Sub-micron interplanetary dust

Details Sub-micron interplanetary dust Sub-micron interplanetary dust

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177p.117p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 177, Dec. 1976, p. 117P-120P.

Astronomy and Astrophysics

Astrophysics

1

Interplanetary Dust, Olivine, Particle Size Distribution, Refractivity, Zodiacal Light, Astrophysics, Chemical Composition, Equilibrium Equations, Saha Equations, Solar Wind

Scientific paper

Observations of zodiacal light indicate that the imaginary part of the refractive index of interplanetary grains is approximately equal to 0.01. The high conductivity implied by this value is difficult to reconcile with the composition of the grains. Olivine is capable of the implied conductivity only if it is saturated with 'donor' hydrogen of solar-wind origin.

Affiliated with

Also associated with

No associations

Rating

Sub-micron interplanetary dust does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Sub-micron interplanetary dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sub-micron interplanetary dust will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1051750