SH037
Solar and Heliospheric Physics: General Contributions V Posters

Monday, 14 December 2020: 04:00-20:59
Poster
Primary Convener:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
Conveners:  Romina Nikoukar, Johns Hopkins Applied Physics Laboratory, Laurel, MD, United States and Elizabeth MacDonald, National Aeronautics and Space Administration, Minneapolis, MN, United States
Primary Liaison:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
Chairs:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States and Erika Palmerio, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
OSPA Liaison:  Christina O Lee, Boston College, Institute for Scientific Research, Chestnut Hill, MA, United States
 
Cross Sections of Coronal Loop Flux Tubes (694935)
James A Klimchuk, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Craig DeForest, Southwest Research Institute, Boulder, CO, United States
 
Can nanoflare heating define the coronal loop size? (684712)
Vadim M Uritsky, Catholic University of America, Washington, DC, United States, Kalman Knizhnik, Naval Research Lab, Washington DC, DC, United States and James A Klimchuk, NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States
 
Understanding Heating Properties in Hot and Warm Active Region Loops through Hydrodynamics and Forward Modeling (668104)
Will Barnes1, Harry Warren2 and Jeffrey W Reep2, (1)National Research Council Research Associate Residing at the US Naval Research Laboratory, Washington, DC, United States, (2)US Naval Research Laboratory, Space Science Division, Washington, DC, United States
 
Evidence of Solar Coronal Heating by Nanoflares Based on Time-Lag Measurements in EUV Light Curves from EIS (681417)
Jeffrey W Brosius, Catholic University of America, Washington, DC, United States and Nicholeen M Viall, NASA GSFC, Greenbelt, MD, United States
 
Coronal Heating Consequences from Alfvén Wave Turbulence in Solar Coronal Loops (754106)
Sydney Hamann1, Mahboubeh Asgari-Targhi2 and Nishu Karna2, (1)University of Georgia, Athens, GA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
 
Investigating power law power spectra as a diagnostic of nanoflare coronal heating in active regions (732366)
Jack Ireland, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Stephen J. Bradshaw, Rice University, Department of Physics and Astronomy, Houston, TX, United States, Nicholeen M Viall, NASA GSFC, Greenbelt, MD, United States and Michael S Kirk, Atmospheric and Space Technology Research Associates, LLC, Boulder, CO, United States
 
A Multi-Fluid Multi-Species (MFMS) numerical code for simulating the solar atmosphere (757082)
Quentin Wargnier, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Juan Martínez-Sykora, LMSAL, San Francisco, CA, United States, Viggo Haraldson Hansteen, Inst Theoretical Astrophysics, Oslo, Norway, Mikolaj Szydlarski, University of Oslo, Institute of Theoretical Astrophysics, Oslo, Norway and Samuel Evans, Boston University, Center for Space Physics, Boston, MA, United States
 
Modeling the Solar Corona: Testing Nonlinear Force-Free Methods with a Magneto-Hydrostatic Test Case (705348)
Santiago Rodriguez1,2, Stuart A Gilchrist2, K. D. Leka3 and Karin Dissauer3, (1)University of Colorado Boulder, Boulder, United States, (2)NorthWest Research Associates Boulder, Boulder, CO, United States, (3)NorthWest Research Associates Boulder, Boulder, United States
 
Estimating Coronal Propagation Effects in the Quiet Sun Corona Using Low Radio Frequency Observations (718935)
Divya Oberoi, Tata Institute for Fundamental Research, National Center for Radio Astronomy, Bangalore, India and Rohit Sharma, University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland
 
Generation of MLSO K-Coronagraph white light images from SDO/AIA EUV (171, 193 & 211 passbands) using deep learning (692186)
Bendict Lawrance1, Yong-Jae Moon2, Eunsu Park3, Il-Hyun Cho4, Harim Lee2 and A. Shanmugaraju5, (1)Kyung Hee University, Department of Astronomy and Space Science, South Korea, Yongin-si, South Korea, (2)School of Space Research, Kyung Hee University, Yongin, South Korea, (3)Department of Astronomy & Space Science, Kyung Hee University, Yongin, South Korea, (4)Kyung Hee University, Astronomy and Space Science, Yongin-si, South Korea, (5)Arul Anandar College, Karumathur, Madurai, Department of Physics, Madurai, India
 
