ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE
Purpose: Compilation of a digital catalog of magnetic storms in the Odesa magnetic anomaly zone in order to find the reasons for possible changes in the radiation fluxes of cosmic radio sources, according to observations at the URAN-4 radio telescope.Design/methodology/approach: Since 1987 until now...
Збережено в:
| Дата: | 2020 |
|---|---|
| Автори: | , , , , , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Видавничий дім «Академперіодика»
2020
|
| Теми: | |
| Онлайн доступ: | http://rpra-journal.org.ua/index.php/ra/article/view/1344 |
| Теги: |
Додати тег
Немає тегів, Будьте першим, хто поставить тег для цього запису!
|
| Назва журналу: | Radio physics and radio astronomy |
Репозитарії
Radio physics and radio astronomy| id |
rpra-journalorgua-article-1344 |
|---|---|
| record_format |
ojs |
| institution |
Radio physics and radio astronomy |
| baseUrl_str |
|
| datestamp_date |
2020-12-07T14:28:43Z |
| collection |
OJS |
| language |
English |
| topic |
solar activity monitoring variability of radio sources magnetic storms catalog of magnetic storms magnetic anomaly |
| spellingShingle |
solar activity monitoring variability of radio sources magnetic storms catalog of magnetic storms magnetic anomaly Sobitnyak, L. I. Ryabov, M. I. Orlyuk, M. I. Sukharev, A. L. Romenets, A. O. Sumaruk, Yu. P. Pilipenko, A. A. ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE |
| topic_facet |
solar activity monitoring variability of radio sources magnetic storms catalog of magnetic storms magnetic anomaly solar activity monitoring variability of radio sources magnetic storms catalog of magnetic storms magnetic anomaly сонячна активність моніторинг мінливості радіоджерел магнітні бурі каталог магнітних бур магнітна аномалія |
| format |
Article |
| author |
Sobitnyak, L. I. Ryabov, M. I. Orlyuk, M. I. Sukharev, A. L. Romenets, A. O. Sumaruk, Yu. P. Pilipenko, A. A. |
| author_facet |
Sobitnyak, L. I. Ryabov, M. I. Orlyuk, M. I. Sukharev, A. L. Romenets, A. O. Sumaruk, Yu. P. Pilipenko, A. A. |
| author_sort |
Sobitnyak, L. I. |
| title |
ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE |
| title_short |
ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE |
| title_full |
ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE |
| title_fullStr |
ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE |
| title_full_unstemmed |
ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE |
| title_sort |
analysis of the magnetic storms catalog for monitoring radio source fluxe data with the uran-4 radio telescope in the odesa magnetic anomaly zone |
| title_alt |
ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE АНАЛІЗ КАТАЛОГУ МАГНІТНИХ БУР ДЛЯ ДАНИХ МОНІТОРИНГУ ПОТОКІВ ВИПРОМІНЮВАННЯ РАДІОДЖЕРЕЛ НА РАДІОТЕЛЕСКОПІ УРАН-4 В ЗОНІ ОДЕСЬКОЇ МАГНІТНОЇ АНОМАЛІЇ |
| description |
Purpose: Compilation of a digital catalog of magnetic storms in the Odesa magnetic anomaly zone in order to find the reasons for possible changes in the radiation fluxes of cosmic radio sources, according to observations at the URAN-4 radio telescope.Design/methodology/approach: Since 1987 until now, the radio flux of powerful galactic and extragalactic radio sources has been monitored at the URAN-4 radio telescope of the Odesa Observatory of the Institute of Radio Astronomy of the National Academy of Sciences of Ukraine. The monitoring program includes radio galaxies 3C274, 3C405 and supernova remnants 