Results 91 to 100 of about 156 (136)

Using dimers to measure biosignatures and atmospheric pressure for terrestrial exoplanets. [PDF]

Astrobiology, 2014
Misra A, Meadows V, Claire M, Crisp D.
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Cometary Dust. [PDF]

Space Sci Rev, 2018
Levasseur-Regourd AC, Agarwal J, Cottin H, Engrand C, Flynn G, Fulle M, Gombosi T, Langevin Y, Lasue J, Mannel T, Merouane S, Poch O, Thomas N, Westphal A.   +13 more
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Solar wind stream interaction regions throughout the heliosphere. [PDF]

Living Rev Sol Phys, 2018
Richardson IG.
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The nature, origin and modification of insoluble organic matter in chondrites, the possibly interstellar source of Earth's C and N. [PDF]

Chem Erde, 2017
Alexander CMO, Cody GD, De Gregorio BT, Nittler LR, Stroud RM.   +4 more
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Astrophysical symmetries. [PDF]

Proc Natl Acad Sci U S A, 1996
Trimble V.
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Micrometeorite collections: a review and their current status. [PDF]

Philos Trans A Math Phys Eng Sci
van Ginneken M, Wozniakiewicz PJ, Brownlee DE, Debaille V, Della Corte V, Delauche L, Duprat J, Engrand C, Folco L, Fries M, Gattacceca J, Genge MJ, Goderis S, Gounelle M, Harvey RP, Jonker G, Krämer Ruggiu L, Larsen J, Lever JH, Noguchi T, Peterson S, Rochette P, Rojas J, Rotundi A, Rudraswami NG, Suttle MD, Taylor S, Van Maldeghem F, Zolensky M.   +28 more
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A physical model for thermal emission from the zodiacal dust cloud

, 1988
Deul, E.R., Wolstencroft, R.D.
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Out of ecliptic zodiacal cloud profile

Planetary and Space Science, 1983
Abstract In a previous paper, Mujica et al (1980), the optical homogeneity of the medium in the ecliptic plane was established calculating, for the ecliptic, the density and scattering functions ρ(r) and σ(θ) respectively. Starting with these results, we attempt now to find the zodiacal cloud shape out of the ecliptic.
A. Mujica, G. López, F. Sánchez
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Dynamical Structure of the Zodiacal Cloud

1999
Advances in infrared astronomy and computing power have made detailed study of the structure of the zodiacal cloud possible. An extremely complex cloud has been revealed, quite distinct from the smooth, rotationally symmetric structure assumed prior to the launch of IRAS.
S. F. Dermott, K. Grogan, E. Holmes, S. Kortenkamp   +3 more
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Origins of the zodiacal dust cloud

Journal of Geophysical Research, 1963
The total intensity of light scattered by interplanetary dust has usually been directly related to the dust mass lost because of the Poynting-Robertson effect. The scattered light intensity thus would appear to define a dust supply rate that must be maintained if the dust intensity is to remain constant. This work suggests that comets apparently cannot
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