SH001
New Insights on the Mass and Energy Transfer in the Low Solar Atmosphere: The DKIST/ALMA/IRIS Era II Posters

Monday, 7 December 2020: 04:00-20:59
Poster
Primary Convener:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Conveners:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Gianna Cauzzi, National Solar Observatory, Tucson, AZ, United States and Jorrit Leenaarts, Institute for Solar Physics, Stockholm University, Stockholm, Sweden
Primary Liaison:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Chairs:  Gianna Cauzzi, INAF-Ossevatorio Astrofisico di Arcetri, Firenze, Italy, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Jorrit Leenaarts, Institute for Solar Physics, Stockholm University, Stockholm, Sweden
OSPA Liaison:  Gianna Cauzzi, INAF-Ossevatorio Astrofisico di Arcetri, Firenze, Italy
 
Probing chromospheric heating with millimeter interferometry (680502)
João Manuel da Silva Santos1, Jaime de la Cruz Rodriguez1, Stephen M. White2, Jorrit Leenaarts1, Gregal J. M. Vissers1, Viggo Haraldson Hansteen3,4 and Sanja Danilovic1, (1)Institute for Solar Physics, Stockholm University, Stockholm, Sweden, (2)Space Vehicles Directorate, Air Force Research Laboratory, Albuquerque, NM, United States, (3)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, (4)Institute for Theoretical Astrophysics, University of Oslo, Oslo, Norway
 
ALMA observations and spectral inversions - what can we learn about the Sun and our techniques? (751703)
Ryan Hofmann, National Solar Observatory, Boulder, CO, United States, Kevin Reardon, National Solar Observatory, Tucson, AZ, United States and Ivan Milic, University of Colorado at Boulder, Boulder, CO, United States
 
Constraining wave propagation throughout the solar atmosphere with IBIS, ALMA and IRIS (688255)
Momchil Molnar1,2, Kevin Reardon1, Steven R Cranmer3 and Adam F Kowalski2, (1)National Solar Observatory, Boulder, CO, United States, (2)University of Colorado at Boulder, Boulder, CO, United States, (3)University of Colorado, Boulder, CO, United States
 
Spectral Contrast in Chromospheric Quiescent Emission (760760)
Daniela Lacatus, High Altitude Observatory, Boulder, CO, United States; Monash University, Melbourne, VIC, Australia and Alina Catalina Donea, Monash University, School of Mathematics, Melbourne, Australia
 
Characterization of UV Bursts Using Line-Ratio Density Diagnostics (730538)
Fiona Conneely1, Chad Allen Madsen2 and Edward DeLuca2, (1)University of San Francisco, San Francisco, CA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
 
Chromospheric response to emergence of internetwork magnetic fields (758958)
Milan Gosic, Bay Area Environmental Research Institute - LMSAL, Palo Alto, CA, United States, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Luis Bellot Rubio, Instituto de Astrofisica de Andalucia (IAA-CSIC), Granada, Spain and Alberto Sainz Dalda, Bay Area Environmental Research Institute - LMSAL, Palo Alto, United States
 
Fine-scale explosive energy release at sites of magnetic flux cancellation in the core of a solar active region: Hi-C 2.1, IRIS and SDO observations (713444)
Sanjiv K Tiwari1, Navdeep K. Panesar1, Ron L Moore2, Bart De Pontieu1, Amy R Winebarger3 and Hi-C 2.1 Science Team , (1)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (2)National Space Science and Technology Center, Huntsville, AL, United States, (3)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
IRIS Mg II Observations and Non-LTE Modeling of Off-limb Spicules (686749)
Akiko Tei1, Stanislav Gunár2, Petr Heinzel3, Takenori J. Okamoto4, Jiří Štěpán2, Sonja Jejčič5,6 and Kazunari Shibata7,8, (1)Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan, (2)Astronomical Institute, Czech Academy of Sciences, Ondřejov, Czech Republic, (3)Astronomical Institute, Czech Academy of Sciences, Ondrejov, Czech Republic, (4)National Astronomical Observatory of Japan, Mitaka, Tokyo, Japan, (5)Faculty of Education, University of Ljubljana, Ljubljana, Slovenia, (6)Faculty of Mathematics and Physics, University of Ljubljana, Ljubljana, Slovenia, (7)Kyoto University, Kyoto, Japan, (8)Doshisha University, Kyotanabe, Japan
 
