Results 101 to 110 of about 2,531 (226)

Polarization of the Interplanetary Dust Medium (Invited)

, 2015
International audienceThe interplanetary dust cloud is visible through its scattered light (the zodiacal light) at visible wavelengths. Brightness observations lead to equilibrium temperature and albedo of the particles and their variation as a function ...
Hadamcik, Edith, Lasue, Jérémie, Levasseur-Regourd, Anny Chantal   +2 more
core   +1 more source

Detailed Radial Scale Height Profile of Dust Grains as Probed by Dust Self-scattering in HL Tau

The Astrophysical Journal Letters
The vertical settling of dust grains in a circumstellar disk, characterized by their scale height, is a pivotal process in the formation of planets. This study offers in-depth analysis and modeling of the radial scale height profile of dust grains in the
Haifeng Yang, Ian W. Stephens, Zhe-Yu Daniel Lin, Manuel Fernández-López, Zhi-Yun Li, Leslie W. Looney, Rachel Harrison   +6 more
doaj   +1 more source

Interaction of interplanetary dust particles with magnetic clouds

, 2009
Context. The interaction of the solar wind with interplanetary dust in the inner solar system appears to result in the formation of inner-source pickup ions.
R. F. Wimmer-Schweingruber, M. Wagner
core   +1 more source

Modeling and Analysis of Main-belt Asteroidal Dust Flux and Velocity Distribution at Inner Planets

The Astrophysical Journal
Interplanetary dust in the inner solar system originates from multiple sources, including short-period comets and main-belt asteroids. In this work, we focus specifically on the dynamical evolution of asteroid-derived dust using N -body simulations that ...
Aanchal Sahu, Jayesh Pabari
doaj   +1 more source

NanoSIMS-Analyse und hochauflösende Elektronenmikroskopie an präsolaren Silikaten aus roten Riesensternen und Supernovaexplosionen

, 2009
This thesis deals with the analysis of “presolar” silicates and oxides by high resolution mass spectrometry and electron microscopy techniques. This “stardust” was identified by its extreme oxygen isotopic anomalies, which point to nucleosynthetic ...
Vollmer, Christian
core  

Measurements of interplanetary dust particle flux from Explorer XVI CdS and wire grid dust particle detectors

, 1966
Interplanetary dust particle flux measured by Explorer XVI cadmium sulfide and wire grid dust particle ...
Secretan, L.
core  

South-North and radial traverses through the interplanetary dust cloud

, 1997
Identical in situ dust detectors are flown on board the Galileo and Ulysses spacecraft. They record impacts of micrometeoroids in the ecliptic plane at heliocentric distances from 0.7 to 5.4 AU and in a plane almost perpendicular to the ecliptic from -79
Zook, H. A., Hanner, M. S., Hanner, M., Morfill, G.E., Kissel, Jochen, Dermott, S., Polanskey, C., Zook, Harald, Hamilton, D. P., Morfill, G. E., Kissel, J., Zook, H., Linkert, G., McDonnell, J.A.M., Lindblad, B.A., Fechtig, H., Hanner, M.S., Schwehm, G., Grun, E., Mann, I., Hamilton, D.P., Horanyi, M., Lindblad, B., Hamilton, D., Staubach, P., Gustafson, B.A., Baguhl, M., Srama, Ralf, McDonnell, J. A. M., Gustafson, B. A., Gustafson, B., Linkert, D., Srama, R., Morfill, G., Lindblad, Bertil Anders, McDonnell, J.   +35 more
core   +1 more source

A Search for Meteoroid Streams and Their Sources in the Near-Sun Zodiacal Dust Cloud

The Astrophysical Journal
The structure and dynamics of the zodiacal cloud close to the Sun may be significantly influenced by the interaction between a background quasihomogeneous zodiacal cloud and discrete meteoroid streams associated with small bodies like comets and ...
David M. Malaspina, Jamey R. Szalay, Avery Mazurkiewicz, Delaney Lee-Bellows, Margaret E. Landis   +4 more
doaj   +1 more source

Comparison of GEMS in Interplanetary Dust Particles and GEMS-like Objects in a Stardust Impact Track in Aerogel. [PDF]

Meteorit Planet Sci, 2019
Ishii HA.
europepmc   +1 more source

Cometary evolution : clues on physical properties from chondritic interplanetary dust particles

, 1997
The degree of diversity or similarity detected in comets depends primarily on the lifetimes of the individual cometary nuclei at the time of analysis. It is inherent in our understanding of cometary orbital dynamics and the seminal model of comet origins
Rietmeijer, Frans J.M., Mackinnon, Ian D.R.   +1 more
core