SH43A:
Mass and Energy Transfer Between the Solar Photosphere and Corona Posters

Submit an Abstract to this Session



Session ID#: 25206

Session Description:
The transport and deposition of non-thermal energy from the photosphere through the chromosphere into the corona drives the dynamics and energetics of the low solar atmosphere and holds the key to chromospheric and coronal heating and solar wind acceleration. Our view of these processes is rapidly changing with the advent of high resolution imaging and spectroscopy covering a wide range of temperatures from photosphere to corona, coupled with advanced numerical simulations. These results highlight the critical role played by the chromosphere in mediating non-thermal energy. This session is focused on new views of the mass and energy transfer between the photosphere and corona, with a particular focus on the chromosphere, and welcomes contributions using recent observations with space-based assets like IRIS, SDO and Hinode, ground-based telescopes (e.g., ALMA), and/or numerical simulations of the coupled solar atmosphere.
Primary Convener:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Convener:  Scott William McIntosh, High Altitude Observatory, Boulder, United States
Chairs:  Scott William McIntosh, High Altitude Observatory, Boulder, United States and Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
OSPA Liaison:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Index Terms:

7507 Chromosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7546 Transition region [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Abstracts Submitted to this Session:

Turbulence Generation by Slow Magnetosonic Wave and Its Implication in Coronal Heating (212592)
Prachi Sharma, Indian Institute of Technology Delhi, New Delhi, India and R. P. Sharma, Indian Institute of Technology, Delhi, India, Centre for Energy Studies, New Delhi, India
MHD Wave Propagation at the Interface Between Solar Chromosphere and Corona (277937)
Paul Song, University of Massachusetts Lowell, Lowell, MA, United States, Vytenis M Vasyliunas, Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany and Yifan Huang, Los Alamos National Lab, Los Alamos, United States
Coronal Heating and the Magnetic Field in Solar Active Regions (280493)
David Allen Falconer, UAHuntsville, Huntsville, AL, United States, Sanjiv K Tiwari, Bay Area Environmental Research Institute Palo Alto, Palo Alto, CA, United States, Amy R Winebarger, NASA Marshall Space Flight Center, Huntsville, AL, United States and Ronald Lee Moore, NASA MSFC, Huntsville, United States
A Microfilament-Eruption Mechanism for Solar Spicules (233738)
Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States and Ronald Lee Moore, NASA MSFC, Huntsville, United States
Dynamic Solar Coronal Jets occurring in a Near-Limb Active Region (263489)
Joy Velasquez, Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States, David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States, Ronald L Moore, NASA Marshall Space Flight Center, Huntsville, United States and Navdeep Kaur Panesar, NASA MSFC, Huntsville, AL, United States
Observations and Modeling of Transition Region and Coronal Heating Associated with Spicules (263319)
Bart De Pontieu1, Juan Martinez-Sykora2, Ineke De Moortel3, Georgios Chintzoglou1 and Scott William McIntosh4, (1)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (2)Bay Area Environmental Research Institute - LMSAL, Palo Alto, CA, United States, (3)University of St Andrews, School of Mathematics and Stastics, St Andrews, United Kingdom, (4)High Altitude Observatory, Boulder, United States
Bridging the Gap: Capturing the Lyα Counterpart of a Type-II Spicule and its Heating Evolution with VAULT2.0 and IRIS Campaign Observations (264734)
Georgios Chintzoglou1,2, Bart De Pontieu2, Juan Martinez-Sykora3, Tiago Mendes Domingos Pereira4, Angelos Vourlidas5 and Samuel Tun Beltran6, (1)University Corporation for Atmospheric Research, Boulder, CO, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)Bay Area Environmental Research Institute - LMSAL, Palo Alto, CA, United States, (4)Institute for Theoretical Astrophysics, Oslo, Norway, (5)Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States, (6)US Naval Research Laboratory, Washington, DC, United States
Dynamics in the Chromosphere Imaged at Four Second Cadence (251359)
Don Schmit, Catholic University of America, Washington, DC, United States, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and the CLASP team
Magnetic Flux Cancellation as the Trigger of Solar Coronal Jets (225081)
Riley McGlasson1, Navdeep Kaur Panesar2, Alphonse C Sterling2 and Ronald Lee Moore3,4, (1)Macalester College, Saint Paul, MN, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States, (3)University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States, (4)NASA Marshall Space Flight Center, Huntsville, United States
