HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS
Purpose: The main most pronounced events, which occurred in the initial period of the pulsars’ study at the decameter wavelength range, are presented. The example of the main scientific problems, which were formulated at the very beginning of pulsar research, shows how the emphasis and priorities of...
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Radio physics and radio astronomy |
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2021-09-27T10:58:17Z |
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aberration frequency band pulse interpulse dispersion measure rotation measure plasma pulsar radio telescope |
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aberration frequency band pulse interpulse dispersion measure rotation measure plasma pulsar radio telescope Ulyanov, O. M. HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS |
topic_facet |
aberration frequency band pulse interpulse dispersion measure rotation measure plasma pulsar radio telescope aberration frequency band pulse interpulse dispersion measure rotation measure plasma pulsar radio telescope аберація діапазон частот імпульс інтерімпульс міра дисперсії міра обертання плазма пульсар радіотелескоп |
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Article |
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Ulyanov, O. M. |
author_facet |
Ulyanov, O. M. |
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Ulyanov, O. M. |
title |
HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS |
title_short |
HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS |
title_full |
HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS |
title_fullStr |
HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS |
title_full_unstemmed |
HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS |
title_sort |
history of low-frequency research of pulsars |
title_alt |
HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS ІСТОРІЯ НИЗЬКОЧАСТОТНИХ ДОСЛІДЖЕНЬ ПУЛЬСАРІВ |
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Purpose: The main most pronounced events, which occurred in the initial period of the pulsars’ study at the decameter wavelength range, are presented. The example of the main scientific problems, which were formulated at the very beginning of pulsar research, shows how the emphasis and priorities of these studies have been changing over time, which tasks have finally been solved, and which are still waiting to be solved. It is shown how the ongoing modernization of the UTR-2 radio telescope have allowed to acquire new qualities in astrophysical research being made with this radio telescope and to identify new scientific directions. The example of the cited references shows how the pulsar research efforts in Ukraine have been developed and how they were integrated into the world astrophysical research of these unique objects.The purpose of this work is to show the relationship between the past and the present on the example of pulsars for longer than a semi-centennial period and to show how the scientific problems that were formulated in the past, and which could not be solved under the then-existing technical conditions, were solved by the subsequent generations of researchers.Design/methodology/approach: The methods of comparison and historical parallels show how the low-frequency studies of pulsars have been developed and evolved almost from their discovery until now.Findings: It is shown how quantitative transformations and technical development, as well as non-standard scientific approaches, unhackneyed thought and international cooperation allow to solve complex radio astronomical problems related to the low-frequency studies of pulsars.Conclusions: The paper provides a historical overview of more than half a century-long radio astronomical studies of pulsars, having been and still being made at the decameter band using the UTR-2 radio telescope. The “old” and current priorities in pulsar research are given, and it is shown how qualitatively the technical parameters of back end facility and computer performance have been changed in studying the coherent pulsar radio emission nature.Key words: aberration; frequency band; pulse; interpulse; dispersion measure; rotation measure; plasma; pulsar; radio telescopeManuscript submitted 17.05.2021Radio phys. radio astron. 