Determination of the Coordinates of Radio Sources on the Sun from RATAN-600 Observations in Multiazimuth Mode
We provide an analytical description of the method for the determination of the coordinates of solar radio sources from multi-azimuth observations on RATAN-600. We analyze models of the displacement of the object across the scan depending as a function of azimuth taking into account solar rotation a...
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Veröffentlicht in: | Astrophysical bulletin 2020-07, Vol.75 (3), p.350-359 |
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creator | Opeikina, L. V. Abramov-Maximov, V. E. Borovik, V. N. Chernenkov, V. N. |
description | We provide an analytical description of the method for the determination of the coordinates of solar radio sources from multi-azimuth observations on RATAN-600. We analyze models of the displacement of the object across the scan depending as a function of azimuth taking into account solar rotation and suggest a method for estimating the rate of displacement due to rotation. We demonstrate the results of the application of the method using the determination of the coordinates of a radio source in the active region NOAA 11 520 as example. After eliminating gross scan referencing errors we obtained the coordinates, which agree well with observational data. We discuss the scan coordinate reference errors. |
doi_str_mv | 10.1134/S1990341320030098 |
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V. ; Abramov-Maximov, V. E. ; Borovik, V. N. ; Chernenkov, V. N.</creator><creatorcontrib>Opeikina, L. V. ; Abramov-Maximov, V. E. ; Borovik, V. N. ; Chernenkov, V. N.</creatorcontrib><description>We provide an analytical description of the method for the determination of the coordinates of solar radio sources from multi-azimuth observations on RATAN-600. We analyze models of the displacement of the object across the scan depending as a function of azimuth taking into account solar rotation and suggest a method for estimating the rate of displacement due to rotation. We demonstrate the results of the application of the method using the determination of the coordinates of a radio source in the active region NOAA 11 520 as example. After eliminating gross scan referencing errors we obtained the coordinates, which agree well with observational data. We discuss the scan coordinate reference errors.</description><identifier>ISSN: 1990-3413</identifier><identifier>EISSN: 1990-3421</identifier><identifier>DOI: 10.1134/S1990341320030098</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Astrophysics and Cosmology ; Azimuth ; Physics ; Physics and Astronomy ; Radio ; Radio sources (astronomy) ; Solar rotation</subject><ispartof>Astrophysical bulletin, 2020-07, Vol.75 (3), p.350-359</ispartof><rights>Pleiades Publishing, Ltd. 2020</rights><rights>Pleiades Publishing, Ltd. 2020.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c268t-b3438a748b500757598ed56119672efdbd7d4f2937c5e2e859976e5554ee10443</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S1990341320030098$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S1990341320030098$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Opeikina, L. 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After eliminating gross scan referencing errors we obtained the coordinates, which agree well with observational data. We discuss the scan coordinate reference errors.</description><subject>Astronomy</subject><subject>Astrophysics and Cosmology</subject><subject>Azimuth</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Radio</subject><subject>Radio sources (astronomy)</subject><subject>Solar rotation</subject><issn>1990-3413</issn><issn>1990-3421</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp1kFtLw0AQhRdRsFZ_gG8LPkdnb0n2sdQrtBaa-hxymdiUZrfuJoL-epNW9EF8muHwnTPDIeSSwTVjQt4kTGsQkgkOIAB0fERGgxQIydnxz87EKTnzfgMQMqHFiDS32KJrapO1tTXUVrRdI51a68pBQz9Iy6ysLU1s54pBMHsm6QytnG3ocrKaPAchAF3kHt37PsnT2tB5t23r7LNuunZN57bEc3JSZVuPF99zTF7u71bTx2C2eHiaTmZBwcO4DXIhRZxFMs4VQKQipWMsVciYDiOOVZmXUSkrrkVUKOQYK62jEJVSEpGBlGJMrg65O2ffOvRtuumfN_3JlEsFknEFYU-xA1U4673DKt25usncR8ogHVpN_7Tae_jB43vWvKL7Tf7f9AXymHc1</recordid><startdate>20200701</startdate><enddate>20200701</enddate><creator>Opeikina, L. 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subjects | Astronomy Astrophysics and Cosmology Azimuth Physics Physics and Astronomy Radio Radio sources (astronomy) Solar rotation |
title | Determination of the Coordinates of Radio Sources on the Sun from RATAN-600 Observations in Multiazimuth Mode |
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