GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES

GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES

Subject and Purpose. The sporadic radio emissions coming from the Sun in a broad frequency range contain a lot of important information concerning the solar corona, parameters of the radio frequency sources therein, and the parameter variations resulting from active processes on and about the Sun. T...

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Дата:2023
Автори: Dorovsky, V. V., Melnik, V. M., Brazhenko, A. I.
Формат: Стаття
Мова:Ukrainian
Опубліковано: Видавничий дім «Академперіодика» 2023
Теми:
the Sun; UTR-2 radio telescope; space probe PSP; ground-based support; spectral density; power flux
calibration
Онлайн доступ:http://rpra-journal.org.ua/index.php/ra/article/view/1411
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Назва журналу:Radio physics and radio astronomy

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Radio physics and radio astronomy
id rpra-journalorgua-article-1411
record_format ojs
institution Radio physics and radio astronomy
baseUrl_str
datestamp_date 2023-06-23T06:09:43Z
collection OJS
language Ukrainian
topic the Sun; UTR-2 radio telescope; space probe PSP; ground-based support; spectral density; power flux
calibration
spellingShingle the Sun; UTR-2 radio telescope; space probe PSP; ground-based support; spectral density; power flux
calibration
Dorovsky, V. V.
Melnik, V. M.
Brazhenko, A. I.
GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES
topic_facet the Sun; UTR-2 radio telescope; space probe PSP; ground-based support; spectral density; power flux
calibration
радіотелескоп УТР-2
космічний зонд PSP
наземна підтримка
спектральна густина
потік
калібрування
format Article
author Dorovsky, V. V.
Melnik, V. M.
Brazhenko, A. I.
author_facet Dorovsky, V. V.
Melnik, V. M.
Brazhenko, A. I.
author_sort Dorovsky, V. V.
title GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES
title_short GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES
title_full GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES
title_fullStr GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES
title_full_unstemmed GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES
title_sort ground based support of the space mission parker performed with ukrainian low frequency radio telescopes
title_alt НАЗЕМНА ПІДТРИМКА КОСМІЧНОЇ МІСІЇ PARKER УКРАЇНСЬКИМИ НИЗЬКОЧАСТОТНИМИ РАДІОТЕЛЕСКОПАМИ
description Subject and Purpose. The sporadic radio emissions coming from the Sun in a broad frequency range contain a lot of important information concerning the solar corona, parameters of the radio frequency sources therein, and the parameter variations resulting from active processes on and about the Sun. These have been the reasons for recent launches of the space missions intended for stud- ying the Sun and its corona, such as the Parker Solar Probe (PSP) and the Solar Orbiter. The present work is aimed at demonstrating effectiveness of the ground-based support for the space missions, the PSP before all, which is provided by the large Ukrainian radio telescopes of the decameter wavelength range. Another purpose has been cross-calibration of the space-borne radiometer against calibrated data from a ground-based instrument.Methods and Methodology. One of the remote diagnosis techniques widely used with respect to the solar corona is to analyze parameters of the radio frequency emissions from sources lying at a variety of altitudes within the corona. The methodology of such joint, space-borne/terrestrial investigations suggests simultaneous observations of certain individual events during closest approach of the space probe PSP to the Sun, with analysis over a widest possible frequency range. The data obtainable within overlapping fre- quency bands are proposed for calibrating the on-board radio receivers of the space probe.Results. The methodology proposed for joint, space-based / terrestrial observations has been substantiated. Data from the UTR-2 and URAN-2 radio telescopes and the space probe PSP have been used to plot the dynamic and the polarization spectra of the June 9, 2020 solar bursts, with identification and comparison of the relevant individual events. A joint