3C144, 3C461. Changes in the radio source flux level are determined by the ionosphere state due to the changes in space weather. At the “Odesa” geomagnetic observatory of the Institute of Geophysics of the National Academy of Sciences of Ukraine, the geomagnetic field measurements have been made since 1948. Simultaneously, the measurements of three elements of the geomagnetic field: horizontal component (H), vertical component (Z) and inclination (D), have been recorded.Findings: Using the “Odesa” geomagnetic observatory data, the digital catalog of magnetic storms was compiled for the measuring period of the powerful space radio source fluxes obtained with the URAN-4 radio telescope. For the magnetic storms monitored during the periods of 1987–1995 and 2000–2009, the date and time are shown for the beginning and the end of the magnetic storm, the magnetic storm duration, the amplitude of the three magnetic field elements, being H, Z, and D, and the magnetic storm type characteristic.The “Odesa” geomagnetic observatory is located near the magnetic anomaly zone. To find the distinctions in manifestations of the geomagnetic activity arisen owing to the magnetic anomaly existence, the geomagnetic disturbances recorded at the “Odesa” and “Moscow” (IZMIRAN, Russia) observatories were compared. It was shown that the total annual duration of the magnetic storms was longer in Odesa than in Moscow. This demonstrates some special role of the magnetic anomaly in the development of geomagnetic disturbances.Conclusions: The digital catalog of magnetic storms in the Odesa magnetic anomaly zone was compiled for the 1987–1995 and 2000–2009 periods. It is also planned to terminate working over the complete catalog of magnetic storms recorded at the “Odesa” observatory for the entire continuous period of monitoring space radio sources at the URAN-4 radio telescope in order to find the manifestations of geomagnetic disturbances impact upon the ionosphere state and changes of intensity in cosmic radio source fluxes. These studies are supplemented by the comparative analysis of the “Odesa” observatory geomagnetic data and the data from some other geomagnetic observatories.Key words: solar activity; monitoring variability of radio sources; magnetic storms; catalog of magnetic storms; magnetic anomalyManuscript submitted 19.10.2020Radio phys. radio astron. 2020, 25(4): 324-330REFERENCES1. ORLIUK, M., SUMARUK, YU., SUMARUK, T., ROMENETS, A. and MELNYCHUK, I., 2009. Geomagnetic observatories of the Ukraine: equipment, measurement practice and data interpretation. In: GEODETIC AND GEOPHYSICAL RESEARCH INSTITUTE OF THE HUNGARIANACADEMYOF SCIENCES. The IAGA 11th Scientific Assembly. Sopron, Hungary.2. SOBITNYAK, L. I., RYABOV, M. I., SUKHAREV, A. L., ORLYUK, M. I., ROMENETS, A. O. and SUMARUK, YU. P., 2018. The catalog of magnetic storms for Odessamagnetic anomaly zone. Odessa Astronomical Publications. vol. 31, pp. 163–166. DOI: https://doi.org/10.18524/1810-4215.2018.31.1466623. SOBITNIAK, L. I., RYABOV, M. I., SUKHAREV, A. L. and PANISHKO, S. K., 2017. Structure of Variability Indexes of Cosmic Weather as Applied to Data Monitoring of Fluxes of Radio Sources at the “URAN-4”Radio Telescope. Radio Phys. Radio Astron. vol. 22, no. 4, pp. 294–303. (in Russian). DOI: https://doi.org/10.15407/rpra22.04.2944. RYABOV, M. I., SUKHAREV, A. L., ORLYUK M. I., SOBITNYAK, L. I. and ROMENETS, A. A., 2019. Comparative Analysis of Geomagnetic Disturbances in the OdessaMagnetic Anomaly Area in the 24th Solar Activity Cycle. Radio Phys. Radio Astron. vol. 24, no. 1, pp. 68–79. (in Russian). DOI: https://doi.org/10.15407/rpra24.01.0685. SUKHAREV, A .L., ORLYUK, M. I., RYABOV, M. I. and ROMENETS, A. A., 2018. On the First Results of Measurements of Geomagnetic Short-Period Field Variations in the Odesa Magnetic Anomaly Zone with a Second-Long Resolution. Radio Phys. Radio Astron. vol. 23, no. 2, pp. 116–127. (in Russian). DOI: https://doi.org/10.15407/rpra23.02.116 |
