospheric escape. The 1.3 R ⊕ exoplanet GJ 486b (T eq ∼ 700 K), orbiting an M3.5 star, is expected to have one of the strongest transmission spectroscopy signals among known terrestrial exoplanets. We observed three transits of GJ 486b using three different high-resolution sp

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17

Krissansen-Totton, Joshua. "Implications of Atmospheric Nondetections for Trappist-1 Inner Planets on Atmospheric Retention Prospects for Outer Planets." Astrophysical Journal Letters 951, no. 2 (2023): L39. http://dx.doi.org/10.3847/2041-8213/acdc26.

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Abstract JWST secondary eclipse observations of Trappist-1b seemingly disfavor atmospheres >∼1 bar since heat redistribution is expected to yield dayside emission temperature below the ∼500 K observed. Given the similar densities of Trappist-1 planets, and the theoretical potential for atmospheric erosion around late M dwarfs, this observation might be assumed to imply substantial atmospheres are also unlikely for the outer planets. However, the processes governing atmosphere erosion and replenishment are fundamentally different for inner and outer planets. Here, an atmosphere–interior evol

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18

Medvedev, Alexander S., and Erdal Yiğit. "Gravity Waves in Planetary Atmospheres: Their Effects and Parameterization in Global Circulation Models." Atmosphere 10, no. 9 (2019): 531. http://dx.doi.org/10.3390/atmos10090531.

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The dynamical and thermodynamical importance of gravity waves was initially recognized in the atmosphere of Earth. Extensive studies over recent decades demonstrated that gravity waves exist in atmospheres of other planets, similarly play a significant role in the vertical coupling of atmospheric layers and, thus, must be included in numerical general circulation models. Since the spatial scales of gravity waves are smaller than the typical spatial resolution of most models, atmospheric forcing produced by them must be parameterized. This paper presents a review of gravity waves in planetary a

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19

Romanovskii, Oleg A., and Gennadii G. Matvienko. "Atmospheric and Ocean Optics: Atmospheric Physics." Atmosphere 12, no. 4 (2021): 468. http://dx.doi.org/10.3390/atmos12040468.

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20

Chance, Quadry, Sarah Ballard, and Keivan Stassun. "Signatures of Impact-driven Atmospheric Loss in Large Ensembles of Exoplanets." Astrophysical Journal 937, no. 1 (2022): 39. http://dx.doi.org/10.3847/1538-4357/ac8a97.

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Abstract The results of large-scale exoplanet transit surveys indicate that the distribution of small planet radii is likely sculpted by atmospheric loss. Several possible physical mechanisms exist for this loss of primordial atmospheres, each of which produces a different set of observational signatures. In this study, we investigate the impact-driven mode of atmosphere loss via N-body simulations. We compare the results from giant impacts, at a demographic level, to results from another commonly invoked method of atmosphere loss, photoevaporation. Applying two different loss prescriptions to

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21

GORDON, G. E. "Atmospheric Science: Atmospheric Chemistry and Atmospheric Chemistry and Physics of Air Pollution." Science 235, no. 4793 (1987): 1263b—1264b. http://dx.doi.org/10.1126/science.235.4793.1263b.

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22

Watanabe, Yasuto, and Kazumi Ozaki. "Relative Abundances of CO₂, CO, and CH₄ in Atmospheres of Earth-like Lifeless Planets." Astrophysical Journal 961, no. 1 (2024): 1. http://dx.doi.org/10.3847/1538-4357/ad10a2.

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Abstract 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 model of atmospheric chemistry to investigate diversity in the atmospheric abundances of CO2, CO, and CH4 on Earth-like lifeless planets orbiting Sun-like (F-, G-, and K-type) stars. We focused on the conditions for the formation of a CO-rich atmosphere, which would be favorable for the origin of life. Results demonstrated that elevated atmospheric C

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23

Wackett, Lawrence P. "Microbiology of atmospheric science." Environmental Microbiology 23, no. 2 (2021): 1298–99. http://dx.doi.org/10.1111/1462-2920.15427.

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24

Brauman, J. I. "Issues in Atmospheric Science." Science 243, no. 4892 (1989): 709. http://dx.doi.org/10.1126/science.243.4892.709.

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25

Smith, H. J. "ATMOSPHERIC SCIENCE: Remote Inversions." Science 291, no. 5502 (2005): 213b—213. http://dx.doi.org/10.1126/science.291.5502.213b.

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26

Smith, H. J. "ATMOSPHERIC SCIENCE: Serendipitous Surcease." Science 305, no. 5685 (2004): 755a. http://dx.doi.org/10.1126/science.305.5685.755a.

