FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2506577675> ?p ?o ?g. }

• W2506577675 endingPage "A80" @default.
• W2506577675 startingPage "A80" @default.
• W2506577675 abstract "We studied the characteristic physical properties and behavior of broadband microwave sub-second pulsations observed in an expanding coronal loop during the GOES C2.4 solar flare on 2011 August 10. We found sub-second pulsations and other different burst groups in the complex radio spectrum. The broadband (bandwidth about 1 GHz) sub-second pulsations (temporal period range 0.07-1.49 s, no characteristic dominant period) lasted 70 s in the frequency range 4-7 GHz. These pulsations were not correlated at their individual frequencies, had no measurable frequency drift, and zero polarization. In these pulsations, we found the signatures of fast sausage magnetoacoustic waves with the characteristic periods of 0.7 and 2 s. The other radio bursts showed their characteristic frequency drifts in the range of -262-520 MHz/s. They helped us to derive average values of 20-80 G for the coronal magnetic field strength in the place of radio emission. It was revealed that the microwave event belongs to an expanding coronal loop with twisted sub-structures observed in the 131, 94, and 193 A SDO/AIA channels. Their slit-time diagrams were compared with the location of the radio source at 5.7 GHz to realize that the EUV intensity of the expanding loop increased just before the radio source triggering. We reveal two EUV bidirectional flows that are linked with the start time of the loop expansion. Their positions were close to the radio source and propagated with velocities within a range of 30-117 km/s. We demonstrate that periodic regime of the electron acceleration in a model of the quasi-periodic magnetic reconnection might be able to explain physical properties and behavior of the sub-second pulsations. The depolarization process of the microwave emission might be caused by a plasma turbulence in the radio source. Finally, the observed EUV flows might be linked with reconnection outflows." @default.
• W2506577675 created "2016-08-23" @default.
• W2506577675 creator A5019460672 @default.
• W2506577675 creator A5032226441 @default.
• W2506577675 creator A5036076449 @default.
• W2506577675 creator A5049796911 @default.
• W2506577675 creator A5054287990 @default.
• W2506577675 creator A5068190184 @default.
• W2506577675 date "2016-09-01" @default.
• W2506577675 modified "2023-09-27" @default.
• W2506577675 title "Broadband microwave sub-second pulsations in an expanding coronal loop of the 2011 August 10 flare" @default.
• W2506577675 cites W1544323195 @default.
• W2506577675 cites W1570260105 @default.
• W2506577675 cites W1660416739 @default.
• W2506577675 cites W1678742593 @default.
• W2506577675 cites W1971322579 @default.
• W2506577675 cites W1972733634 @default.
• W2506577675 cites W1977231776 @default.
• W2506577675 cites W1985017729 @default.
• W2506577675 cites W1987020992 @default.
• W2506577675 cites W1993664025 @default.
• W2506577675 cites W2004790048 @default.
• W2506577675 cites W2007244123 @default.
• W2506577675 cites W2010304464 @default.
• W2506577675 cites W2023737430 @default.
• W2506577675 cites W2024055743 @default.
• W2506577675 cites W2034139177 @default.
• W2506577675 cites W2042084996 @default.
• W2506577675 cites W2058192047 @default.
• W2506577675 cites W2062988435 @default.
• W2506577675 cites W2069578804 @default.
• W2506577675 cites W2075540573 @default.
• W2506577675 cites W2076361606 @default.
• W2506577675 cites W2078411911 @default.
• W2506577675 cites W207884016 @default.
• W2506577675 cites W2080236199 @default.
• W2506577675 cites W2085965421 @default.
• W2506577675 cites W2087710337 @default.
• W2506577675 cites W2087806343 @default.
• W2506577675 cites W2093801307 @default.
• W2506577675 cites W2111078819 @default.
• W2506577675 cites W2119047464 @default.
• W2506577675 cites W2123204707 @default.
• W2506577675 cites W2126216415 @default.
• W2506577675 cites W2137256041 @default.
• W2506577675 cites W2142234851 @default.
• W2506577675 cites W2153178807 @default.
• W2506577675 cites W2158612941 @default.
• W2506577675 cites W2474347819 @default.
• W2506577675 cites W3103163367 @default.
• W2506577675 cites W3103878535 @default.
• W2506577675 cites W3103897637 @default.
• W2506577675 cites W3106213721 @default.
• W2506577675 cites W4376595652 @default.
• W2506577675 doi "https://doi.org/10.1051/0004-6361/201528062" @default.
• W2506577675 hasPublicationYear "2016" @default.
• W2506577675 type Work @default.
• W2506577675 sameAs 2506577675 @default.
• W2506577675 citedByCount "9" @default.
• W2506577675 countsByYear W25065776752017 @default.
• W2506577675 countsByYear W25065776752018 @default.
• W2506577675 countsByYear W25065776752020 @default.
• W2506577675 countsByYear W25065776752021 @default.
• W2506577675 countsByYear W25065776752022 @default.
• W2506577675 crossrefType "journal-article" @default.
• W2506577675 hasAuthorship W2506577675A5019460672 @default.
• W2506577675 hasAuthorship W2506577675A5032226441 @default.
• W2506577675 hasAuthorship W2506577675A5036076449 @default.
• W2506577675 hasAuthorship W2506577675A5049796911 @default.
• W2506577675 hasAuthorship W2506577675A5054287990 @default.
• W2506577675 hasAuthorship W2506577675A5068190184 @default.
• W2506577675 hasBestOaLocation W25065776751 @default.
• W2506577675 hasConcept C108411613 @default.
• W2506577675 hasConcept C115260700 @default.
• W2506577675 hasConcept C120665830 @default.
• W2506577675 hasConcept C121332964 @default.
• W2506577675 hasConcept C1276947 @default.
• W2506577675 hasConcept C146138569 @default.
• W2506577675 hasConcept C147789679 @default.
• W2506577675 hasConcept C162996421 @default.
• W2506577675 hasConcept C185001636 @default.
• W2506577675 hasConcept C185592680 @default.
• W2506577675 hasConcept C205049153 @default.
• W2506577675 hasConcept C2779588948 @default.
• W2506577675 hasConcept C41008148 @default.
• W2506577675 hasConcept C44838205 @default.
• W2506577675 hasConcept C44870925 @default.
• W2506577675 hasConcept C509933004 @default.
• W2506577675 hasConcept C62520636 @default.
• W2506577675 hasConcept C72886185 @default.
• W2506577675 hasConcept C74064498 @default.
• W2506577675 hasConcept C76155785 @default.
• W2506577675 hasConcept C92545706 @default.
• W2506577675 hasConceptScore W2506577675C108411613 @default.
• W2506577675 hasConceptScore W2506577675C115260700 @default.
• W2506577675 hasConceptScore W2506577675C120665830 @default.
• W2506577675 hasConceptScore W2506577675C121332964 @default.
• W2506577675 hasConceptScore W2506577675C1276947 @default.

• next