2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS

2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS

The high efficiency of the interplanetary scintillation methodat the decameter wavelengths for detection of coronal mass ejectionsbeyond Earth’s orbit is shown. It is established that coronalmass ejection in the interplanetary medium continuesslowing at distances from 1 to 1.7 AU from the Sun, its v...

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Date:2013
Main Authors: Kalinichenko, N. N., Konovalenko, O. O., Brazhenko, A. I., Solov’ev, V. V.
Format: Article
Language:Russian
Published: Видавничий дім «Академперіодика» 2013
Online Access:http://rpra-journal.org.ua/index.php/ra/article/view/1150
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Journal Title:Radio physics and radio astronomy

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Radio physics and radio astronomy
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spelling rpra-journalorgua-article-11502019-02-19T09:24:03Z 2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS Корональный выброс массы 15 февраля 2011 г. в межпланетном пространстве и его наблюдения методом мерцаний космических источников в декаметровом диапазоне радиоволн Kalinichenko, N. N. Konovalenko, O. O. Brazhenko, A. I. Solov’ev, V. V. The high efficiency of the interplanetary scintillation methodat the decameter wavelengths for detection of coronal mass ejectionsbeyond Earth’s orbit is shown. It is established that coronalmass ejection in the interplanetary medium continuesslowing at distances from 1 to 1.7 AU from the Sun, its velocitytending to that of the ambient solar wind, the angular size beingno less than 66°. Показана высокая эффективность метода межпланетных мерцаний космических источников в декаметровом диапа-зоне радиоволн для обнаружения корональных выбросов массы за орбитой Земли. Установлено, что на расстоя-ниях от Солнца 1÷1.7 а. е. корональный выброс массы в межпланетном пространстве продолжает замедляться,при этом скорость его распространения стремится к скорости окружающего невозмущенного солнечного ветра,а угловой размер составляет не менее 66° . Видавничий дім «Академперіодика» 2013-12-09 Article Article application/pdf http://rpra-journal.org.ua/index.php/ra/article/view/1150 РАДИОФИЗИКА И РАДИОАСТРОНОМИЯ; Vol 18, No 4 (2013); 301 RADIO PHYSICS AND RADIO ASTRONOMY; Vol 18, No 4 (2013); 301 РАДІОФІЗИКА І РАДІОАСТРОНОМІЯ; Vol 18, No 4 (2013); 301 2415-7007 1027-9636 ru http://rpra-journal.org.ua/index.php/ra/article/view/1150/786
institution Radio physics and radio astronomy
baseUrl_str
datestamp_date 2019-02-19T09:24:03Z
collection OJS
language Russian
topic_facet
format Article
author Kalinichenko, N. N.
Konovalenko, O. O.
Brazhenko, A. I.
Solov’ev, V. V.
spellingShingle Kalinichenko, N. N.
Konovalenko, O. O.
Brazhenko, A. I.
Solov’ev, V. V.
2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS
author_facet Kalinichenko, N. N.
Konovalenko, O. O.
Brazhenko, A. I.
Solov’ev, V. V.
author_sort Kalinichenko, N. N.
title 2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS
title_short 2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS
title_full 2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS
title_fullStr 2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS
title_full_unstemmed 2011 FEBRUARY 15 CME IN THE INTERPLANETARY MEDIUM BY OBSERVATIONS OF RADIO SOURCE SCINTILLATIONS AT THE DECAMETER WAVELENGTHS
title_sort 2011 february 15 cme in the interplanetary medium by observations of radio source scintillations at the decameter wavelengths
title_alt Корональный выброс массы 15 февраля 2011 г. в межпланетном пространстве и его наблюдения методом мерцаний космических источников в декаметровом диапазоне радиоволн
description The high efficiency of the interplanetary scintillation methodat the decameter wavelengths for detection of coronal mass ejectionsbeyond Earth’s orbit is shown. It is established that coronalmass ejection in the interplanetary medium continuesslowing at distances from 1 to 1.7 AU from the Sun, its velocitytending to that of the ambient solar wind, the angular size beingno less than 66°.
publisher Видавничий дім «Академперіодика»
publishDate 2013
url http://rpra-journal.org.ua/index.php/ra/article/view/1150
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