dynamic spectrum of these bursts has been obtained for the frequency band of 0.5 to 32 MHz. The calibrated data from the ground-based radio telescopes have allowed performing cross-calibration of the HF receiver in the FIELDS-PSP data taking module within the frequency band of 10 to 18 MHz.Conclusions. The paper has provided evidence of an effective ground-based support for the space mission PSP on the part of large Ukrainian radio telescopes. Examples of joint observations have been given, and a methodology described which is employed for cross-calibrating the HF receivers of the FIELD-PSP module. Prospects are outlined of further ground-based support for solar space research missions.Keywords: the Sun; UTR-2 radio telescope, space probe PSP,  ground-based support, spectral density, power flux, calibrationManuscript submitted 02.03.2023Radio phys. radio astron. 2023, 28(2): 117-129REFERENCES1. 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Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Seggauberg near Graz, Austria, 25—27 Oct. 2016. Vienna: Austrian Academy of Sciences Press, pp. 467—478. DOI: https://doi.org/10.1553/PRE8s4674. Bougeret, J.L., Goetz, K., Kaiser, M.L., Bale, S.D., Kellogg, P.J., Maksimovic, M., Monge, N., Monson, S.J., Astier, P.L., Davy, S., Dekkali, M., Hinze, J.J., Manning, R.E., Aguilar-Rodriguez, E., Bonnin, X., Briand, C., Cairns, I.H., Cattell, C.A., Cecconi, B., Eastwood, J., Ergun, R.E., Fainberg, J., Hoang, S., Huttunen, K.E.J., Krucker, S., Lecacheux, A., MacDowall, R.J., Mache, W., Mangeney, A., Meetre, C.A., Moussas, X., Nguyen, Q.N., Oswald, T.H., Pulupa, M., Reiner, M.J., Robinson, P.A., Rucker, H., Salem, C., Santolik, O., Silvis, J.M., Ullrich, R., Zarka, P. & Zouganelis, I., 2008. S/WAVES: The Radioand Plasma Wave Investigation on the STEREO Mission. Space Sci. Rev., 136(1—4), pp. 487—528. DOI: https://doi.org/10.1007/s11214-007-9298-85. Konovalenko, A.A.,Stanislavsky, A.A.,Rucker, H.O., Lecacheux, A., Mann, G., Bougeret, J.L., Kaiser, M.L., Briand, C., Zarka, P., Abranin, E.P., Dorovsky, V.V., Koval, A.A., Mel’nik, V.N., Mukha, D.V., Panchenko, M., 2013. Synchronized observations by using the STEREO and the largest ground-based decametre radio telescope. Exp. Astron., 36(1—2), pp. 137—154. DOI: https://doi.org/10.1007/s10686-012-9326-x6. Cecconi, B., Bonnin, X., Hoang, S., Maksimovic, M., Bale, S.D., Bougeret, J.-L., Goetz, K., Lecacheux, A., Reiner, M.J., Rucker, H.O., Zarka, P., 2008. STEREO/Waves Goniopolarimetry. Space Sci. Rev., 136, pp. 549—563. DOI: https://doi.org/10.1007/s11214-007-9255-67. Abranin, E.P., Stanislavsky, A.A., Koval, A.A., Konovalenko, A.A., 2011. Heliograph of the UTR-2 Radio Telescope. II. Design Features. Radio Phys. Radio Astron., 2(4), pp. 299—305. DOI: https://doi.org/10.1615/RadioPhysicsRadioAstronomy.v2.i4.208. Dorovskyy, V.V., Melnik, V.N., Konovalenko, A.A., Brazhenko, A.I., Panchenko, M., Poedts, S., Mykhaylov, V.A., 2015. Fine and Superfine Structure of the Decameter-Hectometer Type II Burst on 7 June 2011. Sol. Phys., 290(7), pp. 2031—2042. DOI: https://doi.org/10.1007/s11207-015-0725-99. Bale, S.D., Goetz, K., Harvey, P.R., Turin, P., Bonnell, J.W., Dudok de Wit, T., Ergun, R.E., MacDowall, R.J., Pulupa, M., Andre, M., Bolton, M., Bougeret, J.L., Bowen, T.A., Burgess, D., Cattell, C.A., Chandran, B.D.G., Chaston, C.C., Chen, C.H.K., Choi, M.K., Connerney, J.E., Cranmer, S., Diaz-Aguado, M., Donakowski, W., Drake, J.F., Farrell, W.M., Fergeau, P., Fermin, J., Fischer, J., Fox, N., Glaser, D., Goldstein, M., Gordon, D., Hanson, E., Harris, S.E., Hayes, L.M., Hinze, J.J., Hollweg, J.V., Horbury, T.S., Howard, R.A., Hoxie, V., Jannet, G., Karlsson, M., Kasper, J.C., Kellogg, P.J., Kien, M., Klimchuk, J.A., Krasnoselskikh, V.V., Krucker, S., Lynch, J.J., Maksimovic, M., Malaspina, D.M., Marker, S., Martin, P., Martinez-Oliveros, J., McCauley, J., McComas, D.J., McDonald, T., Meyer-Vernet, N., Moncuquet, M., Monson, S.J., Mozer, F.S., Murphy, S.D., Odom, J., Oliverson, R., Olson, J., Parker, E.N., Pankow, D., Phan, T., Quataert, E., Quinn, T., Ruplin, S.W., Salem, C., Seitz, D., Sheppard, D.A., Siy, A., Stevens, K., Summers, D., Szabo, A., Timofeeva, M., Vaivads, A., Velli, M., Yehle, A., Werthimer, D., Wygant, J.R., 2016. 