SH41C:
Solar and Heliospheric Physics: General Contributions II Posters


Submit an Abstract to this Session


Session ID#: 43670

Session Description:
Contributions to this session highlight the latest scientific results relevant to solar and heliospheric physics that do not fall within the purview of other focused sessions at the fall AGU meeting.
Primary Convener:  J Todd Hoeksema, Stanford University, Stanford, CA, United States
Conveners:  Anthony J Mannucci, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States and Elizabeth MacDonald, Aurorasaurus, NASA Goddard Space Flight Center, Greenbelt, United States
Primary Liaison:  J Todd Hoeksema, Stanford University, HEPL, Stanford, CA, United States
Chairs:  J Todd Hoeksema, Stanford University, HEPL, Stanford, CA, United States and Anthony J Mannucci, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
OSPA Liaison:  J Todd Hoeksema, Stanford University, HEPL, Stanford, CA, United States

Cross-Listed:
  • SA - SPA-Aeronomy
  • SM - SPA-Magnetospheric Physics
Index Terms:

7599 General or miscellaneous [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7899 General or miscellaneous [SPACE PLASMA PHYSICS]
7999 General or miscellaneous [SPACE WEATHER]

Abstracts Submitted to this Session:

New developments and applications of Helioviewer Project services (411331)
Kirill Gennadevich Vorobyev, ADNET Systems Inc. Lanham, Lanham, MD, United States, Jack Ireland, ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States and Dr. Rachel Connolly, PhD, WGBH, Boston, MA, United States
The method for the detection and energy derivation of nano-flares based on deep learning (365181)
Toshiki Kawai, Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan and Shinsuke Imada, Nagoya University, ISEE, Nagoya, Japan
A Statistical Analysis of X-Ray Bursts Using Mutual Information (420822)
Jesse Michael Snelling1, Jay Johnson2, Jacob Willard1 and Simon Wing3, (1)Andrews University, Berrien Springs, MI, United States, (2)Andrews University, Berrien Springs, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Faint solar X-rays observed with NuSTAR (407738)
Iain G Hannah, University of Glasgow, Glasgow, United Kingdom, Brian Grefenstette, Space Radiation Laboratory, Pasadena, United States, Lindsay Glesener, University of Minnesota Twin Cities, Minneapolis, United States, Sam Krucker, ETH Zürich, Zurich, Switzerland, David Smith, University of California Santa Cruz, Santa Cruz, CA, United States, Hugh S Hudson, UC Berkeley, Space Sciences Lab, Berkeley, United States, Stephen M White, Air Force Research Laboratory Albuquerque, Albuquerque, NM, United States and Matej Kuhar, University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland
The Prevalence of O IV Density Diagnostics in UV Burst Spectra (411086)
Amanda Bacon, Bennington College, Bennington, VT, United States, Chad Allen Madsen, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States and Edward DeLuca, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
Dynamical Properties of He II EUV Surges that are Components of Solar Active Region Coronal Jets (393315)
Sabrina A Hernandez, Rice University, Houston, TX, United States, Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States, Ronald Lee Moore, NASA MSFC, Huntsville, United States and David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States
Magnetic Flux Emergence, Interchange Reconnection, Flux Cancellation, and Blow-out Eruptions in a Small Coronal Hole (419963)
Mitzi Adams, NASA Marshall Space Flight Center, ST13, Huntsville, AL, United States, Ron L Moore, National Space Science and Technology Center, Huntsville, AL, United States and Navdeep Kaur Panesar, NASA MSFC, Huntsville, AL, United States
Fine Structures and Rotational Motions of an Erupting Solar Quiescent Filament (366851)
Qiao Song, National Center for Space Weather, China Meteorological Administration, Beijing, China and Shuhong Yang, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
Dependence of heating of active region coronal loops on their photospheric magnetic setting (371418)
Ronald Lee Moore1, Sanjiv K Tiwari2, Julia K Thalmann3, Navdeep Kaur Panesar4 and Amy R Winebarger4, (1)University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)Institute for Physics/IGAM, University of Graz, Graz, Austria, (4)NASA Marshall Space Flight Center, Huntsville, AL, United States
Photospheric Magnetic Polarity of the Brightest Coronal Loops in a Solar Active Region (397425)
Ulric Baptiste II, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, Sanjiv K. Tiwari, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, Navdeep Kaur Panesar, NASA MSFC, Huntsville, AL, United States and Ronald Lee Moore, NASA MSFC, Huntsville, United States
Where is the strongest field located in sunspots ? - A statistical analysis using Hinode/Spectro-Polarimeter - (395229)
Joten Okamoto, NAOJ National Astronomical Observatory of Japan, NAOJ Chile Observatory, Tokyo, Japan and Takashi Sakurai, NAOJ, Mitaka, Japan
3-D Simulation Study of the Spreading/Elongation of Ribbons in Two-Ribbon Flares (375459)