2021, 26(2): 130-147REFERENCES1. HEWISH, A., BELL, S. J., PILKINGTON, J. D. H., SCOTT, P. F. and COLLINS, R. A., 1968. Observation of a rapidly pulsating radio source. Nature. vol. 217, no. 5130, pp. 709–713. DOI: https://doi.org/10.1038/217709a02. BRAUDE, S. YA., MEGN, A. V. and SODIN, L. G., 1978. Decameter wavelength radio telescope UTR-2. Antennas. Moscow, Russia: Svyaz’ Publ., no. 26, pp. 3–14. (in Russian).3. MEGN, A. V., SODIN, L. G., SHARYKIN, N. K., BRUCK, YU. M., MEL’YANOVSKY, P. A., INYUTIN, G. A. and GONCHAROV, N. Yu., 1978. 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Видавничий дім «Академперіодика» |
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2021 |
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http://rpra-journal.org.ua/index.php/ra/article/view/1355 |
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oai:ri.kharkov.ua:article-13552021-09-27T10:58:17Z HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS HISTORY OF LOW-FREQUENCY RESEARCH OF PULSARS ІСТОРІЯ НИЗЬКОЧАСТОТНИХ ДОСЛІДЖЕНЬ ПУЛЬСАРІВ Ulyanov, O. M. aberration; frequency band; pulse; interpulse; dispersion measure; rotation measure; plasma; pulsar; radio telescope aberration; frequency band; pulse; interpulse; dispersion measure; rotation measure; plasma; pulsar; radio telescope аберація; діапазон частот; імпульс; інтерімпульс; міра дисперсії; міра обертання; плазма; пульсар; радіотелескоп Purpose: The main most pronounced events, which occurred in the initial period of the pulsars’ study at the decameter wavelength range, are presented. The example of the main scientific problems, which were formulated at the very beginning of pulsar research, shows how the emphasis and priorities of these studies have been changing over time, which tasks have finally been solved, and which are still waiting to be solved. It is shown how the ongoing modernization of the UTR-2 radio telescope have allowed to acquire new qualities in astrophysical research being made with this radio telescope and to identify new scientific directions. The example of the cited references shows how the pulsar research efforts in Ukraine have been developed and how they were integrated into the world astrophysical research of these unique objects.The purpose of this work is to show the relationship between the past and the present on the example of pulsars for longer than a semi-centennial period and to show how the scientific problems that were formulated in the past, and which could not be solved under the then-existing technical conditions, were solved by the subsequent generations of researchers.Design/methodology/approach: The methods of comparison and historical parallels show how the low-frequency studies of pulsars have been developed and evolved almost from their discovery until now.Findings: It is shown how quantitative transformations and technical development, as well as non-standard scientific approaches, unhackneyed thought and international cooperation allow to solve complex radio astronomical problems related to the low-frequency studies of pulsars.Conclusions: The paper provides a historical overview of more than half a century-long radio astronomical studies of pulsars, having been and still being made at the decameter band using the UTR-2 radio telescope. The “old” and current priorities in pulsar research are given, and it is shown how qualitatively the technical parameters of back end facility and computer performance have been changed in studying the coherent pulsar radio emission nature.Key words: aberration; frequency band; pulse; interpulse; dispersion measure; rotation measure; plasma; pulsar; radio telescopeManuscript submitted 17.05.2021Radio phys. radio astron. 