| publisher |
Видавничий дім «Академперіодика» |
| publishDate |
2020 |
| url |
http://rpra-journal.org.ua/index.php/ra/article/view/1344 |
| work_keys_str_mv |
AT sobitnyakli analysisofthemagneticstormscatalogformonitoringradiosourcefluxedatawiththeuran4radiotelescopeintheodesamagneticanomalyzone AT ryabovmi analysisofthemagneticstormscatalogformonitoringradiosourcefluxedatawiththeuran4radiotelescopeintheodesamagneticanomalyzone AT orlyukmi analysisofthemagneticstormscatalogformonitoringradiosourcefluxedatawiththeuran4radiotelescopeintheodesamagneticanomalyzone AT sukhareval analysisofthemagneticstormscatalogformonitoringradiosourcefluxedatawiththeuran4radiotelescopeintheodesamagneticanomalyzone AT romenetsao analysisofthemagneticstormscatalogformonitoringradiosourcefluxedatawiththeuran4radiotelescopeintheodesamagneticanomalyzone AT sumarukyup analysisofthemagneticstormscatalogformonitoringradiosourcefluxedatawiththeuran4radiotelescopeintheodesamagneticanomalyzone AT pilipenkoaa analysisofthemagneticstormscatalogformonitoringradiosourcefluxedatawiththeuran4radiotelescopeintheodesamagneticanomalyzone AT sobitnyakli analízkatalogumagnítnihburdlâdanihmonítoringupotokívvipromínûvannâradíodžerelnaradíoteleskopíuran4vzoníodesʹkoímagnítnoíanomalíí AT ryabovmi analízkatalogumagnítnihburdlâdanihmonítoringupotokívvipromínûvannâradíodžerelnaradíoteleskopíuran4vzoníodesʹkoímagnítnoíanomalíí AT orlyukmi analízkatalogumagnítnihburdlâdanihmonítoringupotokívvipromínûvannâradíodžerelnaradíoteleskopíuran4vzoníodesʹkoímagnítnoíanomalíí AT sukhareval analízkatalogumagnítnihburdlâdanihmonítoringupotokívvipromínûvannâradíodžerelnaradíoteleskopíuran4vzoníodesʹkoímagnítnoíanomalíí AT romenetsao analízkatalogumagnítnihburdlâdanihmonítoringupotokívvipromínûvannâradíodžerelnaradíoteleskopíuran4vzoníodesʹkoímagnítnoíanomalíí AT sumarukyup analízkatalogumagnítnihburdlâdanihmonítoringupotokívvipromínûvannâradíodžerelnaradíoteleskopíuran4vzoníodesʹkoímagnítnoíanomalíí AT pilipenkoaa analízkatalogumagnítnihburdlâdanihmonítoringupotokívvipromínûvannâradíodžerelnaradíoteleskopíuran4vzoníodesʹkoímagnítnoíanomalíí |
| first_indexed |
2025-12-02T15:32:33Z |
| last_indexed |
2025-12-02T15:32:33Z |
| _version_ |
1850836446473093120 |
| spelling |
rpra-journalorgua-article-13442020-12-07T14:28:43Z ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE ANALYSIS OF THE MAGNETIC STORMS CATALOG FOR MONITORING RADIO SOURCE FLUXE DATA WITH THE URAN-4 RADIO TELESCOPE IN THE ODESA MAGNETIC ANOMALY ZONE АНАЛІЗ КАТАЛОГУ МАГНІТНИХ БУР ДЛЯ ДАНИХ МОНІТОРИНГУ ПОТОКІВ ВИПРОМІНЮВАННЯ РАДІОДЖЕРЕЛ НА РАДІОТЕЛЕСКОПІ УРАН-4 В ЗОНІ ОДЕСЬКОЇ МАГНІТНОЇ АНОМАЛІЇ Sobitnyak, L. I. Ryabov, M. I. Orlyuk, M. I. Sukharev, A. L. Romenets, A. O. Sumaruk, Yu. P. Pilipenko, A. A. solar activity; monitoring variability of radio sources; magnetic storms; catalog of magnetic storms; magnetic anomaly solar activity; monitoring variability of radio sources; magnetic storms; catalog of magnetic storms; magnetic