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Prominence Characteristics in 16th Activity Cycle. / Tlatova, K. A.; Nagnibeda, V. G.

In: Geomagnetism and Aeronomy, Vol. 57, No. 7, 01.12.2017, p. 829-834.

Research output: Contribution to journal › Article › peer-review

Harvard

Tlatova, KA & Nagnibeda, VG 2017, 'Prominence Characteristics in 16th Activity Cycle', Geomagnetism and Aeronomy, vol. 57, no. 7, pp. 829-834. https://doi.org/10.1134/S0016793217070234

APA

Tlatova, K. A., & Nagnibeda, V. G. (2017). Prominence Characteristics in 16th Activity Cycle. Geomagnetism and Aeronomy, 57(7), 829-834. https://doi.org/10.1134/S0016793217070234

Vancouver

Tlatova KA, Nagnibeda VG. Prominence Characteristics in 16th Activity Cycle. Geomagnetism and Aeronomy. 2017 Dec 1;57(7):829-834. https://doi.org/10.1134/S0016793217070234

Author

Tlatova, K. A. ; Nagnibeda, V. G. / Prominence Characteristics in 16th Activity Cycle. In: Geomagnetism and Aeronomy. 2017 ; Vol. 57, No. 7. pp. 829-834.

BibTeX

@article{18a7abd0911a495889b9a7d95fba4912,
title = "Prominence Characteristics in 16th Activity Cycle",
abstract = "Digitization of the daily prominence sketches based on data from the global observational network of visual solar spectroscopes was performed for 1922–1934. More than 55000 prominences were distinguished. The results of analysis of distributions by area, height, and prominence location are presented. In addition, the prominence characteristics were compared to those obtained from more recent observations at the Kislovodsk Mountain Astronomical Station of Pulkovo Observatory. The distributions of prominence areas and heights are close to lognormal. The maximal height distribution corresponds to ~25–40 arcsecs. A second maximum also exists for prominence heights of ~70–90 arcsecs.",
author = "Tlatova, {K. A.} and Nagnibeda, {V. G.}",
year = "2017",
month = dec,
day = "1",
doi = "10.1134/S0016793217070234",
language = "English",
volume = "57",
pages = "829--834",
journal = "Geomagnetism and Aeronomy",
issn = "0016-7932",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "7",

}

RIS

TY - JOUR

T1 - Prominence Characteristics in 16th Activity Cycle

AU - Tlatova, K. A.

AU - Nagnibeda, V. G.

PY - 2017/12/1

Y1 - 2017/12/1

N2 - Digitization of the daily prominence sketches based on data from the global observational network of visual solar spectroscopes was performed for 1922–1934. More than 55000 prominences were distinguished. The results of analysis of distributions by area, height, and prominence location are presented. In addition, the prominence characteristics were compared to those obtained from more recent observations at the Kislovodsk Mountain Astronomical Station of Pulkovo Observatory. The distributions of prominence areas and heights are close to lognormal. The maximal height distribution corresponds to ~25–40 arcsecs. A second maximum also exists for prominence heights of ~70–90 arcsecs.

AB - Digitization of the daily prominence sketches based on data from the global observational network of visual solar spectroscopes was performed for 1922–1934. More than 55000 prominences were distinguished. The results of analysis of distributions by area, height, and prominence location are presented. In addition, the prominence characteristics were compared to those obtained from more recent observations at the Kislovodsk Mountain Astronomical Station of Pulkovo Observatory. The distributions of prominence areas and heights are close to lognormal. The maximal height distribution corresponds to ~25–40 arcsecs. A second maximum also exists for prominence heights of ~70–90 arcsecs.

UR - http://www.scopus.com/inward/record.url?scp=85042523284&partnerID=8YFLogxK

U2 - 10.1134/S0016793217070234

DO - 10.1134/S0016793217070234

M3 - Article

AN - SCOPUS:85042523284

VL - 57

SP - 829

EP - 834

JO - Geomagnetism and Aeronomy

JF - Geomagnetism and Aeronomy

SN - 0016-7932

IS - 7

ER -

ID: 47568565