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相关论文: Earthshine as an Illumination Source at the Moon

200 篇论文

Measurements from the Solar Irradiance Monitor (SIM) onboard the SORCE mission indicate that solar spectral irradiance at Visible and IR wavelengths varies in counter phase with the solar activity cycle. The sign of these variations is not…

太阳与恒星天体物理 · 物理学 2015-06-19 Serena Criscuoli , Han Uitenbroek

Moons orbiting extrasolar planets are the next class of object to be observed and characterized for possible habitability. Like the host-planets to their host-star, exomoons have a limiting radius at which they may be gravitationally bound,…

地球与行星天体物理 · 物理学 2015-06-16 Natalie R. Hinkel , Stephen R. Kane

The Sun albedo of cosmic rays at GeVs energy has been discovered recently by FERMI satellite. They are traces of atmospheric CR hitting solar atmosphere and reflecting skimming gamma photons. Even if relevant for astrophysics, as being…

高能天体物理现象 · 物理学 2018-10-05 Daniele Fargion , Pietro Oliva , Pier Giorgio De Sanctis Lucentini , Maxim Yu. Khlopov

Using viscoelastic mass spring model simulations to track heat distribution inside a tidally perturbed body, we measure the asymmetry of heating in the crust of a spin synchronous Moon in eccentric orbit about the Earth. With the Moon…

地球与行星天体物理 · 物理学 2019-05-01 Alice C. Quillen , Larkin Martini , Miki Nakajima

The Mauna Loa Observatory record of direct-beam solar irradiance measurements for the years 1958-2010 is analysed to investigate the variation of clear-sky terrestrial insolation with solar activity over more than four solar cycles. The raw…

地球与行星天体物理 · 物理学 2013-01-22 Georg Feulner

The light scattered by an extrasolar Earth-like planet's surface and atmosphere will vary in intensity and color as the planet rotates; the resulting light curve will contain information about the planet's properties. Since most of the…

天体物理学 · 物理学 2007-05-23 Eric B. Ford , Sara Seager , Edwin L. Turner

The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3+C muon spectrometer at CERN. A significant effect of the Earth magnetic field is observed. Since no event…

天体物理学 · 物理学 2008-11-26 L3 Collaboration , P. Achard

Numerous missions planned for the next decade are likely to target a handful of smal sites of interest on the Moon's surface, creating risks of crowding and interference at these locations. The Moon presents finite and scarce areas with…

科普物理 · 物理学 2021-03-17 Martin Elvis , Alanna Krolikowski , Tony Milligan

Atmospheric electrification is not a purely terrestrial phenomenon: all Solar System planetary atmospheres become slightly electrified by cosmic ray ionisation. There is evidence for lightning on Jupiter, Saturn, Uranus and Neptune, and it…

地球物理 · 物理学 2007-05-23 Karen Aplin

In Papers II and III we show that Transient Lunar Phenomena (TLPs) are likely related to lunar outgassing, albeit in ways not fully understood. Here we propose a path forward, in which current and forthcoming technologies provide a more…

天体物理学 · 物理学 2007-06-28 Arlin P. S. Crotts

Can we observe the solar eclipses in the neutrino light? In principle, this is possible by identifying the lunar matter effects on the flavor conversions of solar neutrinos when they traverse the Moon before reaching the detectors at the…

高能物理 - 唯象学 · 物理学 2018-05-09 Guo-yuan Huang , Jun-Hao Liu , Shun Zhou

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

We present a comprehensive set of spectropolarimetric observations of Earthshine as obtained by FORS2 at the VLT for phase angles from 50degree to 135degree (Sun-Earth-Moon angle), covering a spectral range from 430nm to 920nm. The degree…

地球与行星天体物理 · 物理学 2019-01-30 Michael F. Sterzik , Stefano Bagnulo , Daphne M. Stam , Claudia Emde , Mihail Manev

Multiple nations are planning activity on the Moon's surface, and to deconflict lunar operations we must understand the sandblasting damage from rocket exhaust blowing soil. Prior research disagreed over the scaling of the erosion rate,…

地球与行星天体物理 · 物理学 2024-03-28 Philip Metzger

We present a new rough-surface thermophysical model (Advanced Thermophysical Model or ATPM) that describes the observed directional thermal emission from any atmosphereless planetary surface. It explicitly incorporates partial shadowing,…

地球与行星天体物理 · 物理学 2012-11-09 Ben Rozitis , Simon F. Green

The formation of electric potential over lunar magnetized regions is essential for understanding fundamental lunar science, for understanding the lunar environment, and for planning human exploration on the Moon. A large positive electric…

空间物理 · 物理学 2013-02-26 Y. Futaana , S. Barabash , M. Wieser , C. Lue , P. Wurz , A. Vorburger , A. Bhardwaj , K. Asamura

The applicability of the linear theory of elasticity to the Moon has been studied. As a criterion was taken the smallness of the strain tensor. The elastic moduli are obtained from the data of the project "Apollo". The pressure was…

地球物理 · 物理学 2017-06-29 Vladimir Pavlov

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

Magnetic features on the surfaces of cool stars cause variations of their brightness. Such variations have been extensively studied for the Sun. Recent planet-hunting space telescopes allowed measuring brightness variations in hundred…

太阳与恒星天体物理 · 物理学 2020-04-15 N. -E. Nèmec , A. I. Shapiro , N. A. Krivova , S. K. Solanki , R. V. Tagirov , R. H. Cameron , S. Dreizler