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Flare Occurrence Tomorrow as a Function of Area and Flariness of Sunspot Today

Flare Occurrence Tomorrow as a Function of Area and Flariness of Sunspot Today
Author: Alfred E. Reilly
Publisher:
Total Pages: 24
Release: 1969
Genre: Probabilities
ISBN:

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An objective technique has been developed for estimating the probability of occurrence of solar flares in a particular sunspot group using both the size of the sunspot group and its 'flariness'. Tables are given which indicate the probability that at least one flare of importance two or greater will occur tomorrow, given the area and flariness of the sunspot group today. (Author).


Flare Occurrence Tomorrow as a Function of Area and Flariness of Sunspot Today

Flare Occurrence Tomorrow as a Function of Area and Flariness of Sunspot Today
Author: Alfred E. Reilly
Publisher:
Total Pages: 0
Release: 1969
Genre: Probabilities
ISBN:

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An objective technique has been developed for estimating the probability of occurrence of solar flares in a particular sunspot group using both the size of the sunspot group and its 'flariness'. Tables are given which indicate the probability that at least one flare of importance two or greater will occur tomorrow, given the area and flariness of the sunspot group today. (Author)


Solar Flare Occurrence as a Function of Sunspot Size

Solar Flare Occurrence as a Function of Sunspot Size
Author: Isadore Enger
Publisher:
Total Pages: 32
Release: 1966
Genre: Astronomy
ISBN:

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An objective technique has been developed for assessing the probability of occurrence of solar flares in a particular sunspot group, given only the sizes of the sunspot group on two consecutive days. The sunspot data cover the 10-year period 1955 to 1964 and have been published in the Greenwich Photoheliographic Results. The flare data were measured at Sacramento Peak, New Mexico. The flare and spot data were combined by a simple, objective technique which depends only on the size of the spot group and the relative positions of the spot group and flare. These results show the very marked dependence of flare occurrence on the size of the spot group and a significant, but very much smaller, dependence on the change in group size from one day to the next. (Author).


Solar Flare Occurrence as a Function of Sunspot Size

Solar Flare Occurrence as a Function of Sunspot Size
Author:
Publisher:
Total Pages: 25
Release: 1966
Genre:
ISBN:

Download Solar Flare Occurrence as a Function of Sunspot Size Book in PDF, ePub and Kindle

An objective technique has been developed for assessing the probability of occurrence of solar flares in a particular sunspot group, given only the sizes of the sunspot group on two consecutive days. The sunspot data cover the 10-year period 1955 to 1964 and have been published in the Greenwich Photoheliographic Results. The flare data were measured at Sacramento Peak, New Mexico. The flare and spot data were combined by a simple, objective technique which depends only on the size of the spot group and the relative positions of the spot group and flare. These results show the very marked dependence of flare occurrence on the size of the spot group and a significant, but very much smaller, dependence on the change in group size from one day to the next. (Author).


Literature 1970, Part 1

Literature 1970, Part 1
Author: Siegfried Böhme
Publisher: Springer Science & Business Media
Total Pages: 497
Release: 2013-04-18
Genre: Science
ISBN: 3662009595

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Astronomy and Astrophysics Abstracts. which appears in semi-annual volumes, is devoted to the re cording, summarizing and indexing of astronomical publications throughout the world. It is prepared under the auspices of the International Astronomical Union (according to a resolution adopted at the 14th General Assembly in 1970). Astronomy and Astrophysics Abstracts aims to present a comprehensive documentation of literature in all fields of astronomy and astrophysics. Every effort will be made to ensure that the average time interval between the date of receipt of the original literature and publication of the abstracts will not exceed eight months. This time interval is near to that achieved by monthly abstracting journals, com pared to which our system of accumulating abstracts for about six months offers the advantage of greater convenience for the user. Volume 3 contains literature published in 1970 and received before August IS, 1970; some older lite rature which was received late and which is not recorded in earlier volumes is also included.


Solar activity reports

Solar activity reports
Author: Richard Frank Donnelly
Publisher:
Total Pages: 528
Release: 1979
Genre: Cosmic physics
ISBN:

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Nuclear Science Abstracts

Nuclear Science Abstracts
Author:
Publisher:
Total Pages: 516
Release: 1973
Genre: Nuclear energy
ISBN:

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