Search Results - "JIONG QIU"
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Tracing field lines that are reconnecting, or expanding, or both
Published in Frontiers in astronomy and space sciences (22-07-2024)“…The explosive release of energy in the solar atmosphere is driven magnetically, but the mechanisms that trigger the onset of the eruption remain controversial…”
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2
Observational Analysis of Magnetic Reconnection Sequence
Published in The Astrophysical journal (20-02-2009)“…We conduct comprehensive analysis of an X2.0 flare to derive quantities indicative of magnetic reconnection in solar corona by following temporally and…”
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LONG DURATION FLARE EMISSION: IMPULSIVE HEATING OR GRADUAL HEATING?
Published in The Astrophysical journal (20-03-2016)“…ABSTRACT Flare emissions in X-ray and EUV wavelengths have previously been modeled as the plasma response to impulsive heating from magnetic reconnection. Some…”
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4
Two-phase Heating in Flaring Loops
Published in The Astrophysical journal (20-03-2018)“…We analyze and model a C5.7 two-ribbon solar flare observed by the Solar Dynamics Observatory, Hinode, and GOES on 2011 December 26. The flare is made of many…”
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HEATING OF FLARE LOOPS WITH OBSERVATIONALLY CONSTRAINED HEATING FUNCTIONS
Published in The Astrophysical journal (20-06-2012)“…We analyze high-cadence high-resolution observations of a C3.2 flare obtained by AIA/SDO on 2010 August 1. The flare is a long-duration event with soft X-ray…”
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Micro-nano aeration is a promising alternative for achieving high-rate partial nitrification
Published in The Science of the total environment (15-11-2021)“…Biological nitrogen removal is the most prevalent wastewater nitrogen removal process but nitrification limits the rate of the whole process mainly due to the…”
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Reconnection and Energetics in Two-ribbon Flares: A Revisit of the Bastille-day Flare
Published in The Astrophysical journal (10-12-2010)“…We conduct a semi-quantitative analysis of two-ribbon flares to investigate the observational relationship between magnetic reconnection and energetics by…”
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A RECONNECTION-DRIVEN MODEL OF THE HARD X-RAY LOOP-TOP SOURCE FROM FLARE 2004 FEBRUARY 26
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT A compact X-class flare on 2004 February 26 showed a concentrated source of hard X-rays at the tops of the flare's loops. This was analyzed in…”
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Evolution of Solar Eruptive Events: Investigating the Relationships among Magnetic Reconnection, Flare Energy Release, and Coronal Mass Ejections
Published in The Astrophysical journal (01-04-2023)“…We study the evolution of solar eruptive events by investigating the temporal relationships among magnetic reconnection, flare energy release, and the…”
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Evolution of a Magnetic Flux Rope toward Eruption
Published in The Astrophysical journal (20-01-2019)“…It is well accepted that a magnetic flux rope (MFR) is a critical component of many coronal mass ejections (CMEs), yet how it evolves toward eruption remains…”
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Investigating Pre-eruptive Magnetic Properties at the Footprints of Erupting Magnetic Flux Ropes
Published in The Astrophysical journal (01-02-2023)“…It is well established that solar eruptions are powered by free magnetic energy stored in the current-carrying magnetic field in the corona. It has also been…”
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12
Structure of the Plasma near the Heliospheric Current Sheet as Seen by WISPR/Parker Solar Probe from inside the Streamer Belt
Published in The Astrophysical journal (01-05-2023)“…Parker Solar Probe (PSP) crossed the heliospheric current sheet (HCS) near the perihelion on encounters E8 and E11, enabling the Wide-field Imager for Solar…”
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Evidence of Continuous Reconnection along a Helmet Streamer Current Sheet Observed by WISPR on Parker Solar Probe
Published in The Astrophysical journal (01-07-2024)“…Parker Solar Probe's second solar encounter from 2019 March 30 to April 11 occurred during a period when the corona had a simple magnetic structure and…”
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DETERMINING HEATING RATES IN RECONNECTION FORMED FLARE LOOPS OF THE M8.0 FLARE ON 2005 MAY 13
Published in The Astrophysical journal (20-06-2013)“…We analyze and model an M8.0 flare on 2005 May 13 observed by the Transition Region and Coronal Explorer and the Reuven Ramaty High Energy Solar Spectroscopic…”
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On the Magnetic Flux Budget in Low-Corona Magnetic Reconnection and Interplanetary Coronal Mass Ejections
Published in The Astrophysical journal (10-04-2007)“…We present the first quantitative comparison between the total magnetic reconnection flux in the low corona in the wake of coronal mass ejections (CMEs) and…”
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Large-scale Coronal Dimming Foreshadowing a Solar Eruption on 2011 October 1
Published in The Astrophysical journal (01-02-2024)“…Understanding large-scale solar eruptions requires detailed investigation of the entire system's evolution, including the magnetic environment enveloping the…”
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A FLARE OBSERVED IN CORONAL, TRANSITION REGION, AND HELIUM I 10830 Å EMISSIONS
Published in The Astrophysical journal (01-10-2014)“…On 2012 June 17, we observed the evolution of a C-class flare associated with the eruption of a filament near a large sunspot in the active region NOAA 11504…”
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ULTRAVIOLET AND EXTREME-ULTRAVIOLET EMISSIONS AT THE FLARE FOOTPOINTS OBSERVED BY ATMOSPHERE IMAGING ASSEMBLY
Published in The Astrophysical journal (01-09-2013)“…A solar flare is composed of impulsive energy release events by magnetic reconnection, which forms and heats flare loops. Recent studies have revealed a…”
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Magnetic diffusion in solar atmosphere produces measurable electric fields
Published in Nature communications (11-10-2024)“…The efficient release of magnetic energy in astrophysical plasmas, such as during solar flares, can in principle be achieved through magnetic diffusion, at a…”
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Direct Observation of High-Speed Plasma Outflows Produced by Magnetic Reconnection in Solar Impulsive Events
Published in The Astrophysical journal (01-06-2007)“…Spectroscopic observations of a solar limb flare recorded by SUMER on SOHO reveal for the first time hot, fast magnetic reconnection outflows in the corona. As…”
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