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We build a conceptual coupled model of the climate and tidal evolution of the Earth-Moon system to find the influence of the former on the latter. An energy balance model is applied to calculate steady-state temperature field from the mean…

地球与行星天体物理 · 物理学 2019-09-25 Nan Wang , Zhi-Guo He

We have developed a characterization of the geological evolution of the Earths atmosphere and surface in order to model the observable spectra of an Earth-like planet through its geological history. These calculations are designed to guide…

天体物理学 · 物理学 2011-03-16 L. Kaltenegger , W. A. Traub , K. W. Jucks

It is straightforward to determine the size of the Earth and the distance to the Moon without making use of a telescope. The methods have been known since the 3rd century BC. However, few amateur or professional astronomers have worked this…

天体物理仪器与方法 · 物理学 2015-05-30 Kevin Krisciunas , Erika DeBenedictis , Jeremy Steeger , Agnes Bischoff-Kim , Gil Tabak , Kanika Pasricha

We directly determine the sensitivity and time delay of Earth's surface temperature response to annual solar irradiance variations from 60 years of data. A two-layer energy balance model is developed to interpret the results. Explaining…

天体物理学 · 物理学 2009-11-10 David H. Douglass , Eric G. Blackman , Robert S. Knox

The atmospheres of extrasolar giant planets are modeled with various effective temperatures and gravities, with and without clouds. Bond albedos are computed by calculating the ratio of the flux reflected by a planet (integrated over…

天体物理学 · 物理学 2009-10-31 Christopher R. Gelino , M. Marley , D. Stephens , J. Lunine , R. Freedman

The Total Solar Irradiance varies over a solar cycle of 11 years and maybe over cycles with longer period. Is the solar diameter variable over time too? We introduce a new method to perform high resolution astrometry of the solar diameter…

太阳与恒星天体物理 · 物理学 2012-02-20 Andrea Raponi , Costantino Sigismondi , Konrad Guhl , Richard Nugent , Andreas Tegtmeier

We use the GEANT4 Monte Carlo framework to calculate the gamma-ray albedo of the Moon due to interactions of cosmic ray (CR) nuclei with moon rock. Our calculation of the albedo spectrum agrees with the EGRET data. We show that the spectrum…

天体物理学 · 物理学 2009-02-25 Igor V. Moskalenko , Troy A. Porter

The ice-albedo feedback is a potentially important de-stabilizing effect for the climate of terrestrial planets. It is based on the positive feedback between decreasing surface temperatures, an increase of snow and ice cover and an…

地球与行星天体物理 · 物理学 2015-06-16 P. von Paris , F. Selsis , D. Kitzmann , H. Rauer

The mean surface temperature on Earth and other planets with atmospheres is determined by the radiative balance between the non-reflected incoming solar radiation and the outgoing long-wave black-body radiation from the atmosphere. The…

天体物理学 · 物理学 2009-11-11 Peter D. Ditlevsen

The Sun is the main energy source to Earth, and understanding its variability is of direct relevance to climate studies. Measurements of total solar irradiance exist since 1978, but this is too short compared to climate-relevant time…

太阳与恒星天体物理 · 物理学 2023-10-17 Theodosios Chatzistergos , Natalie A. Krivova , Kok Leng Yeo

The vegetation's ``red edge'', an intensity bump in the Earth's spectrum near 700 $nm$ when sunlight is reflected from greenery, is often suggested as a tool in the search for life in terrestrial-like extrasolar planets. Here, through…

天体物理学 · 物理学 2008-11-26 Pilar Montanes-Rodriguez , E. Palle , P. R. Goode

Climate change is affecting and will increasingly affect astronomical observations. In this paper, we investigated the role some key weather parameters play in the quality of astronomical observations, and analysed their long-term trends…

We proposed an analytical model for the calculus of illumination time of the Earth for any time of year and any latitude, this model assumes the obliquity of the ecliptic as constant, the light beams as parallels, the Earth as spherical,…

地球与行星天体物理 · 物理学 2012-10-15 Paco Talero , Fernanda Santana , César Mora

It will be shown that the rotation of the Earth in the Earth-Moon system can be detected by comparing the deflection of a Foucault pendulum at noon on the one hand and at midnight on the other hand. More precisely, on 21 June the midnight…

经典物理 · 物理学 2011-12-23 Bertrand M. Roehner

The state of earth's climate is constrained by well-known physical principles such as energy balance and the conservation of energy. Increased greenhouse gas concentrations affect the atmospheric optical depth, and physical consistency…

大气与海洋物理 · 物理学 2011-06-27 Rasmus E. Benestad

A surprisingly large amount of information on our solar system can be gained from simple measurements of the apparent angular diameters of the sun and the moon. This information includes the average density of the sun, the distance between…

物理教育 · 物理学 2009-11-10 K. Capelle

We report the visible reflection spectrum of the integrated Earth, illuminated as it would be seen as an spatially-unresolved extrasolar planet. The spectrum was derived from observation of lunar earthshine in the range 4800 to 9200…

天体物理学 · 物理学 2009-11-07 N. J. Woolf , P. S. Smith , W. A. Traub , K. W. Jucks

In a recent article by Scafetta, 2010, the author investigates whether or not the decadal and multi-decadal climate oscillations have an astronomical origin. In particular, the author note that several global surface temperature records,…

数据分析、统计与概率 · 物理学 2011-05-20 S. Sello

Over the past two decades, enormous advances in the detection of exoplanets have taken place. Currently, we have discovered hundreds of earth-sized planets, several of them within the habitable zone of their star. In the coming years, the…

地球与行星天体物理 · 物理学 2018-12-05 Enric Palle

The evolution of Earth-Moon system is described by the dark matter field fluid model proposed in the Meeting of Division of Particle and Field 2004, American Physical Society. The current behavior of the Earth-Moon system agrees with this…

综合物理 · 物理学 2008-01-13 Hongjun Pan