Generation of He I 1083nm Images from SDO/AIA Images by Deep Learning (720984)
Jihyeon Son1, Junghun Cha2, Yong-Jae Moon1, Harim Lee3, Eunsu Park3 and Hyun-Jin Jeong1, (1)School of Space Research, Kyung Hee University, Yongin, South Korea, (2)Department of Astronomy & Space Science, Kyung Hee University, Yongin-si, South Korea, (3)Department of Astronomy & Space Science, Kyung Hee University, Yongin, South Korea
 
Extraction of Photospheric and Chromospheric Bright Regions and aSunspot Using Fuzzy C-Means Clustering and Region Growing Methods (731646)
Shahriar Esmaeili, Texas A&M University College Station, Department of Physics and Astronomy, College Station, TX, United States, Mohsen Javaherian, University of Maragheh, Institute of Astronomy and Astrophysics of Maragha, Maragheh, Iran and Farzaneh Jafari, University of Mohaghegh Ardabili, Department of Physics, Ardabil, Iran
 
An Improved Data-Driven Analysis Pipeline for Coronal Hole Detection and Mapping (700193)
Tamar Ervin, James Turtle, Cooper Downs, Ronald M. Caplan and Jon Linker, Predictive Science Inc., San Diego, CA, United States
 
Solar cycle around the onset of the Spoerer Minimum (671433)
Hiroko Miyahara1, Toru Moriya2, Fuyuki Tokanai2, Mirei Takeyama2, Hirohisa Sakurai2, Motonari Ohyama3 and Masataka Hakozaki4, (1)Musashino Art University, Kodaira-city, Japan, (2)Yamagata University, Yamagata, Japan, (3)Tohoku University, Sendai, Japan, (4)National Museum of Japanese History, Sakura, Japan
 
10Be record in travertine sediment: a potential proxy for reconstructing high-resolution solar activity (715752)
Hongyang Xu1,2, Hiroko Miyahara2, Limin Zhou1 and Kazuho Horiuchi3, (1)East China Normal University, Shanghai, China, (2)Musashino Art University, Kodaira-city, Japan, (3)Hirosaki University, Aomori, Japan
 
Update on Space Physics Data Facility (SPDF) Data Archives and Services (713678)
Robert M Candey1, Dieter Bilitza1,2, Reine Chimiak1, John F Cooper1, Leonard N Garcia1,3, Bernard T Harris1, Lan Jian1, Rita C Johnson1,4, Tamara J Kovalick1,4, Nand Lal1, Howard A Leckner1,4, Michael H Liu1,4, Sonya Lyatsky1,5, Robert E McGuire1, Natalia E Papitashvili1,4, Uthra R Rao1,4, D Aaron Roberts1 and Ronald E Yurow1,4, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)George Mason University, Washington, DC, United States, (3)SGT, Inc., Lanham, MD, United States, (4)ADNET Systems Inc., Greenbelt, MD, United States, (5)Catholic University of America, Washington, DC, United States
 
Development of a Telescope Design System Using STOP Analysis (759830)
Sukhmanpreet Singh, Yale University, New Haven, CT, United States, Peter Cheimets, SAO, Cambridge, MA, United States and Edward Hertz, SAO, Cambridge, United States
 
Modeling the whistler-heat flux instability in the solar wind using skew kappa distribution functions (689889)
Bea Zenteno-Quinteros, University of Chile, Departamento de Fisica, Santiago, Chile, Adolfo F Viñas, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States and Pablo S Moya, University of Chile, Santiago, Chile
 
Spontaneous Magnetic Fluctuations of Kappa Electron Distributions (714805)
Daniel Hermosilla1, Pablo S Moya1, Rodrigo A López2, Marian Lazar3 and Stefaan Poedts4, (1)University of Chile, Santiago, Chile, (2)Univ. Chile, Santiago, Chile, (3)Katholieke Universiteit Leuven, Department of Mathematics, Leuven, Belgium, (4)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium
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