Author: Theodore John Pepin
Publisher:
ISBN:
Category :
Languages : en
Pages : 194
Book Description
Part I Observations of the Brightness and Polarization of the Outer Corona During the November 12, 1966 Total Eclipse of the Sun
Author: Theodore John Pepin
Publisher:
ISBN:
Category :
Languages : en
Pages : 194
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 194
Book Description
Part 1: Observations of the Brightness and Polarization of the Outer Corona During the November 12, 1966 Total Eclipse of the Sun. Part 2: The Use of Extinction from High Altitude Balloons as a Probe of the Atmospheric Aerosols
Author: Theodore John Pepin
Publisher:
ISBN:
Category : Sun
Languages : en
Pages : 194
Book Description
Publisher:
ISBN:
Category : Sun
Languages : en
Pages : 194
Book Description
Nuclear Science Abstracts
Author:
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 914
Book Description
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 914
Book Description
Nuclear Science Abstracts
Author:
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 628
Book Description
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 628
Book Description
Scientific and Technical Aerospace Reports
Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 912
Book Description
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 912
Book Description
Observations of the Brightness and Polarization of the Outer Corona During the November 12, 1966, Total Eclipse of the Sun
Author: T. J. Pepin
Publisher:
ISBN:
Category :
Languages : en
Pages : 26
Book Description
Photographs of the solar corona from a camera flown at an altitude of 40,000 feet were obtained on November 12, 1966. The absolute brightness, polarization and the direction of polarization of the solar corona between 3.5 and 13 solar radii were determined from these photographs. A significant polarized component was found in this region, the structure of which can be closely correlated with features in the inner corona. Comparisons are made in the July 20, 1963 and May 30, 1965 eclipses and evidence is given for changes in brightness of the coronal light between these eclipses. (Author).
Publisher:
ISBN:
Category :
Languages : en
Pages : 26
Book Description
Photographs of the solar corona from a camera flown at an altitude of 40,000 feet were obtained on November 12, 1966. The absolute brightness, polarization and the direction of polarization of the solar corona between 3.5 and 13 solar radii were determined from these photographs. A significant polarized component was found in this region, the structure of which can be closely correlated with features in the inner corona. Comparisons are made in the July 20, 1963 and May 30, 1965 eclipses and evidence is given for changes in brightness of the coronal light between these eclipses. (Author).
Comprehensive Dissertation Index, 1861-1972: Astronomy and physics, A-L
Author: Xerox University Microfilms
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 960
Book Description
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 960
Book Description
Comprehensive Dissertation Index
Author:
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 964
Book Description
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 964
Book Description
American Doctoral Dissertations
Author:
Publisher:
ISBN:
Category : Dissertation abstracts
Languages : en
Pages : 490
Book Description
Publisher:
ISBN:
Category : Dissertation abstracts
Languages : en
Pages : 490
Book Description
Infrared Observations of the Outer Solar Corona
Author: Robert M. MacQueen
Publisher:
ISBN:
Category : Infrared astronomy
Languages : en
Pages : 62
Book Description
The 2.2 microns wavelength outer solar corona has been observed in two experiments: first, employing a ground-based telescope during the 93 second totality of the eclipse of 12 November 1966; and second, employing a balloon package with an infrared coronagraph, flown to an altitude of 28 km, during a 5.25 hour period, on 9 January 1967. The design and evaluation of the balloon-borne coronagraph is discussed, and the various origins of stray light investigated. The flight coronagraph was found to introduce a stray radiance of less than 3 x 10 to the -12th power B sub dot, where B sub dot is the radiance of the mean solar disk at 2.2 microns. During eclipse the corona was observed from 2 to 6 solar radii in the ecliptic plane, and at a single point perpendicular to the ecliptic, at 5 solar radii. Balloon observations covered the range 3.7 to 10 solar radii, at position angles from 20 degrees north to 40 degrees south of the ecliptic, on the east limb of the sun. Features attributed to the vaporization of interplanetary material were observed at 3.5, 4, 8.7 and 9.2 solar radii, the former two during the period of totality, and the latter three during the balloon observations. (Author).
Publisher:
ISBN:
Category : Infrared astronomy
Languages : en
Pages : 62
Book Description
The 2.2 microns wavelength outer solar corona has been observed in two experiments: first, employing a ground-based telescope during the 93 second totality of the eclipse of 12 November 1966; and second, employing a balloon package with an infrared coronagraph, flown to an altitude of 28 km, during a 5.25 hour period, on 9 January 1967. The design and evaluation of the balloon-borne coronagraph is discussed, and the various origins of stray light investigated. The flight coronagraph was found to introduce a stray radiance of less than 3 x 10 to the -12th power B sub dot, where B sub dot is the radiance of the mean solar disk at 2.2 microns. During eclipse the corona was observed from 2 to 6 solar radii in the ecliptic plane, and at a single point perpendicular to the ecliptic, at 5 solar radii. Balloon observations covered the range 3.7 to 10 solar radii, at position angles from 20 degrees north to 40 degrees south of the ecliptic, on the east limb of the sun. Features attributed to the vaporization of interplanetary material were observed at 3.5, 4, 8.7 and 9.2 solar radii, the former two during the period of totality, and the latter three during the balloon observations. (Author).