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Melnik, V.N., Brazhenko, A.I., Konovalenko, A.A., Frantsuzenko, A.V., Yerin, S.M., Dorovskyy, V.V., Bubnov, I.M., 2021. Properties of Type III and Type IIIb Bursts in the Frequency Band of 8—80 MHz During PSP Perihelion at the Beginning of April 2019. Sol. Phys., 296(1), id. 9. DOI:https://doi.org/10.1007/s11207-020-01754-514. Stanislavsky, A.A., Bubnov, I.N., Koval, A.A., Yerin, S.N., 2022. Parker Solar Probe detects solar radio bursts related with a behind- the-limb active region. Astron. Astrophys., 657, id. A21, 10 pp. DOI: https://doi.org/10.1051/0004-6361/20214198415. 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Melnik, V.N., Konovalenko, A.A., Rucker, H.O., Boiko, A.I., Dorovsky, V.V., Abranin, E.P., Lecacheux, A., 2011. Observations of Powerful Type III Bursts in the Frequency Range 10–30 MHz. Sol. Phys., 269(2), pp. 335—350. DOI: https://doi.org/10.1007/s11207-010-9703-417. Dulk, G.A., Erickson, W.C., Manning, R., Bougeret, J.-L., 2001. Calibration of low-frequency radio telescopes using the galactic background radiation. Astron. Astrophys., 365, pp. 294—300. DOI: https://doi.org/10.1051/0004-6361:20000006
publisher Видавничий дім «Академперіодика»
publishDate 2023
url http://rpra-journal.org.ua/index.php/ra/article/view/1411
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spelling rpra-journalorgua-article-14112023-06-23T06:09:43Z GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES НАЗЕМНА ПІДТРИМКА КОСМІЧНОЇ МІСІЇ PARKER УКРАЇНСЬКИМИ НИЗЬКОЧАСТОТНИМИ РАДІОТЕЛЕСКОПАМИ Dorovsky, V. V. Melnik, V. M. Brazhenko, A. I. the Sun; UTR-2 radio telescope; space probe PSP; ground-based support; spectral density; power flux, calibration радіотелескоп УТР-2; космічний зонд PSP; наземна підтримка; спектральна густина; потік; калібрування Subject and Purpose. The sporadic radio emissions coming from the Sun in a broad frequency range contain a lot of important information concerning the solar corona, parameters of the radio frequency sources therein, and the parameter variations resulting from active processes on and about the Sun. These have been the reasons for recent launches of the space missions intended for stud- ying the Sun and its corona, such as the Parker Solar Probe (PSP) and the Solar Orbiter. The present work is aimed at demonstrating effectiveness of the ground-based support for the space missions, the PSP before all, which is provided by the large Ukrainian radio telescopes of the decameter wavelength range. Another purpose has been cross-calibration of the space-borne radiometer against calibrated data from a ground-based instrument.Methods and Methodology. One of the remote diagnosis techniques widely used with respect to the solar corona is to analyze parameters of the radio frequency emissions from sources lying at a variety of altitudes within the corona. The methodology of such joint, space-borne/terrestrial investigations suggests simultaneous observations of certain individual events during closest approach of the space probe PSP to the Sun, with analysis over a widest possible frequency range. The data obtainable within overlapping fre- quency bands are proposed for calibrating the on-board radio receivers of the space probe.Results. The methodology proposed for joint, space-based / terrestrial observations has been substantiated. Data from the UTR-2 and URAN-2 radio telescopes and the space probe PSP have been used to plot the dynamic and the polarization spectra of the June 9, 2020 solar bursts, with identification and comparison of the relevant individual events. A joint dynamic spectrum of these bursts has been obtained for the frequency band of 0.5 to 32 MHz. The calibrated data from the ground-based radio telescopes have allowed performing cross-calibration of the HF receiver in the FIELDS-PSP data taking module within the frequency band of 10 to 18 MHz.Conclusions. The paper has provided evidence of an effective ground-based support for the space mission PSP on the part of large Ukrainian radio telescopes. Examples of joint observations have been given, and a methodology described which is employed for cross-calibrating the HF receivers of the FIELD-PSP module. Prospects are outlined of further ground-based support for solar space research missions.Keywords: the Sun; UTR-2 radio telescope, space probe PSP,  ground-based support, spectral density, power flux, calibrationManuscript submitted 02.03.2023Radio phys. radio astron. 