anomaly сонячна активність; моніторинг мінливості радіоджерел; магнітні бурі; каталог магнітних бур; магнітна аномалія Purpose: Compilation of a digital catalog of magnetic storms in the Odesa magnetic anomaly zone in order to find the reasons for possible changes in the radiation fluxes of cosmic radio sources, according to observations at the URAN-4 radio telescope.Design/methodology/approach: Since 1987 until now, the radio flux of powerful galactic and extragalactic radio sources has been monitored at the URAN-4 radio telescope of the Odesa Observatory of the Institute of Radio Astronomy of the National Academy of Sciences of Ukraine. The monitoring program includes radio galaxies 3C274, 3C405 and supernova remnants 3C144, 3C461. Changes in the radio source flux level are determined by the ionosphere state due to the changes in space weather. At the “Odesa” geomagnetic observatory of the Institute of Geophysics of the National Academy of Sciences of Ukraine, the geomagnetic field measurements have been made since 1948. Simultaneously, the measurements of three elements of the geomagnetic field: horizontal component (H), vertical component (Z) and inclination (D), have been recorded.Findings: Using the “Odesa” geomagnetic observatory data, the digital catalog of magnetic storms was compiled for the measuring period of the powerful space radio source fluxes obtained with the URAN-4 radio telescope. For the magnetic storms monitored during the periods of 1987–1995 and 2000–2009, the date and time are shown for the beginning and the end of the magnetic storm, the magnetic storm duration, the amplitude of the three magnetic field elements, being H, Z, and D, and the magnetic storm type characteristic.The “Odesa” geomagnetic observatory is located near the magnetic anomaly zone. To find the distinctions in manifestations of the geomagnetic activity arisen owing to the magnetic anomaly existence, the geomagnetic disturbances recorded at the “Odesa” and “Moscow” (IZMIRAN, Russia) observatories were compared. It was shown that the total annual duration of the magnetic storms was longer in Odesa than in Moscow. This demonstrates some special role of the magnetic anomaly in the development of geomagnetic disturbances.Conclusions: The digital catalog of magnetic storms in the Odesa magnetic anomaly zone was compiled for the 1987–1995 and 2000–2009 periods. It is also planned to terminate working over the complete catalog of magnetic storms recorded at the “Odesa” observatory for the entire continuous period of monitoring space radio sources at the URAN-4 radio telescope in order to find the manifestations of geomagnetic disturbances impact upon the ionosphere state and changes of intensity in cosmic radio source fluxes. These studies are supplemented by the comparative analysis of the “Odesa” observatory geomagnetic data and the data from some other geomagnetic observatories.Key words: solar activity; monitoring variability of radio sources; magnetic storms; catalog of magnetic storms; magnetic anomalyManuscript submitted 19.10.2020Radio phys. radio astron. 