Distribution of the longitudinal component of the magnetic field of prominences from radioastronomical measurements

Standard

Distribution of the longitudinal component of the magnetic field of prominences from radioastronomical measurements. / Nesterov, N. S.; Topchilo, N. A.; Tsyganov, A. N.

In: Radiophysics and Quantum Electronics, Vol. 39, No. 11-12, 01.11.1996, p. 962-966.

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

BibTeX

@article{2ad73aef31164d4a8dcc14bbab190448,

title = "Distribution of the longitudinal component of the magnetic field of prominences from radioastronomical measurements",

abstract = "We present the results of prominence observations at RT-22 CrAO in April, May, and September 1993 at 13.5 mm (intensity and circular polarization) and at 8.2 mm (intensity) wavelengths carried out by circular scanning using the combined scalar horn. On the assumption of thermal cyclotron radiation we have measured the values of the longitudinal component of the magnetic field for 18 prominences. The histogram of the distribution of the longitudinal component indicates the presence of maxima in the vicinity of 8, 15, and 25– 30 G. Our results are compared with the distributions obtained from optical measurements.",

keywords = "Circular Polarization, Magnetic Field, Nonlinear Optic, Quantum Electronics, Radiation",

author = "Nesterov, {N. S.} and Topchilo, {N. A.} and Tsyganov, {A. N.}",

note = "Publisher Copyright: {\textcopyright} 1997 Plenum Publishing Corporation.",

year = "1996",

month = nov,

day = "1",

doi = "10.1007/BF02250973",

language = "English",

volume = "39",

pages = "962--966",

journal = "Radiophysics and Quantum Electronics",

issn = "0033-8443",

publisher = "Springer Nature",

number = "11-12",

}

RIS

TY - JOUR

T1 - Distribution of the longitudinal component of the magnetic field of prominences from radioastronomical measurements

AU - Nesterov, N. S.

AU - Topchilo, N. A.

AU - Tsyganov, A. N.

PY - 1996/11/1

Y1 - 1996/11/1

N2 - We present the results of prominence observations at RT-22 CrAO in April, May, and September 1993 at 13.5 mm (intensity and circular polarization) and at 8.2 mm (intensity) wavelengths carried out by circular scanning using the combined scalar horn. On the assumption of thermal cyclotron radiation we have measured the values of the longitudinal component of the magnetic field for 18 prominences. The histogram of the distribution of the longitudinal component indicates the presence of maxima in the vicinity of 8, 15, and 25– 30 G. Our results are compared with the distributions obtained from optical measurements.

AB - We present the results of prominence observations at RT-22 CrAO in April, May, and September 1993 at 13.5 mm (intensity and circular polarization) and at 8.2 mm (intensity) wavelengths carried out by circular scanning using the combined scalar horn. On the assumption of thermal cyclotron radiation we have measured the values of the longitudinal component of the magnetic field for 18 prominences. The histogram of the distribution of the longitudinal component indicates the presence of maxima in the vicinity of 8, 15, and 25– 30 G. Our results are compared with the distributions obtained from optical measurements.

KW - Circular Polarization

KW - Magnetic Field

KW - Nonlinear Optic

KW - Quantum Electronics

KW - Radiation

UR - http://www.scopus.com/inward/record.url?scp=85051241914&partnerID=8YFLogxK

U2 - 10.1007/BF02250973

DO - 10.1007/BF02250973

M3 - Article

AN - SCOPUS:85051241914

VL - 39

SP - 962

EP - 966

JO - Radiophysics and Quantum Electronics

JF - Radiophysics and Quantum Electronics

SN - 0033-8443

IS - 11-12

ER -

ID: 91674788