JQ
Member Since 2018
Jiong Qiu
Montana State University
AGU Research
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A New Form of the Biot-Savart Law and Decomposition of Vector Magnetograms
ONLINE POSTER SESSION FOR SPA: SOLAR AND HELIOSPHERIC PHYSICS I
spa-solar and heliospheric physics | 22 january 2024
Viacheslav S. Titov, Cooper Downs, Tibor Torok, Jo...
We have derived a new form of the Biot-Savart law that allows one to calculate the coronal magnetic field generated by a closed line current under the...
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Energy Release Process in the 2021 October 28 X1.0 Flare
SOLAR FLARE ONSET AND ENERGY RELEASE III ORAL
spa-solar and heliospheric physics | 16 december 2022
Brock Parker, Chunming Zhu, Jiong Qiu, Dana Longco...
We study the heating process in the X1.0 flare on 2021 October 28 using the UV Footpoint Calorimeter (UFC) method. This method efficiently derives fla...
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Early Bursts during Flare Precursor and the Relationship to Onset of Solar Eruption
SOLAR FLARE ONSET AND ENERGY RELEASE II POSTER
spa-solar and heliospheric physics | 16 december 2022
Chunming Zhu, Jiong Qiu, Juliana T. Vievering, Lau...
We investigate the characteristics of early bursts during the precursor phase of flares, to understand what role magnetic reconnection plays in the in...
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UV Foot-point Calorimeter (UFC) Method and the UV-SXR Neupert Effect in Solar Flares
SOLAR FLARE ONSET AND ENERGY RELEASE I ONLINE POSTER DISCUSSION
spa-solar and heliospheric physics | 16 december 2022
Jiong Qiu, Dana Longcope, Chunming Zhu
We have developed the Ultraviolet Foot-point Calorimeter (UFC) method to model flare heating. The experiment extends the traditional Neupert effect to...
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Measuring Magnetic Reconnection Rate and Shear in a Two-ribbon Flare
SOLAR FLARE ONSET AND ENERGY RELEASE II POSTER
spa-solar and heliospheric physics | 16 december 2022
Audrey Robison, Jiong Qiu
How magnetic reconnection converts free magnetic energy into flare energy is an outstanding question in solar flare physics. To shed light on this iss...
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Insights into Solar Flare Reconnection and Energetics from Novel Forms of Observation and Modeling
SOLAR FLARE ONSET AND ENERGY RELEASE III ORAL
spa-solar and heliospheric physics | 16 december 2022
Dana Longcope, Jiong Qiu
According to our current understanding, solar flares are driven by magnetic energy stored in the solar corona being rapidly released through a process...
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The Multi-scale Inner Structure of Coronal Streamers Imaged by WISPR/Parker Solar Probe
PARKER SOLAR PROBE OBSERVATIONS OF NEAR-SUN PHENOMENA I ONLINE POSTER DISCUSSION
spa-solar and heliospheric physics | 14 december 2022
Paulett C. Liewer, Jiong Qiu, Paulo Penteado, Ange...
In its eighth orbit, Parker Solar Probe (PSP) reached a perihelion of 16 Rsun. From this vantage point, the inner edge (13.5o from Sun center) of WISP...
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Investigating Energy Release during Solar Eruptive Events
MAGNETOSPHERIC PHYSICS: GENERAL CONTRIBUTIONS INCLUDING RESEARCH SUPPORTED BY THE HELIOPHYSICS SYSTEM OBSERVATORY I ORAL
spa-magnetospheric physics | 13 december 2022
Juliana T. Vievering, Angelos Vourlidas, Chunming ...
The overarching science goal for our study is to understand the relationships among magnetic reconnection, flare energy release, and initiation/accele...
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