Outline of a Method for Determining the Absorption in the Surroundings of the Sun

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Communications Faculty of Sciences University Ankara Series A1 Mathematics and Statistics
Volume:10
Outline of a Method for Determining the Absorption in the Surroundings of the Sun

Outline of a Method for Determining the Absorption in the Surroundings of the Sun

Authors : Ea KREIKEN

Pages : 0-0

Doi:10.1501/Commua1_0000000092

View : 13 | Download : 10

Publication Date : 1959-01-01

Article Type : Research Paper

Abstract :In the follovving a method is proposed to determine the mean coefficient of interstellar absorption and the mean extinction from the observed spectroscopic parallazes, the radial velocity and the proper moti- ons. The distribution $ insert ignore into journalissuearticles values(x, y, z/S); is assumed to be constant in the immedi- ate surroundings of the sun. This is a reasonable assumption. Therefore the velocity Iaw must be a constant along any axis. independent of its orienta- tion. In different areas of the sky it is cor.venient to adopt as axis the radi- us vector and the direetion perpendieular to and tangent to the cireles »and S The equations of motion containing a are derived. From these the nume- rical values of a can easily be derived.
Keywords : Outline, Method for Determining, Absorption

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