On the influence of the Sun on the rapid variability of compact extragalactic sources
Since December 2004, we have performed a program to monitor intraday variable sources at a frequency of 5 GHz at the Urumqi Observatory. We present our analysis of the variability characteristics of the flat-spectrum radio source AO 0235+164, which detects an annual cycle in the variability amplitud...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2011-06, Vol.530, p.A129 |
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container_start_page | A129 |
container_title | Astronomy and astrophysics (Berlin) |
container_volume | 530 |
creator | Marchili, N. Krichbaum, T. P. Liu, X. Song, H.-G. Anderson, J. M. Witzel, A. Zensus, J. A. |
description | Since December 2004, we have performed a program to monitor intraday variable sources at a frequency of 5 GHz at the Urumqi Observatory. We present our analysis of the variability characteristics of the flat-spectrum radio source AO 0235+164, which detects an annual cycle in the variability amplitude. This appears to correlate with the solar elongation of the source. A thorough analysis of the results of the MASIV IDV survey – which provides the variability characteristics of a large sample of compact radio sources – confirms that there is a small but detectable component of the observed fractional modulation that increases with decreasing solar elongation. We discuss the hypothesis that the phenomenon is related to interplanetary scintillation. |
doi_str_mv | 10.1051/0004-6361/201016033 |
format | Article |
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P. ; Liu, X. ; Song, H.-G. ; Anderson, J. M. ; Witzel, A. ; Zensus, J. A.</creator><creatorcontrib>Marchili, N. ; Krichbaum, T. P. ; Liu, X. ; Song, H.-G. ; Anderson, J. M. ; Witzel, A. ; Zensus, J. A.</creatorcontrib><description>Since December 2004, we have performed a program to monitor intraday variable sources at a frequency of 5 GHz at the Urumqi Observatory. We present our analysis of the variability characteristics of the flat-spectrum radio source AO 0235+164, which detects an annual cycle in the variability amplitude. This appears to correlate with the solar elongation of the source. A thorough analysis of the results of the MASIV IDV survey – which provides the variability characteristics of a large sample of compact radio sources – confirms that there is a small but detectable component of the observed fractional modulation that increases with decreasing solar elongation. 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A thorough analysis of the results of the MASIV IDV survey – which provides the variability characteristics of a large sample of compact radio sources – confirms that there is a small but detectable component of the observed fractional modulation that increases with decreasing solar elongation. We discuss the hypothesis that the phenomenon is related to interplanetary scintillation.</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>quasars: individual: AO 0235+164</subject><subject>radio continuum: general</subject><subject>scattering</subject><subject>solar wind</subject><subject>surveys</subject><issn>0004-6361</issn><issn>1432-0746</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNo9kEtLw0AUhQdRsFZ_gZtsXMbOIzOTLKVqFQoKbRHcDLc3MzqaJmEmlfbfm1jp6j7Ody6cS8g1o7eMSjahlGapEopNOGWUKSrECRmxTPCU6kydktGROCcXMX71I2e5GJHVS510nzbxtau2tkabNO5vsdjWSXPQArS-TH4geFj7ynf7gcFm0wJ2id11AT6g6nuPSWy2AW28JGcOqmiv_uuYrB4fltOndP4ye57ezVMUinepdnmpHNfaSSytQmQZcid1UTJZWA6Istcp51DmTpcZSAW5WhcFCmkF02JMxOEuhibGYJ1pg99A2BtGzfAZM-Q2Q25z_Ezvujm4WogIlQtQo49HK8-klnlBey49cD52dnfUIXwbpYWWJqdvZrko7uXi9d3MxC_yEHL0</recordid><startdate>20110601</startdate><enddate>20110601</enddate><creator>Marchili, N.</creator><creator>Krichbaum, T. 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source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; EZB-FREE-00999 freely available EZB journals |
subjects | Astronomy Earth, ocean, space Exact sciences and technology quasars: individual: AO 0235+164 radio continuum: general scattering solar wind surveys |
title | On the influence of the Sun on the rapid variability of compact extragalactic sources |
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