Critical Magnetic Field Strengths for Unipolar Solar Coronal Plumes in Quiet Regions and Coronal Holes? (228971)
Ellis A Avallone, University of Hawaii at Manoa, Astronomy, Honolulu, HI, United States, Sanjiv K Tiwari, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States; Bay Area Environmental Research Institute Palo Alto, Palo Alto, CA, United States, Navdeep Kaur Panesar, NASA Marshall Space Flight Center, Huntsville, AL, United States and Ronald Lee Moore, NASA Marshall Space Flight Center, Huntsville, United States; University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States
Conditions for Thermal Non-Equilibrium (256297)
James A Klimchuk, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Manuel Luna, Universidad de Las Islas Baleares, Physics, Palma de Mallorca, Spain
Magnetic Connection and Properties of the Solar Magnetic Field (261764)
Brandon L Burkholder, University of Alaska Fairbanks, Fairbanks, United States, Antonius Otto, Geophysical Institute Fairbanks, Fairbanks, AK, United States, Joseph Borovsky, Space Science Institute, Los Alamos, United States and Peter A Delamere, University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States
Numerical MHD Coronal Simulations: Energy Statistics and FORWARD Analysis. (264417)
Kenzie Nimmo, University of Glasgow, Glasgow, G12, United Kingdom, Matthias Rempel, National Center for Atmospheric Research, High Altitude Observatory, Boulder, United States, Feng Chen, National Center for Atmospheric Research, Boulder, CO, United States, Sarah E Gibson, National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States and Yuhong Fan, NCAR, Boulder, United States
Ellerman bombs and UV bursts: reconnection at different atmospheric layers? (271478)
Viggo Haraldson Hansteen, Institute for Theoretical Astrophysics, University of Oslo, Oslo, Norway, Ada N Ortiz-Carbonell and Luc Rouppe van der Voort, University of Oslo, Oslo, Norway
Results of the IRIS UV Burst Survey, Part I: Active Regions Tracked Limb to Limb (299813)
Chad Allen Madsen, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States and Edward DeLuca, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
The temporal evolution of explosive events and its implication on reconnection dynamics (294937)
Wei Liu, Bay Area Environmental Research Institute at Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, Lijia Guo, Bay Area Environmental Research Institute at Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Yi-Min Huang, Princeton University, Princeton Plasma Physics Laboratory, Princeton, NJ, United States, Hardi Peter, Max Planck Institute for Solar System Research, Göttingen, Germany and Amitava Bhattacharjee, Princeton Plasma Physics Laboratory, Princeton University, Princeton, NJ, United States
Constraints on active region coronal heating properties from observations and modeling of chromospheric, transition region, and coronal emission (288945)
Paola Testa, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Vanessa Polito, Bay Area Environmental Research Institue, Moffett Field, United States, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Mats Carlsson, University of Oslo, Rosseland Centre for Solar Physics, Institute of Theoretical Astrophysics, Oslo, Norway, Fabio Reale, University of Palermo, Dipartimento di Fisica & Chimica, Palermo, Italy, Joel C Allred, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Viggo Haraldson Hansteen, Inst Theoretical Astrophysics, Oslo, Norway
Energy release from a stream of infalling prominence debris on 2011 September 7-8 (286889)
Andrew R Inglis, Catholic University of America, Washington, United States, Holly Robin Gilbert, National Center for Atmospheric Research, Boulder, United States and Leon Ofman, NASA GSFC/CUA, Greenbelt, United States
ALMA Discovery of Solar Umbral Brightness Enhancement at λ = 3 mm (219206)
Kazumasa Iwai, Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, Maria Loukitcheva, New Jersey Institute of Technology, Edison, NJ, United States, Masumi Shimojo, NAOJ, Mitaka, Tokyo, Japan, Sami K Solanki, Max Planck Institute for Solar System Research, Göttingen, Germany and Stephen M White, AFRL, Kirtland AFB, NM, United States
I. Jet Formation and Evolution due to 3D Magnetic Reconnection (240983)
José Juan González, Universidad Nacional Autónoma de México, Instituto de Geofísica, Unidad Michoacán, Morelia, Mexico, Francisco Guzmán, Universidad Michoacana de San Nicolás de Hidalgo, Instituto de Física y Matemáticas, Morelia, Mexico, Viktor Fedun, The University of Sheffield, School of Electrical and Electronic Engineering, Sheffield, United Kingdom, Gary Verth, University of Sheffield, School of Mathematical and Physical Sciences, Sheffield, United Kingdom, Sergiy Shelyag, Deakin University, Newcastle-Upon-Tyne, Australia and Stephane Regnier, Northumbria University, Newcastle-Upon-Tyne, United Kingdom

See more of: SPA-Solar and Heliospheric Physics