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Radio astronomical measurements of magnetic fields in prominences. / Apushkinskii, G. P.; Gunder, K.; Nesterov, N. S.; Strepka, I. D.; Topchilo, N. A.; Tsyganov, A. N.

In: Astronomy Reports, Vol. 40, No. 3, 05.1996, p. 393-396.

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

Harvard

Apushkinskii, GP, Gunder, K, Nesterov, NS, Strepka, ID, Topchilo, NA & Tsyganov, AN 1996, 'Radio astronomical measurements of magnetic fields in prominences', Astronomy Reports, vol. 40, no. 3, pp. 393-396.

APA

Apushkinskii, G. P., Gunder, K., Nesterov, N. S., Strepka, I. D., Topchilo, N. A., & Tsyganov, A. N. (1996). Radio astronomical measurements of magnetic fields in prominences. Astronomy Reports, 40(3), 393-396.

Vancouver

Apushkinskii GP, Gunder K, Nesterov NS, Strepka ID, Topchilo NA, Tsyganov AN. Radio astronomical measurements of magnetic fields in prominences. Astronomy Reports. 1996 May;40(3):393-396.

Author

Apushkinskii, G. P. ; Gunder, K. ; Nesterov, N. S. ; Strepka, I. D. ; Topchilo, N. A. ; Tsyganov, A. N. / Radio astronomical measurements of magnetic fields in prominences. In: Astronomy Reports. 1996 ; Vol. 40, No. 3. pp. 393-396.

BibTeX

@article{fb46de5b909e4773ade10ba25d82801e,
title = "Radio astronomical measurements of magnetic fields in prominences",
abstract = "The brightness distribution and circular polarization in prominences outside the solar disk have been measured at millimeter wavelengths. A lack of coincidence of the maxima in intensity and circular polarization is noted, apparently associated with the orientation of the magnetic field. The intensity of the magnetic fields in prominences is calculated and found to be from 8 to 30 G.",
author = "Apushkinskii, {G. P.} and K. Gunder and Nesterov, {N. S.} and Strepka, {I. D.} and Topchilo, {N. A.} and Tsyganov, {A. N.}",
year = "1996",
month = may,
language = "English",
volume = "40",
pages = "393--396",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

TY - JOUR

T1 - Radio astronomical measurements of magnetic fields in prominences

AU - Apushkinskii, G. P.

AU - Gunder, K.

AU - Nesterov, N. S.

AU - Strepka, I. D.

AU - Topchilo, N. A.

AU - Tsyganov, A. N.

PY - 1996/5

Y1 - 1996/5

N2 - The brightness distribution and circular polarization in prominences outside the solar disk have been measured at millimeter wavelengths. A lack of coincidence of the maxima in intensity and circular polarization is noted, apparently associated with the orientation of the magnetic field. The intensity of the magnetic fields in prominences is calculated and found to be from 8 to 30 G.

AB - The brightness distribution and circular polarization in prominences outside the solar disk have been measured at millimeter wavelengths. A lack of coincidence of the maxima in intensity and circular polarization is noted, apparently associated with the orientation of the magnetic field. The intensity of the magnetic fields in prominences is calculated and found to be from 8 to 30 G.

UR - http://www.scopus.com/inward/record.url?scp=0030500214&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0030500214

VL - 40

SP - 393

EP - 396

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 3

ER -

ID: 91675176