2021, 26(2): 130-147REFERENCES1. HEWISH, A., BELL, S. J., PILKINGTON, J. D. H., SCOTT, P. F. and COLLINS, R. A., 1968. Observation of a rapidly pulsating radio source. Nature. vol. 217, no. 5130, pp. 709–713. DOI: https://doi.org/10.1038/217709a02. BRAUDE, S. YA., MEGN, A. V. and SODIN, L. G., 1978. Decameter wavelength radio telescope UTR-2. Antennas. Moscow, Russia: Svyaz’ Publ., no. 26, pp. 3–14. (in Russian).3. MEGN, A. V., SODIN, L. G., SHARYKIN, N. K., BRUCK, YU. M., MEL’YANOVSKY, P. A., INYUTIN, G. A. and GONCHAROV, N. Yu., 1978. Principles of construction and characteristics of antennas of the UTR-2 radio telescope. Antennas. Moscow, Russia: Svyaz’ Publ., no 26. pp. 15–57. (in Russian).4. BRUK, YU. M., 1970. Estimates of radio emission intensity of pulsars CP 0808 and CP 1133 at 25 MHz frequency. Izv. Vyssh. Uchebn. Zaved. Radiofiz. vol. 13, no. 12, pp. 1814–1817. (in Russian). DOI: https://doi.org/10.1007/BF010329905. BRUK, YU. M., 1970. Observation of the Radio Emission of the Pulsar NP 0532 at the Frequency 25 MHz. Izv. Vyssh. Uchebn. Zaved. Radiofiz. vol. 13, no. 12, pp. 1818–1826. (in Russian). DOI: https://doi.org/10.1007/BF010329916. COMELLA, J. M., CRAFT, H. D., LOVELACE, R. V. E., SUTTON, J. M. and TYLER, G. L., 1969. Crab Nebula Pulsar NP0532. Nature. vol. 221, pp. 453–454. DOI: https://doi.org/10.1038/221453a07. CODE, A. D., 1970. The Possible Effects of Scattering of Pulsar Radiation. Astrophys. J. vol. 159, pp. L29–L34. DOI: https://doi.org/10.1086/1804728. STAELIN, D. H. and SUTTON, J. M., 1970. Observed Shapes of Crab Nebula Radio Pulses. Nature. vol. 226, pp. 69–70. DOI: https://doi.org/10.1038/226069a09. POPOV, M. V., KUZ’MIN, A. D., UL’YANOV, O. M., DESHPANDE, A. A., ERSHOV, A. A., ZAKHARENKO, V. V., KONDRAT’EV, V. I., KOSTYUK, S. V., LOSOVSKII, B. YA. and SOGLASNOV, V. A., 2006. Instantaneous Radio Spectra of Giant Pulses from the Crab Pulsar from Decimeter to Decameter Wavelengths Astron. Rep. vol. 50, is. 7, pp. 562–568. DOI: https://doi.org/10.1134/S106377290607006710. ULYANOV, O. M., ZAKHARENKO, V. V., KONOVALENKO, O. O., LECACHEUX, A., ROSOLEN, C. and RUCKER, H. O., 2006. Detection of Individual Pulses from Pulsars B0809+74; B0834+06; B0943+10; B0950+08 and B1133+16 in the Decameter Wavelengths. Radio Phys. Radio Astron. vol. 11, no. 2, pp. 113–133. (in Russian).11. ULYANOV, O. M., DESHPANDE, A., ZAKHARENKO, V. V., ASGEKAR, A. and SHANKAR, U., 2007. Two-Frequency Observations of Six Pulsars Using UTR-2 and GEETEE Radio Telescopes. Radio Phys. 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Y. and PLAKHOV, M. S., 2018. Time and Polarization Radiation Characteristics of PSR J0242+6256 at the Decameter Wavelength Range. Kinemat. Phys. Celest. Bodies. vol. 34, no. 4, pp. 174–183. DOI: https://doi.org/10.3103/S088459131804006216. BRUCK, YU. M. and USTIMENKO, B. YU. 1973. Decametric Pulse Radioemission from PSR 0809, PSR 1133, and PSR 1919. Nat. Phys. Sci. vol. 242, is. 117, pp. 58–59. DOI: https://doi.org/10.1038/physci242058a017. BRUK, YU. M. and USTIMENKO, B. YU., 1973. Methods and apparatus for observation of pulsars in the decameter wavelength range. Izv. Vyssh. Uchebn. Zaved. Radiofiz. vol. 16, pp. 1867–1870. (in Russian). DOI: https://doi.org/10.1007/BF0103704318. BRUK, YU. M. and USTIMENKO, B. YU., 1973. Procedure and Equipment for Observation of Pulsars in the Decameter Range of Wavelengths. Radiophys. and Quantum Electron. vol. 16, is. 12, pp. 1450–1452. DOI: https://doi.org/10.1007/BF0103704319. BRUCK, YU. M. and USTIMENKO, B. YU., 1977. The Interpulse Radio Emission of the Pulsar PSR 191+21 at the Frequencies 16.7–38 MHz. Astrophys. Space Sci. vol. 51, pp. 225–227. DOI: https://doi.org/10.1007/BF0064247420. BRUCK, YU. M. and USTIMENKO, B. YU., 1979. The Interpulse Emission Structure in Pulsars. Astron. Astrophys. vol. 80, pp. 170–173.21. BRUK, YU. M., DAVIES, J. G., KUZ’MIN, A. D., LYNE, A. G., MALOFEEV, V. M., ROWSON, B., USTIMENKO, B. YU. and SHITOV, YU. P., 1978. Radio-emission spectra of five pulsars in the 17–1420 MHz range. Sov. Astron. vol. 22, pp. 588–593.22. NOVIKOV, A. YU., POPOV, M. V., SOGLASNOV, V. A., BRUK, YU. M. and USTIMENKO, B. YU., 1984. Observations of pulsar PSR 0809+74 at a frequency of 25 MHz with a time resolution of 100 msec. Sov. Astron. vol. 28, is. 2, pp. 199–201.23. UL’YANOV, O. M., ZAKHARENKO, V. V. and BRUK, YU. M., 2008. The parameters of pulsar subpulse emission at decameter wavelengths. Astron. Rep. vol. 52, is. 11, pp. 917–924. DOI: https://doi.org/10.1134/S106377290811006124. 