2020, 25(4): 324-330REFERENCES1. ORLIUK, M., SUMARUK, YU., SUMARUK, T., ROMENETS, A. and MELNYCHUK, I., 2009. Geomagnetic observatories of the Ukraine: equipment, measurement practice and data interpretation. In: GEODETIC AND GEOPHYSICAL RESEARCH INSTITUTE OF THE HUNGARIANACADEMYOF SCIENCES. The IAGA 11th Scientific Assembly. Sopron, Hungary.2. SOBITNYAK, L. I., RYABOV, M. I., SUKHAREV, A. L., ORLYUK, M. I., ROMENETS, A. O. and SUMARUK, YU. P., 2018. The catalog of magnetic storms for Odessamagnetic anomaly zone. Odessa Astronomical Publications. vol. 31, pp. 163–166. DOI: https://doi.org/10.18524/1810-4215.2018.31.1466623. SOBITNIAK, L. I., RYABOV, M. I., SUKHAREV, A. L. and PANISHKO, S. K., 2017. Structure of Variability Indexes of Cosmic Weather as Applied to Data Monitoring of Fluxes of Radio Sources at the “URAN-4”Radio Telescope. Radio Phys. Radio Astron. vol. 22, no. 4, pp. 294–303. (in Russian). DOI: https://doi.org/10.15407/rpra22.04.2944. RYABOV, M. I., SUKHAREV, A. L., ORLYUK M. I., SOBITNYAK, L. I. and ROMENETS, A. A., 2019. Comparative Analysis of Geomagnetic Disturbances in the OdessaMagnetic Anomaly Area in the 24th Solar Activity Cycle. Radio Phys. Radio Astron. vol. 24, no. 1, pp. 68–79. (in Russian). DOI: https://doi.org/10.15407/rpra24.01.0685. SUKHAREV, A .L., ORLYUK, M. I., RYABOV, M. I. and ROMENETS, A. A., 2018. On the First Results of Measurements of Geomagnetic Short-Period Field Variations in the Odesa Magnetic Anomaly Zone with a Second-Long Resolution. Radio Phys. Radio Astron. vol. 23, no. 2, pp. 116–127. (in Russian). DOI: https://doi.org/10.15407/rpra23.02.116 Purpose: Compilation of a digital catalog of magnetic storms in the Odesa magnetic anomaly zone in order to find the reasons for possible changes in the radiation fluxes of cosmic radio sources, according to observations at the URAN-4 radio telescope.Design/methodology/approach: Since 1987 until now, the radio flux of powerful galactic and extragalactic radio sources has been monitored at the URAN-4 radio telescope of the Odesa Observatory of the Institute of Radio Astronomy of the National Academy of Sciences of Ukraine. The monitoring program includes radio galaxies 3C274, 3C405 and supernovaremnants 3C144, 3C461. Changes in the radio source flux level are determined by the ionosphere state due to the changes in space weather. At the “Odesa” geomagnetic observatory of the Institute of Geophysics of the National Academy of Sciences of Ukraine, the geomagnetic field measurements have been made since 1948. Simultaneously, the measurements of three elements of the geomagnetic field: horizontal component (H), vertical component (Z) and inclination (D), have beenrecorded.Findings: Using the “Odesa” geomagnetic observatory data, the digital catalog of magnetic storms was compiled for the measuring period of the powerful space radio source fluxes obtained with the URAN-4 radio telescope. For the magnetic storms monitored during the periods of 1987–1995 and 2000–2009, the date and time are shown for the beginning and the end of the magnetic storm, the magnetic storm duration, the amplitude of the three magnetic field elements, being H, Z, and D, and the magnetic storm type characteristic.The “Odesa” geomagnetic observatory is located near the magnetic anomaly zone. To find the distinctions in manifestations of the geomagnetic activity arisen owing to the magnetic anomaly existence, the geomagnetic disturbances recorded at the “Odesa” and “Moscow” (IZMIRAN, Russia) observatories were compared. It was shown that the total annual duration of the magnetic storms was longer in Odesa than in Moscow. This demonstrates some special role of the magnetic anomaly in the development of geomagnetic disturbances.Conclusions: The digital catalog of magnetic storms in the Odesa magnetic anomaly zone was compiled for the 1987–1995 and 