Comparative Studies of Visible and IRAS Interplanetary Dust Bands | Zendy

Masateru Ishiguro | Zendy; Ryosuke Nakamura | Zendy; Yasumasa Fujii | Zendy; T. Mukai | Zendy

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Comparative Studies of Visible and IRAS Interplanetary Dust Bands

Author(s) -

Masateru Ishiguro,

Ryosuke Nakamura,

Yasumasa Fujii,

T. Mukai

Publication year - 1999

Publication title -

publications of the astronomical society of japan

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.99

H-Index - 110

eISSN - 2053-051X

pISSN - 0004-6264

DOI - 10.1093/pasj/51.3.363

Subject(s) - physics , interplanetary dust cloud , infrared , astrophysics , astronomy , cosmic dust , visible spectrum , interplanetary medium , extinction (optical mineralogy) , latitude , solar system , interplanetary spaceflight , solar wind , optics , quantum mechanics , magnetic field

We have examined the diversity and similarity of visible dust bands and infrared dust bands based on data obtained by our ground-based observations (Ishiguro et al. 1999, ApJ 511, 432) and by the Infrared Astronomy Satellite (IRAS). It is found that the latitude profile of visible dust bands at the solar elongation, λ - λ⊙ = 89°, is similar to that of infrared dust bands, except for the appearance...

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