Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...261..329m&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 261, no. 1, p. 329-335.
Astronomy and Astrophysics
Astrophysics
42
Brightness Distribution, Infrared Spectra, Interplanetary Dust, Interplanetary Medium, Solar Corona, Stellar Envelopes, Polarization Characteristics, Remote Sensing, Scattering, Solar Radiation, Thermal Emission
Scientific paper
The brightness of the solar F-corona along the ecliptic is calculated in the visual and near-IR spectral range, and the results are discussed with respect to future observations. It is shown that dust particles close to the sun have a strong influence on the corona brightness, which enables their investigation by remote sensing experiments. Comparison of model calculations with the observations indicates that the zodiacal dust cloud remains mainly undisturbed up to the beginning of a dust-free zone that amounts to about 5 solar radii. Calculations of visual brightness and polarization indicate a change of particle properties for a solar distance smaller than 20, which has to be proven by future experiments. The IR F-corona brightness has contributions from solar radiation scattered at dust particles up to wavelengths of 5 microns. The superposition with the thermal emission of particles produces a significant feature at the edge of the dust-free zone but the existence of an additional dust ring cannot be supported. The observational data at 10 microns are found to be in contradiction to the present study.
No associations
LandOfFree
The solar F-corona - Calculations of the optical and infrared brightness of circumsolar 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 The solar F-corona - Calculations of the optical and infrared brightness of circumsolar dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The solar F-corona - Calculations of the optical and infrared brightness of circumsolar dust will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1203325