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27

Smith, H. J. "ATMOSPHERIC SCIENCE: Violet Rain." Science 301, no. 5639 (2003): 1447a—1447. http://dx.doi.org/10.1126/science.301.5639.1447a.

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28

Hanson, B. "ATMOSPHERIC SCIENCE: Parisian Airs." Science 301, no. 5641 (2003): 1815b—1815. http://dx.doi.org/10.1126/science.301.5641.1815b.

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29

Smith, H. J. "ATMOSPHERIC SCIENCE: Icy Complications." Science 302, no. 5647 (2003): 951d—951. http://dx.doi.org/10.1126/science.302.5647.951d.

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30

Smith, H. J. "ATMOSPHERIC SCIENCE: Clean Competition." Science 314, no. 5803 (2006): 1219a. http://dx.doi.org/10.1126/science.314.5803.1219a.

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31

Smith, H. J. "ATMOSPHERIC SCIENCE: Sourcing Methane." Science 316, no. 5826 (2007): 799b. http://dx.doi.org/10.1126/science.316.5826.799b.

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32

Smith, H. J. "ATMOSPHERIC SCIENCE: Fat Coats." Science 308, no. 5721 (2005): 469c. http://dx.doi.org/10.1126/science.308.5721.469c.

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33

Erickson, Britt. "Science: Atmospheric pressure MALDI." Analytical Chemistry 72, no. 5 (2000): 186 A. http://dx.doi.org/10.1021/ac002757e.

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34

Solow, Andrew R. "Statistics in Atmospheric Science." Statistical Science 18, no. 4 (2003): 422–29. http://dx.doi.org/10.1214/ss/1081443226.

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35

Hanson, B. "ATMOSPHERIC SCIENCE: Air Supplies." Science 294, no. 5546 (2001): 1419a—1419. http://dx.doi.org/10.1126/science.294.5546.1419a.

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36

Smith, H. J. "ATMOSPHERIC SCIENCE: Certainly Warmer." Science 298, no. 5593 (2002): 497d—497. http://dx.doi.org/10.1126/science.298.5593.497d.

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37

Smith, H. J. "ATMOSPHERIC SCIENCE: Carbon Budgeting." Science 298, no. 5599 (2002): 1681a—1681. http://dx.doi.org/10.1126/science.298.5599.1681a.

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38

Robock, A. "ATMOSPHERIC SCIENCE: Whither Geoengineering?" Science 320, no. 5880 (2008): 1166–67. http://dx.doi.org/10.1126/science.1159280.

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39

Bromwich, David H. "Climatology: An atmospheric science." Geochimica et Cosmochimica Acta 57, no. 19 (1993): 4863. http://dx.doi.org/10.1016/0016-7037(93)90208-e.

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40

Slonaker, Richard L. "Handbook of Atmospheric Science." Atmospheric Research 70, no. 2 (2004): 143–45. http://dx.doi.org/10.1016/j.atmosres.2004.03.001.

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41

Romanovskii, Oleg A., and Gennadii G. Matvienko. "Atmospheric and Ocean Optics: Atmospheric Physics II." Atmosphere 12, no. 4 (2021): 430. http://dx.doi.org/10.3390/atmos12040430.

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42

Chouqar, J., Z. Benkhaldoun, A. Jabiri, J. Lustig-Yaeger, A. Soubkiou, and A. Szentgyorgyi. "Properties of sub-Neptune atmospheres: TOI-270 system." Monthly Notices of the Royal Astronomical Society 495, no. 1 (2020): 962–70. http://dx.doi.org/10.1093/mnras/staa1198.

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ABSTRACT We investigate the potential for the James Webb Space Telescope (JWST) to detect and characterize the atmospheres of the sub-Neptunian exoplanets in the TOI-270 system. Sub-Neptunes are considered more likely to be water worlds than gas dwarfs. We model their atmospheres using three atmospheric compositions – two examples of hydrogen-dominated atmospheres and a water-dominated atmosphere. We then simulate the infrared transmission spectra of these atmospheres for JWST instrument modes optimized for transit observation of exoplanet atmospheres: NIRISS, NIRSpec, and MIRI. We then predic

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43

Teng, Chen-Ke-Min, Sheng-Yang Gu, Yusong Qin, and Xiankang Dou. "Impact of Solar Activity on Global Atmospheric Circulation Based on SD-WACCM-X Simulations from 2002 to 2019." Atmosphere 12, no. 11 (2021): 1526. http://dx.doi.org/10.3390/atmos12111526.

