Bright ultraviolet knots as possible sources of coherent microwave radiation

A distinctive feature of the September 6, 2012 event was that sources of narrow-band (2–4 GHz) sub-second pulses (SSP) were observed in small areas of flare loops with so-called bright ultraviolet knots with high plasma density up to 1011 10¹¹ cm⁻³. Time profiles of hard X-rays of the flare, althoug...

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Main Authors: Meshalkina N. S., Altyntsev A. T.
Format: Article
Language:English
Published: INFRA-M 2023-12-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/65064/view
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author Meshalkina N. S.
Altyntsev A. T.
author_facet Meshalkina N. S.
Altyntsev A. T.
author_sort Meshalkina N. S.
collection DOAJ
description A distinctive feature of the September 6, 2012 event was that sources of narrow-band (2–4 GHz) sub-second pulses (SSP) were observed in small areas of flare loops with so-called bright ultraviolet knots with high plasma density up to 1011 10¹¹ cm⁻³. Time profiles of hard X-rays of the flare, although similar to microwave light curves, do not have structures corresponding to SSP. Analysis of microwave, X-ray, and ultraviolet data has shown that the observable pulses of microwave radiation with a narrow spectral band are coherent in nature and are generated by electrons with energies of several tens of kiloelectronvolt in bright knots at a double plasma frequency. The results of the observations suggest that the appearance of bright knots is associated with local processes of energy release due to interaction of flare loops.
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spelling doaj.art-52a13dd507ef491f80d0c9c8b24f27902024-01-07T07:45:15ZengINFRA-MSolar-Terrestrial Physics2500-05352023-12-0194172410.12737/stp-94202302Bright ultraviolet knots as possible sources of coherent microwave radiationMeshalkina N. S.0Altyntsev A. T.1Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, RussiaInstitute of Solar-Terrestrial Physics SB RAS, Irkutsk, RussiaA distinctive feature of the September 6, 2012 event was that sources of narrow-band (2–4 GHz) sub-second pulses (SSP) were observed in small areas of flare loops with so-called bright ultraviolet knots with high plasma density up to 1011 10¹¹ cm⁻³. Time profiles of hard X-rays of the flare, although similar to microwave light curves, do not have structures corresponding to SSP. Analysis of microwave, X-ray, and ultraviolet data has shown that the observable pulses of microwave radiation with a narrow spectral band are coherent in nature and are generated by electrons with energies of several tens of kiloelectronvolt in bright knots at a double plasma frequency. The results of the observations suggest that the appearance of bright knots is associated with local processes of energy release due to interaction of flare loops.https://naukaru.ru/en/nauka/article/65064/viewsunfine temporal structureuv bright knotsmicrowave burstscoherent emission
spellingShingle Meshalkina N. S.
Altyntsev A. T.
Bright ultraviolet knots as possible sources of coherent microwave radiation
Solar-Terrestrial Physics
sun
fine temporal structure
uv bright knots
microwave bursts
coherent emission
title Bright ultraviolet knots as possible sources of coherent microwave radiation
title_full Bright ultraviolet knots as possible sources of coherent microwave radiation
title_fullStr Bright ultraviolet knots as possible sources of coherent microwave radiation
title_full_unstemmed Bright ultraviolet knots as possible sources of coherent microwave radiation
title_short Bright ultraviolet knots as possible sources of coherent microwave radiation
title_sort bright ultraviolet knots as possible sources of coherent microwave radiation
topic sun
fine temporal structure
uv bright knots
microwave bursts
coherent emission
url https://naukaru.ru/en/nauka/article/65064/view
work_keys_str_mv AT meshalkinans brightultravioletknotsaspossiblesourcesofcoherentmicrowaveradiation
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