2000–2009 periods. It is also planned to terminate working over the complete catalog of magnetic storms recorded at the “Odesa” observatory for the entire continuous period of monitoring space radio sources at the URAN-4 radio telescope in order to find the manifestations of geomagnetic disturbances impact upon the ionosphere state and changes of intensity in cosmic radio source fluxes. These studies are supplemented by the comparative analysis of the “Odesa” observatory geomagnetic data and the data from some other geomagnetic observatories.Key words: solar activity, monitoring variability of radio sources, magnetic storms, catalog of magnetic storms, magnetic anomalyManuscript submitted 19.10.2020Radio phys. radio astron. 2020, 25(4): 324-330REFERENCES1. ORLIUK, M., SUMARUK, YU., SUMARUK, T., ROMENETS, A. and MELNYCHUK, I., 2009. Geomagnetic observatories of the Ukraine: equipment, measurement practice and data interpretation. In: GEODETIC AND GEOPHYSICAL RESEARCH INSTITUTE OF THE HUNGARIANACADEMYOF SCIENCES. The IAGA 11th Scientific Assembly. Sopron, Hungary.2. SOBITNYAK, L. I., RYABOV, M. I., SUKHAREV, A. L., ORLYUK, M. I., ROMENETS, A. O. and SUMARUK, YU. P., 2018. The catalog of magnetic storms for Odessamagnetic anomaly zone. Odessa Astronomical Publications. vol. 31, pp. 163–166. DOI: 10.18524/1810-4215.2018.31.1466623. SOBITNIAK, L. I., RYABOV, M. I., SUKHAREV, A. L. and PANISHKO, S. K., 2017. Structure of Variability Indexes of Cosmic Weather as Applied to Data Monitoring of Fluxes of Radio Sources at the “URAN-4”Radio Telescope. Radio Phys. Radio Astron. vol. 22, no. 4, pp. 294–303. (in Russian). DOI: 10.15407/rpra22.04.2944. RYABOV, M. I., SUKHAREV, A. L., ORLYUK M. I., SOBITNYAK, L. I. and ROMENETS, A. A., 2019. Comparative Analysis of Geomagnetic Disturbances in the OdessaMagnetic Anomaly Area in the 24th Solar Activity Cycle. Radio Phys. Radio Astron. vol. 24, no. 1, pp. 68–79. (in Russian). DOI: 10.15407/rpra24.01.0685. SUKHAREV, A .L., ORLYUK, M. I., RYABOV, M. I. and ROMENETS, A. A., 2018. On the First Results of Measurements of Geomagnetic Short-Period Field Variations in the Odesa Magnetic Anomaly Zone with a Second-Long Resolution. Radio Phys. Radio Astron. vol. 23, no. 2, pp. 116–127. (in Russian). DOI: 10.15407/rpra23.02.116 Предмет і мета роботи: Складання цифрового каталогу магнітних бур в зоні Одеської магнітної аномалії для виявлення причин зміни рівня потоків випромінювання космічних радіоджерел за даними спостережень на радіотелескопі УРАН-4.Методи і методологія: Від 1987 р. та дотепер на радіотелескопі “УРАН-4” Одеської обсерваторії Радіоастрономічного інституту НАН України виконується моніторинг потоку випромінювання потужних галактичних і позагалактичних радіоджерел. Програма моніторингу включає спостереження радіогалактик 3C274, 3C405 і залишків наднових 3C144, 3C461. Зміни рівня потоків випромінювання радіоджерел визначаються станом іоносфери, обумовленим зміною космічної погоди. З 1948 р. в геомагнітній обсерваторії “Одеса” Інституту геофізики НАН України виконуються вимірювання варіацій магнітного поля Землі. Одночасно реєструються вимірювання трьох елементів магнітного поля: горизонтальна складова (H), вертикальна складова (Z) і схилення (D).