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In this study, a global atmospheric model, Specified Dynamics Whole Atmosphere Community Climate Model with thermosphere and ionosphere eXtension (SD-WACCM-X), and the residual circulation principle were used to study the global atmospheric circulation from the lower to upper atmosphere (~500 km) from 2002 to 2019. Our analysis shows that the atmospheric circulation is clearly influenced by solar activity, especially in the upper atmosphere, which is mainly characterized by an enhanced atmospheric circulation in years with high solar activity. The atmospheric circulation in the upper atmospher

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44

Petzold, Andreas, Ulrich Bundke, Anca Hienola, et al. "Opinion: New directions in atmospheric research offered by research infrastructures combined with open and data-intensive science." Atmospheric Chemistry and Physics 24, no. 9 (2024): 5369–88. http://dx.doi.org/10.5194/acp-24-5369-2024.

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Abstract. The acquisition and dissemination of essential information for understanding global biogeochemical interactions between the atmosphere and ecosystems and how climate–ecosystem feedback loops may change atmospheric composition in the future comprise a fundamental prerequisite for societal resilience in the face of climate change. In particular, the detection of trends and seasonality in the abundance of greenhouse gases and short-lived climate-active atmospheric constituents is an important aspect of climate science. Therefore, easy and fast access to reliable, long-term, and high-qua

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45

Madhusudhan, Nikku, Subhajit Sarkar, Savvas Constantinou, Måns Holmberg, Anjali A. A. Piette, and Julianne I. Moses. "Carbon-bearing Molecules in a Possible Hycean Atmosphere." Astrophysical Journal Letters 956, no. 1 (2023): L13. http://dx.doi.org/10.3847/2041-8213/acf577.

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Abstract The search for habitable environments and biomarkers in exoplanetary atmospheres is the holy grail of exoplanet science. The detection of atmospheric signatures of habitable Earth-like exoplanets is challenging owing to their small planet–star size contrast and thin atmospheres with high mean molecular weight. Recently, a new class of habitable exoplanets, called Hycean worlds, has been proposed, defined as temperate ocean-covered worlds with H2-rich atmospheres. Their large sizes and extended atmospheres, compared to rocky planets of the same mass, make Hycean worlds significantly mo

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46

Herbst, Konstantin, Saša Banjac, and Tom A. Nordheim. "Revisiting the cosmic-ray induced Venusian ionization with the Atmospheric Radiation Interaction Simulator (AtRIS)." Astronomy & Astrophysics 624 (April 2019): A124. http://dx.doi.org/10.1051/0004-6361/201935152.

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Context. Cosmic ray bombardment represents a major source of ionization in planetary atmospheres. The higher the energy of the primary cosmic ray particles, the deeper they can penetrate into the atmosphere. In addition, incident high energy cosmic ray particles induce extensive secondary particle cascades (“air showers”) that can contain up to several billion secondary particles per incoming primary particle. To quantify cosmic ray-induced effects on planetary atmospheres it is therefore important to accurately model the entire secondary particle cascade. This is particularly important in thi

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47

Westing;, A. H. "Atmospheric Ethics." Science 291, no. 5505 (2001): 827c—828. http://dx.doi.org/10.1126/science.291.5505.827c.

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48

Somerville, R. C. J. "Atmospheric Interplay." Science 264, no. 5155 (1994): 115. http://dx.doi.org/10.1126/science.264.5155.115.

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49

Marshak, A., Y. Knyazikhin, J. C. Chiu, and W. J. Wiscombe. "Spectrally Invariant Approximation within Atmospheric Radiative Transfer." Journal of the Atmospheric Sciences 68, no. 12 (2011): 3094–111. http://dx.doi.org/10.1175/jas-d-11-060.1.

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Abstract Certain algebraic combinations of single scattering albedo and solar radiation reflected from, or transmitted through, vegetation canopies do not vary with wavelength. These “spectrally invariant relationships” are the consequence of wavelength independence of the extinction coefficient and scattering phase function in vegetation. In general, this wavelength independence does not hold in the atmosphere, but in cloud-dominated atmospheres the total extinction and total scattering phase function vary only weakly with wavelength. This paper identifies the atmospheric conditions under whi

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50

Zhang, Xi, Cheng Li, Huazhi Ge, and Tianhao Le. "The Inhomogeneity Effect. III. Weather Impacts on the Heat Flow of Hot Jupiters." Astrophysical Journal 957, no. 1 (2023): 22. http://dx.doi.org/10.3847/1538-4357/acee7d.

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Abstract The interior flux of a giant planet impacts atmospheric motion, and the atmosphere dictates the interior’s cooling. Here we use a non-hydrostatic general circulation model (Simulating Non-hydrostatic Atmospheres on Planets) coupled with a multi-stream multi-scattering radiative module (High-performance Atmospheric Radiation Package) to simulate the weather impacts on the heat flow of hot Jupiters. We found that the vertical heat flux is primarily transported by convection in the lower atmosphere and regulated by dynamics and radiation in the overlying radiation-circulation zone. The t

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