ALMA and IRIS Observations Highlighting the Dynamics and Structure of Chromospheric Plage (689677)
Georgios Chintzoglou1, Bart De Pontieu2, Juan Martinez-Sykora3, Viggo Haraldson Hansteen4, Jaime de la Cruz Rodriguez5, Mikolaj Szydlarski6, Shahin Jafarzadeh6, Sven Wedemeyer6, Tim Bastian7 and Alberto Sainz Dalda8, (1)University Corporation for Atmospheric Research, Boulder, CO, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)Bay Are Environmental Research Institute - LMSAL, Palo Alto, CA, United States, (4)Inst Theoretical Astrophysics, Oslo, Norway, (5)Institute for Solar Physics, Dept. of Astronomy, Stockholm University, AlbaNova University Centre, Stockholm, Sweden, (6)University of Oslo, Institute of Theoretical Astrophysics, Oslo, Norway, (7)Natl Radio Astron Observ, Charlottesville, VA, United States, (8)Bay Area Environmental Research Institute - LMSAL, Palo Alto, United States
 
The correlation between chromospheric and coronal heating in active region plage (701384)
Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Viggo Haraldson Hansteen, Inst Theoretical Astrophysics, Oslo, Norway, Amy R Winebarger, NASA Marshall Space Flight Center, Huntsville, AL, United States and The HiC team
 
Implications of the correlation between Doppler shifts and line widths in Si IV spectral lines from the active region transition region (685953)
Dana Longcope, Montana State University, Bozeman, MT, United States and Chunming Zhu, Montana State University, Physics, Bozeman, MT, United States
 
Measuring complex bright-point motion and wave excitation in high-resolution solar observations (707870)
Samuel Van Kooten, University of Colorado at Boulder, Astrophysical & Planetary Sciences, Boulder, CO, United States and Steven R Cranmer, University of Colorado, Boulder, CO, United States
 
Spectroscopic Observations of the Eruption of an Filament and Associated Magnetic Reconnection (728008)
Huidong Hu1, Ying D. Liu1, Hardi Peter2, Lakshmi Pradeep Chitta3 and Rui Wang1, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (3)Max Planck Institute for Solar System Research, Göttingen, Germany
 
Solar Prominence Bubbles and Associated Plasma Instabilities: IRIS Observations and MHD Modeling (774364)
Wei Liu, Bay Area Environmental Research Institute Palo Alto, Palo Alto, CA, United States, Thomas E Berger, NOAA Space Weather Prediction Center, Boulder, CO, United States and Yuhong Fan, NCAR, Boulder, CO, United States
 
Effects of Cowling Resistivity in the Weakly-Ionized Chromosphere (761632)
Mehmet Sarp Yalim1, Avijeet Prasad2, Nikolai V Pogorelov3, Gary Paul Zank4, Qiang Hu3 and Sanjiv K. Tiwari5, (1)University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, (2)University of Alabama in Huntsville, Huntsville, United States, (3)University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States, (4)Univ of Alabama, Huntsville, Huntsville, AL, United States, (5)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States
 
Multi-Fluid Simulations of Collisional Plasma Instabilities in the Solar Chromosphere (746305)
Samuel Evans1, Juan Martínez-Sykora2, Yakov S Dimant1 and Meers M Oppenheim1, (1)Boston University, Center for Space Physics, Boston, MA, United States, (2)LMSAL, San Francisco, CA, United States
 
On the velocity drift between ions in the solar atmosphere (713416)
Juan Martínez-Sykora, Bay Area Environmental Research Institute Moffett Field, Moffett Field, CA, United States, Mikolaj Szydlarski, University of Oslo, Institute of Theoretical Astrophysics, Oslo, Norway, Viggo Haraldson Hansteen, Inst Theoretical Astrophysics, Oslo, Norway and Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
Collisional and Reactive Multi-fluid Modeling of Acoustic Wave Propagation and Heating in Gravitationally Stratified Chromospheric plasma (681603)
Fan Zhang1, Stefaan Poedts1,2, Andrea Lani1, Błażej Kuźma2 and Kris Murawski2, (1)KU Leuven, Centre for mathematical Plasma-Astrophysics, Department of Mathematics, Leuven, Belgium, (2)University of Maria Curie-Skłodowska, Institute of Physics, Lublin, Poland
 
Expected spectropolarimetric observables in the lower solar atmosphere from 3D radiative MHD models (705229)
Alberto Sainz Dalda, Bay Area Environmental Research Institute - LMSAL, Palo Alto, United States; Stanford University, Stanford, United States, Milan Gosic, Bay Area Environmental Research Institute - LMSAL, Palo Alto, CA, United States and Juan Martinez-Sykora, Bay Are Environmental Research Institute - LMSAL, Palo Alto, CA, United States; University of Oslo, Oslo, Norway
 
Chromospheric and TR diagnostics in a large scale numerical simulation of flux emergence: Synthetic vs Real observables (741973)
Viggo Haraldson Hansteen, Bay Area Environmental Research Institute Palo Alto, Palo Alto, CA, United States, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Paola Testa, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Milan Gosic, Lockheed Martin Solar & Astrophysics Laboratory, Palo Alto, CA, United States and Juan Martinez-Sykora, Bay Are Environmental Research Institute - LMSAL, Palo Alto, CA, United States
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