Part I Observations of the Brightness and Polarization of the Outer Corona During the November 12, 1966 Total Eclipse of the Sun

Part I Observations of the Brightness and Polarization of the Outer Corona During the November 12, 1966 Total Eclipse of the Sun PDF Author: Theodore John Pepin
Publisher:
ISBN:
Category :
Languages : en
Pages : 194

Get Book Here

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

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 PDF Author: Theodore John Pepin
Publisher:
ISBN:
Category : Sun
Languages : en
Pages : 194

Get Book Here

Book Description


Nuclear Science Abstracts

Nuclear Science Abstracts PDF Author:
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 914

Get Book Here

Book Description


Nuclear Science Abstracts

Nuclear Science Abstracts PDF Author:
Publisher:
ISBN:
Category : Nuclear energy
Languages : en
Pages : 628

Get Book Here

Book Description


Scientific and Technical Aerospace Reports

Scientific and Technical Aerospace Reports PDF Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 912

Get Book Here

Book Description


Observations of the Brightness and Polarization of the Outer Corona During the November 12, 1966, Total Eclipse of the Sun

Observations of the Brightness and Polarization of the Outer Corona During the November 12, 1966, Total Eclipse of the Sun PDF Author: T. J. Pepin
Publisher:
ISBN:
Category :
Languages : en
Pages : 26

Get Book Here

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

Comprehensive Dissertation Index, 1861-1972: Astronomy and physics, A-L PDF Author: Xerox University Microfilms
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 960

Get Book Here

Book Description


Comprehensive Dissertation Index

Comprehensive Dissertation Index PDF Author:
Publisher:
ISBN:
Category : Dissertations, Academic
Languages : en
Pages : 964

Get Book Here

Book Description


American Doctoral Dissertations

American Doctoral Dissertations PDF Author:
Publisher:
ISBN:
Category : Dissertation abstracts
Languages : en
Pages : 490

Get Book Here

Book Description


Infrared Observations of the Outer Solar Corona

Infrared Observations of the Outer Solar Corona PDF Author: Robert M. MacQueen
Publisher:
ISBN:
Category : Infrared astronomy
Languages : en
Pages : 62

Get Book Here

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).