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Status, First Results, Multiparametric Pipeline for Candidate Selection. Odessa Astronomical Publications. vol. 28, no. 2, pp. 252–255. DOI: https://doi.org/10.18524/1810-4215.2015.28.7104743. KRAVTSOV, I. P., ZAKHARENKO, V. V., VASYLIEVA, I. Y., MYKHAILOVA, S. S., ULYANOV, O. M., SHEVTSOVA, A. I. and SKORYK, A. O., 2016. Parameters of the transient signals detected in the decameter survey of the Northern sky. Odessa Astronomical Publications. vol. 29, pp. 179–183. DOI: https://doi.org/10.18524/1810-4215.2016.29.8521044. ZAKHARENKO, V. V., NIKOLAENKO, V. S., ULYANOV, O. M. and MOTIYENKO, R. A., 2007. A waveform receiver for continuous registration of fast processes in pulsar radio emission. In: 2007 International Kharkov Symposium Physics and Engrg. of Millimeter and Sub-Millimeter Waves (MSMW). vol. 2, pp. 745–747. DOI: https://doi.org/10.1109/MSMW.2007.429480045. ZAKHARENKO, V. V., NIKOLAENKO, V. S., ULYANOV, O. M. and MOTIYENKO, R. A., 2007. 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V., SHEVTSOVA, A. I., MIROSHNICHENKO, A. P., KUHAI, N. V., SOBOLEV, YA. M. and TSVYK, N. O., 2021. The Founder of the Decameter Radio Astronomy in Ukraine Academician of NAS of Ukraine Semen Yakovych Braude is 110 Years Old: History of Creation and Development of the National Experimental Base for the Last Half Century. Radio Phys. Radio Astron. vol. 26, no. 1, pp. 5–73. (in Ukrainian). DOI: https://doi.org/10.15407/rpra26.01.00548. BRAZHENKO, A. I., BULATSEN, V. G., VASHCHISHIN, R. V., FRANTSUZENKO, A. V., KONOVALENKO, A. A., FALKOVICH, I. S., ABRANIN, E. P., ULYANOV, O. M., ZAKHARENKO, V. V., LECACHEUX, A. and RUCKER, H., 2005. New Decameter Radiopolarimeter URAN-2. Kinematika i fizika nebesnyh tel. vol. 21, no. 5 (suppl.), pp. 43–46.49. SHKURATOV, Y. G., KONOVALENKO, A. A., ZAKHARENKO, V. V., STANISLAVSKY, A. A., BANNIKOVA, E. Y., KAYDASH, V. G., STANKEVICH, D. G., KOROKHIN, V. V., VAVRIV, D. M., GALUSHKO, V. G., YERIN, S. N., BUBNOV, I. N., TOKARSKY, P. L., ULYANOV, O. 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DOI: https://doi.org/10.1016/j.icarus.2012.07.02453. KRAVTSOV, I. P., ZAKHARENKO, V. V., VASYLIEVA, I. Y., MYKHAILOVA, S. S., ULYANOV, O. M., SHEVTSOVA, A. I., SKORYK, A. O., ZARKA, P. and KONOVALENKO, O. O., 2016. Search for Transient Signals in the data of Decameter Survey of the Northern Sky. Adv. Astron. Space Phys. vol. 6, is. 2, pp. 79–84. DOI: https://doi.org/10.17721/2227-1481.6.79-84 Purpose: The main most pronounced events, which occurred in the initial period of the pulsars’ study at the decameter wavelength range, are presented. The example of the main scientific problems, which were formulated at the very beginning of pulsar research, shows how the emphasis and priorities of these studies have been changing over time, which tasks have finally been solved, and which are still waiting to be solved. It is shown how the ongoing modernization of the UTR-2 radio telescope have allowed to acquire new qualities in astrophysical research being made with this radio telescope and to identify new scientific directions. The example of the cited references shows how the pulsar research efforts in Ukraine have been developed and how they were integrated into the world astrophysical research of these unique objects.The purpose of this work is to show the relationship between the past and the present on the example of pulsars for longer than a semi-centennial period and to show how the scientific problems that were formulated in the past, and which could not be solved under the then-existing technical conditions, were solved by the subsequent generations of researchers.Design/methodology/approach: The methods of comparison and historical parallels show how the low-frequency studies of pulsars have been developed and evolved almost from their discovery until now.Findings: It is shown how quantitative transformations and technical development, as well as non-standard scientific approaches, unhackneyed thought and international cooperation allow to solve complex radio astronomical problems related to the low-frequency studies of pulsars.Conclusions: The paper provides a historical overview of more than half a century-long radio astronomical studies of pulsars, having been and still being made at the decameter band using the UTR-2 radio telescope. The “old” and current priorities in pulsar research are given, and it is shown how qualitatively the technical parameters of back end facility and computer performance have been changed in studying the coherent pulsar radio emission nature.Key words: aberration; frequency band; pulse; interpulse; dispersion measure; rotation measure; plasma; pulsar; radio telescopeManuscript submitted 17.05.2021Radio phys. radio astron. 