2023, 28(2): 117-129REFERENCES1. Brazhenko, A., Vashchishin, R., Pylaev, O., Koshovyy, V., Lozinsky, A., Ivantyshin, O., Rucker, H.O., Panchenko, M., Fischer, G., Lecacheux, A., Denis, L., Coffre, A., Grieβmeier, J.-M., Tagger, M., Girard, J., Charrier, D., Briand, C. & Mann, G., 2016. The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT. Exp. Astron., 42(1), pp. 11—48. DOI: https://doi.org/10.1007/s10686-016-9498-x2. Konovalenko, A.A., Yerin, S.M., Bubnov, I.M., Tokarsky, P.L., Zakharenko, V.V., Ulyanov, O.M., Sidorchuk, M.A., Stepkin, S.V., Gridin, A.O., Kvasov, G.V., Koliadin, V.L., Melnik, V.M., Dorovskyy, V.V., Kalinichenko, M.M., Litvinenko, G.V., Zarka, P., Denis, L., Girard, J., Rucker, H.O., Panchenko, M., Stanislavsky, A.A., Khristenko, O.D., Mukha, D.V., Reznichenko, O.M., Lisachenko, V.M., Bortsov, V.V., Brazhenko, A.I., Vasylieva, I.Y., Skoryk, A.O., Shevtsova, A.I., Mylostna, K.Y., 2016. Astrophysical Studies with Small Low-Frequency Radio Telescopes of New Generation. Radio Phys. Radio Astron., 21(2), pp. 83—131 (in Russian). DOI: https://doi.org/10.15407/rpra21.02.0833. Konovalenko, A., Zarka, P., Rucker, H.O., Zakharenko, V., Ulyanov, O., Sidorchuk, M., Stepkin, S., Melnik, V., Kalinichenko, N., Stanislavsky, A., Tokarsky, P., Koliadin, V., Shepelev, V., Dorovskyy, V., Bubnov, I., Yerin, S., Reznichenko, A., Litvinenko, G., Shevchuk, N., Koval, A., Vasylieva, I., Mylostna, K., Skoryk, A., Shevtsova, A., Volvach, Y., Vasylkovsky, E., Ryabov, V., Lecacheux, A., Denis, L., Panchenko, M., Fischer, G., Imai, M., Griessmeier, J.-M., Mann, G., Litvinenko, O., Brazhenko, A., Vashchishin, R., Frantsuzenko, A., Koshovy, V., Lozinsky, A., Ivantyshin, O., 2016 Multi-antenna observerations in the low-frequency radio astronomy of solar system objects and related topics studies. In: G. Fischer, G. Mann, M. Panchenko, and P. Zarka, eds. Planetary Radio Emissions VIII. Proc. 8th Int. Workshop on Planetary, Solar and Heliospheric Radio Emissions held at Seggauberg near Graz, Austria, 25—27 Oct. 2016. Vienna: Austrian Academy of Sciences Press, pp. 467—478. 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Метою цієї роботи є демонстрація ефективності наземної підтримки космічних місій, перш за все PSP, за допомогою великих українських радіотелескопів декаметрового діапазону. Ще однією метою роботи є проведення крос-калібрування радіометра космічної місії за каліброваними даними наземного радіотелескопа.Методи та методологія. Одним із найпоширеніших методів дистанційної діагностики властивостей  сонячної корони є вивчення параметрів радіовипромінювання, джерела якого знаходяться в короні Сонця на різних геліовисотах. Методика спільних наземно-космічних спостережень полягає в одночасному спостереженні окремих подій та їхньому аналізі в максимально широкій смузі частот під час максимального наближення апарата PSP до Сонця. При цьому спостереження в спіль- ній смузі частот пропонується використовувати для калібрування бортових радіоприймачів.Результати. Обґрунтовано методику планування спільних наземно-космічних спостережень. За даними радіотелеско- пів УТР-2, УРАН-2 і зонда PSP отримано динамічні та поляризаційні спектри сплесків 9 червня 2020 року, проведено ідентифікацію та співставлення окремих сплесків. Одержано спільний динамічний спектр сплесків у смузі частот 0.5…32 МГц. За допомогою каліброваних даних наземних радіотелескопів проведено крос-калібрування приймача HFR модуля FIELDS-PSP у смузі частот 10…18 МГц.Висновки. Показано ефективність наземної підтримки місії PSP за допомогою великих українських радіотелескопів, наведено приклади спільних спостережень, продемонстровано методику крос-калібрування приймачів модуля FIELD-PSP. Наведено перспективи подальшої наземної підтримки сонячних космічних місій.Ключові слова: радіотелескоп УТР-2, космічний зонд PSP, наземна підтримка, спектральна густина, потік, калібруванняСтаття надійшла до редакції 02.03.2023Radio phys. radio astron. 2023, 28(2): 117-129БІБЛІОГРАФІЧНИЙ СПИСОК    1. 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