Результати: За даними геомагнітної обсерваторії “Одеса” складений цифровий каталог магнітних бур для періодів моніторингу потоків потужних космічних радіоджерел, виконаного на радіотелескопі “УРАН-4”. Для магнітних бур у періоди моніторингу 1987–1995 рр. та 2000–2009 рр. вказані дата і час початку та закінчення магнітної бурі, тривалість магнітної бурі, значення амплітуд трьох елементів магнітного поля, H, Z і D, та характеристика типу магнітної бурі. Геомагнітна обсерваторія “Одеса” розташована поблизу зони магнітної аномалії. Для виявлення відмінностей у проявах геомагнітної активності, що виникають внаслідок існування магнітної аномалії, виконано порівняння геомагнітних збурень, зареєстрованих в обсерваторіях “Одеса” та “Москва” (ІЗМІРАН, Росія). Показано, що сумарна щорічна тривалість магнітних бур в Одесі більша, ніж у Москві. Це демонструє особливу роль магнітної аномалії в розвиткугеомагнітних збурень.Висновок: Створено цифровий каталогу магнітних бур в зоні Одеської магнітної аномалії у періоди 1987–1995 рр., 2000–2009 рр. та планується завершення роботи над повним каталогом магнітних бур, зареєстрованих в обсерваторії “Одеса” упродовж усього безперервного періоду моніторингу космічних радіоджерел на радіотелескопі УРАН-4, з метою виявлення впливу геомагнітної активності на стан іоносфери та зміну рівня потоків випромінювання космічних радіоджерел. Ці дослідження доповнені порівняльниманалізом геомагнітних даних обсерваторії “Одеса” і даних інших геомагнітних обсерваторій.Ключові слова: сонячна активність; моніторинг мінливості радіоджерел; магнітні бурі; каталог магнітних бур; магнітна аномаліяСтаття надійшла до редакції 19.10.2020Radio phys. radio astron. 2020, 25(4): 324-330СПИСОК ЛІТЕРАТУРИ1. ORLIUK, M., SUMARUK, YU., SUMARUK, T., ROMENETS, A. and MELNYCHUK, I., 2009. Geomagnetic observatories of the Ukraine: equipment, measurement practice and data interpretation. In: GEODETIC AND GEOPHYSICAL RESEARCH INSTITUTE OF THE HUNGARIANACADEMYOF SCIENCES. The IAGA 11th Scientific Assembly. Sopron, Hungary.2. SOBITNYAK, L. I., RYABOV, M. I., SUKHAREV, A. L., ORLYUK, M. I., ROMENETS, A. O. and SUMARUK, YU. P., 2018. The catalog of magnetic storms for Odessamagnetic anomaly zone. Odessa Astronomical Publications. vol. 31, pp. 163–166. DOI: 10.18524/1810-4215.2018.31.1466623. SOBITNIAK, L. I., RYABOV, M. I., SUKHAREV, A. L. and PANISHKO, S. K., 2017. Structure of Variability Indexes of Cosmic Weather as Applied to Data Monitoring of Fluxes of Radio Sources at the “URAN-4”Radio Telescope. Radio Phys. Radio Astron. vol. 22, no. 4, pp. 294–303. (in Russian). DOI: 10.15407/rpra22.04.2944. RYABOV, M. I., SUKHAREV, A. L., ORLYUK M. I., SOBITNYAK, L. I. and ROMENETS, A. A., 2019. Comparative Analysis of Geomagnetic Disturbances in the OdessaMagnetic Anomaly Area in the 24th Solar Activity Cycle. Radio Phys. Radio Astron. vol. 24, no. 1, pp. 68–79. (in Russian). DOI: 10.15407/rpra24.01.0685. SUKHAREV, A .L., ORLYUK, M. I., RYABOV, M. I. and ROMENETS, A. A., 2018. On the First Results of Measurements of Geomagnetic Short-Period Field Variations in the Odesa Magnetic Anomaly Zone with a Second-Long Resolution. Radio Phys. Radio Astron. vol. 23, no. 2, pp. 116–127. (in Russian). DOI: 10.15407/rpra23.02.116 Видавничий дім «Академперіодика» 2020-11-30 Article Article application/pdf http://rpra-journal.org.ua/index.php/ra/article/view/1344 10.15407/rpra25.04.324 РАДИОФИЗИКА И РАДИОАСТРОНОМИЯ; Vol 25, No 4 (2020); 324 RADIO PHYSICS AND RADIO ASTRONOMY; Vol 25, No 4 (2020); 324 РАДІОФІЗИКА І РАДІОАСТРОНОМІЯ; Vol 25, No 4 (2020); 324 2415-7007 1027-9636 10.15407/rpra25.04 en http://rpra-journal.org.ua/index.php/ra/article/view/1344/pdf Copyright (c) 2020 RADIO PHYSICS AND RADIO ASTRONOMY |