2021, 26(2): 130-147REFERENCES1. HEWISH, A., BELL, S. J., PILKINGTON, J. D. H., SCOTT, P. F. and COLLINS, R. A., 1968. Observation of a rapidly pulsating radio source. Nature. vol. 217, no. 5130, pp. 709–713. DOI: https://doi.org/10.1038/217709a02. BRAUDE, S. YA., MEGN, A. V. and SODIN, L. G., 1978. Decameter wavelength radio telescope UTR-2. Antennas. Moscow, Russia: Svyaz’ Publ., no. 26, pp. 3–14. (in Russian).3. MEGN, A. V., SODIN, L. G., SHARYKIN, N. K., BRUCK, YU. M., MEL’YANOVSKY, P. A., INYUTIN, G. A. and GONCHAROV, N. Yu., 1978. 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DOI: https://doi.org/10.1016/j.icarus.2012.07.02453. KRAVTSOV, I. P., ZAKHARENKO, V. V., VASYLIEVA, I. Y., MYKHAILOVA, S. S., ULYANOV, O. M., SHEVTSOVA, A. I., SKORYK, A. O., ZARKA, P. and KONOVALENKO, O. O., 2016. Search for Transient Signals in the data of Decameter Survey of the Northern Sky. Adv. Astron. Space Phys. vol. 6, is. 2, pp. 79–84. DOI: https://doi.org/10.17721/2227-1481.6.79-84 Предмет i мета роботи: Наведені основні найяскравіші події, які відбувались в початковий період дослідження пульсарів в декаметровому діапазоні. На прикладі головних наукових задач, сформульованих ще на початку цих досліджень, показано, як змінювались акценти та пріоритети досліджень з плином часу, які задачі врешті-решт були вирішені, а які все ще очікують на своє вирішення. Показано, як невпинна модернізація радіотелескопу УТР-2 дозволила набути нових якостей астрофізичним дослідженням, що проводяться на цьому радіотелескопі, та визначити в них нові наукові напрямки. На прикладі цитованих літературних посилань показано, як розвивались дослідження пульсарів в Україні і як вони інтегрувались в світові астрофізичні дослідження цих унікальних об’єктів.Мета цієї роботи – на прикладі дослідження пульсарів показати взаємозв’язок між минулим і сьогоденням на більш ніж півсторічному інтервалі часу та продемонструвати, як ті наукові задачі, що були сформульовані в минулому та які неможливо було розв’язати з тодішніми технічними умовами, були розв’язані наступними поколіннями дослідників.Методи і методологія: Методами порівнянь та історичних паралелей показано, як розвивались та еволюціонували низькочастотні дослідження пульсарів майже від їх відкриття аж дотепер.Результати: Показано, як кількісні перетворення і технічний розвиток, а також нестандартні наукові підходи, оригінальне мислення та міжнародна співпраця дозволяють вирішувати складні радіоастрономічні задачі, пов’язані з низькочастотними дослідженнями пульсарів.Висновки: Наведено історичний огляд понад півсторічних радіоастрономічних досліджень пульсарів, які проводилися та продовжують проводитися в декаметровому діапазоні за допомогою радіотелескопу УТР-2. Висвітлені “старі” та сучасні пріоритети в дослідженнях пульсарів і показано, як якісно змінились технічні параметри приймально-реєструвальної апаратури та комп’ютерні можливості, які були доступні в минулому, та ті, що використовуються зараз для вивчення природи когерентного радіовипромінювання пульсарів.Ключові слова: аберація; діапазон частот; імпульс; інтерімпульс; міра дисперсії; міра обертання; плазма; пульсар; радіотелескопManuscript submitted 17.05.2021Radio phys. radio astron. 2021, 26(2): 130-147СПИСОК ЛІТЕРАТУРИ1. Hewish A., Bell S. J., Pilkington J. D. H., Scott P. F., and Collins R. A. Observation of a rapidly pulsating radio source. Nature. 1968. Vol. 217, No. 5130. P. 709–713. DOI: 10.1038/217709a02. Брауде С. Я., Мень А. В., Содин Л. Г. Радиотелескоп декаметрового диапазона волн УТР-2. Антенны. Москва: Связь, 1978. Вып. 26. С. 3–14.3. Мень А. В., Содин Л. Г., Шарыкин Н. К., Брук Ю. М., Мельяновский П. А., Инютин Г. А., Гончаров Н. Ю. 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DOI: 10.17721/2227-148 Видавничий дім «Академперіодика» 2021-06-22 Article Article application/pdf http://rpra-journal.org.ua/index.php/ra/article/view/1355 10.15407/rpra26.02.130 РАДИОФИЗИКА И РАДИОАСТРОНОМИЯ; Vol 26, No 2 (2021); 130 RADIO PHYSICS AND RADIO ASTRONOMY; Vol 26, No 2 (2021); 130 РАДІОФІЗИКА І РАДІОАСТРОНОМІЯ; Vol 26, No 2 (2021); 130 2415-7007 1027-9636 10.15407/rpra26.02 rus http://rpra-journal.org.ua/index.php/ra/article/view/1355/pdf Copyright (c) 2021 RADIO PHYSICS AND RADIO ASTRONOMY |