Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths
The single pulse emission from five pulsars (PSR В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16) is detected at frequencies 18ё30 MHz. This radio emission is most probably due to the strong subpulses with peak intensities of 20 and more times larger than those of the average profiles. The inten...
Збережено в:
| Дата: | 2013 |
|---|---|
| Автори: | , , , , , |
| Формат: | Стаття |
| Мова: | rus |
| Опубліковано: |
Видавничий дім «Академперіодика»
2013
|
| Онлайн доступ: | http://rpra-journal.org.ua/index.php/ra/article/view/648 |
| 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 |
oai:ri.kharkov.ua:article-648 |
|---|---|
| record_format |
ojs |
| spelling |
oai:ri.kharkov.ua:article-6482013-02-09T10:44:23Z Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths Обнаружение индивидуальных импульсов пульсаров В0809+74; В0834+06; В0943+10; В0950+08; В1133+16 в декаметровом диапазоне волн Ulyanov, O. M. Zakharenko, V. V. Konovalenko, O. O. Lecacheux, A. Rosolen, C. Rucker, H. O. The single pulse emission from five pulsars (PSR В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16) is detected at frequencies 18ё30 MHz. This radio emission is most probably due to the strong subpulses with peak intensities of 20 and more times larger than those of the average profiles. The intensity of single pulses is strongly frequency- and time-modulated. The detection probability for the anomalously intense pulses is as low as a few percent in the decameter wavelengths. As a rule, such pulses are detected in short series (of no more than 10 pulses). Typical band widths of detected pulses with anomalous intensities lie within 0.2 to 0.5 octave. Обнаружены индивидуальные импульсы излучения пяти пульсаров (PSR В0809+74; В0834+06; В0943+10; В0950+08; В1133+16) на частотах 18ё30 МГц. Это излучение, вероятнее всего, обусловлено наличием мощных субимпульсов, пиковая интенсивность которых в 20 и более раз превышает пиковую интенсивность средних профилей. Интенсивность индивидуальных импульсов сильно промодулирована по частоте и по времени. Вероятность регистрации аномально интенсивных импульсов в декаметровом диапазоне не превышает нескольких процентов. Как правило, такие импульсы регистрируются короткими сериями (не более 10 импульсов). Характерные значения полосы регистрации импульсов, имеющих аномальную интенсивность, находятся в диапазоне 0.2ё0.5 октавы. Видавничий дім «Академперіодика» 2013-02-09 Article Article application/pdf http://rpra-journal.org.ua/index.php/ra/article/view/648 РАДИОФИЗИКА И РАДИОАСТРОНОМИЯ; Vol 11, No 2 (2006); 113 RADIO PHYSICS AND RADIO ASTRONOMY; Vol 11, No 2 (2006); 113 РАДІОФІЗИКА І РАДІОАСТРОНОМІЯ; Vol 11, No 2 (2006); 113 2415-7007 1027-9636 rus http://rpra-journal.org.ua/index.php/ra/article/view/648/199 |
| institution |
Radio physics and radio astronomy |
| collection |
OJS |
| language |
rus |
| format |
Article |
| author |
Ulyanov, O. M. Zakharenko, V. V. Konovalenko, O. O. Lecacheux, A. Rosolen, C. Rucker, H. O. |
| spellingShingle |
Ulyanov, O. M. Zakharenko, V. V. Konovalenko, O. O. Lecacheux, A. Rosolen, C. Rucker, H. O. Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths |
| author_facet |
Ulyanov, O. M. Zakharenko, V. V. Konovalenko, O. O. Lecacheux, A. Rosolen, C. Rucker, H. O. |
| author_sort |
Ulyanov, O. M. |
| title |
Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths |
| title_short |
Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths |
| title_full |
Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths |
| title_fullStr |
Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths |
| title_full_unstemmed |
Detection of Individual Pulses from Pulsars В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16 in the Decameter Wavelengths |
| title_sort |
detection of individual pulses from pulsars в0809+74; в0834+06; в0943+10; в0950+08 and в1133+16 in the decameter wavelengths |
| title_alt |
Обнаружение индивидуальных импульсов пульсаров В0809+74; В0834+06; В0943+10; В0950+08; В1133+16 в декаметровом диапазоне волн |
| description |
The single pulse emission from five pulsars (PSR В0809+74; В0834+06; В0943+10; В0950+08 and В1133+16) is detected at frequencies 18ё30 MHz. This radio emission is most probably due to the strong subpulses with peak intensities of 20 and more times larger than those of the average profiles. The intensity of single pulses is strongly frequency- and time-modulated. The detection probability for the anomalously intense pulses is as low as a few percent in the decameter wavelengths. As a rule, such pulses are detected in short series (of no more than 10 pulses). Typical band widths of detected pulses with anomalous intensities lie within 0.2 to 0.5 octave. |
| publisher |
Видавничий дім «Академперіодика» |
| publishDate |
2013 |
| url |
http://rpra-journal.org.ua/index.php/ra/article/view/648 |
| work_keys_str_mv |
AT ulyanovom detectionofindividualpulsesfrompulsarsv080974v083406v094310v095008andv113316inthedecameterwavelengths AT zakharenkovv detectionofindividualpulsesfrompulsarsv080974v083406v094310v095008andv113316inthedecameterwavelengths AT konovalenkooo detectionofindividualpulsesfrompulsarsv080974v083406v094310v095008andv113316inthedecameterwavelengths AT lecacheuxa detectionofindividualpulsesfrompulsarsv080974v083406v094310v095008andv113316inthedecameterwavelengths AT rosolenc detectionofindividualpulsesfrompulsarsv080974v083406v094310v095008andv113316inthedecameterwavelengths AT ruckerho detectionofindividualpulsesfrompulsarsv080974v083406v094310v095008andv113316inthedecameterwavelengths AT ulyanovom obnaruženieindividualʹnyhimpulʹsovpulʹsarovv080974v083406v094310v095008v113316vdekametrovomdiapazonevoln AT zakharenkovv obnaruženieindividualʹnyhimpulʹsovpulʹsarovv080974v083406v094310v095008v113316vdekametrovomdiapazonevoln AT konovalenkooo obnaruženieindividualʹnyhimpulʹsovpulʹsarovv080974v083406v094310v095008v113316vdekametrovomdiapazonevoln AT lecacheuxa obnaruženieindividualʹnyhimpulʹsovpulʹsarovv080974v083406v094310v095008v113316vdekametrovomdiapazonevoln AT rosolenc obnaruženieindividualʹnyhimpulʹsovpulʹsarovv080974v083406v094310v095008v113316vdekametrovomdiapazonevoln AT ruckerho obnaruženieindividualʹnyhimpulʹsovpulʹsarovv080974v083406v094310v095008v113316vdekametrovomdiapazonevoln |
| first_indexed |
2024-05-26T06:32:04Z |
| last_indexed |
2024-05-26T06:32:04Z |
| _version_ |
1800095792344596480 |