Milton Arencibia, West Virginia University, Morgantown, WV, United States, Paul Cassak, West Virginia University, Department of Physics and Astronomy, Morgantown, United States, Jiong Qiu, Montana State University, Department of Physics, Bozeman, MT, United States, Dana Longcope, Montana State University Bozeman, Bozeman, United States and Eric R Priest, University of Saint Andrews, School of Mathematics and Statistics, Saint Andrews, United Kingdom
Si IV Resonance Line Emission During Solar Flares: NLTE radiation transfer simulations (410426)
Dr. Graham Stewart Kerr, PhD1, Mats Carlsson2, Joel C Allred3, Peter Young4 and Adrian Nigel Daw1, (1)NASA Goddard Space Flight Center, Greenbelt, United States, (2)University of Oslo, Rosseland Centre for Solar Physics, Institute of Theoretical Astrophysics, Oslo, Norway, (3)NASA GSFC, Solar Physics Lab, Greenbelt, United States, (4)George Mason University Fairfax, Fairfax, VA, United States
SDO/EVE Observations of Lyman Continuum Emission During Solar Flares (436859)
Ryan O Milligan, University of Glasgow, Glasgow, G12, United Kingdom, Marcos Machado, Comisión Nacional de Actividades Espaciales, Buenos Aires, Argentina and Paulo Jose de Aguiar Simoes, Presbyterian Mackenzie University, Sao Paulo, Brazil
Microwave Brightness Variation along a Loop during a Solar Flare (459272)
Sujin Kim, Korea Astronomy and Space Science Institute, Daejeon, South Korea
Observation of Quiet Limb in He I 1083.0 nm, H Paschen alpha1281.8 nm and H Brackett gamma 2166.1 nm lines (430208)
Debi Prasad Choudhary, California State University Northridge, Department of Physics and Astronomy, Northridge, CA, United States
A Comparison of On-Disk Plume and Non-Plume Regions with the Interface Region Imaging Spectrograph and the Solar Dynamics Observatory (448065)
Ellis A Avallone, University of Hawaii, Institute of Astronomy, Honolulu, CA, United States, Sanjiv K. Tiwari, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States and Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Evaluating the Performance of a Non-LTE Archive for Fast Inversion of Chromospheric Spectra (419736)
Chantelle Luise Kiessner, University of Hawaii at Hilo, Physics and Astronomy, Hilo, HI, United States, Christian Beck, National Solar Observatory, Makawao, United States and Sanjay Gosain, National Solar Observatory, Boulder, CO, United States
Constraints of temperature and density of plasma in non-equilibrium ionization state (465372)
Jin-Yi Lee, Kyung Hee University, Yongin, Korea, Republic of (South), John Raymond, Harvard Smithsonian Center for Astrophysics, Cambridge, MA, United States, Katharine Reeves, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States, Chengcai Shen, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States and Yong-Jae Moon, School of Space Research, Kyung Hee University, Yongin, South Korea
He II 304 Å proxy for magnetic field properties in far-side complex topologies (448805)
Ignacio Ugarte-Urra, US Naval Research Laboratory, Space Science Division, Washington, DC, United States, Lisa Upton and Harry P Warren, Naval Research Laboratory, Washington, DC, United States
Enhancing Solar Observations from GOES-R: Derived Products from the Extreme Ultraviolet and X-Ray Irradiance Sensors (EXIS) and Solar Ultraviolet Imager (SUVI) (439653)
Margaret Tilton, Cooperative Institute for Research in Environmental Sciences, Boulder, CO, United States, Jonathan Darnel, NOAA, Boulder, CO, United States, Janet L Machol, CU/CIRES-NOAA/NCEI, Boulder, United States, William Floyd Rowland, University of Colorado Boulder, Boulder, CO, United States and Daniel B Seaton, Southwest Research Institute, Boulder, CO, United States
A Hydrodynamic Model for Solar Acoustic Wave Propagation (465435)
John T Stefan, New Jersey Institute of Technology, Department of Physics, Edison, NJ, United States and Alexander G Kosovichev, New Jersey Institute of Technology, Physics, Newark, United States
Properties of sunspot oscillations and wave propagation in NOAA AR 12470 as observed with ALMA and BBSO instruments (455593)
Yi Chai1, Dale E Gary2, Bin Chen3, Kevin Reardon4, Gregory D Fleishman2 and Vasyl Yurchyshyn5, (1)New Jersey Institute of Technology, Edison, NJ, United States, (2)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, (3)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Edison, NJ, United States, (4)National Solar Observatory, Tucson, AZ, United States, (5)Big Bear Solar Observatory, Big Bear City, CA, United States
Statistical studies of Equatorial Coronal Holes and Active Regions during the maximum phase of four Solar Cycles. (384459)
Mahendra Lal Karna, Retired, Janakpur Dham, Nepal and Nishu Karna, Center for Astrophysics, Harvard & Smithsonian, Cambridge, United States
Using NOAA and Mount Wilson Observatory Sunspot Data to Investigate the Impact of Joy's Law Tilt on Simulations of Solar Cycle 22 with the Advective Flux Transport Model (388464)
Blaire Ness, Stony Brook University, Stony Brook, NY, United States and Lisa Upton, SSRC, Alexandria, United States
Closing the Book on Solar Cycle 24 (449534)
J Todd Hoeksema, Stanford University, Stanford, CA, United States
Plage areas from seven historical Ca II K archives (468336)
Theodosios Chatzistergos1,2, Ilaria Ermolli3, Natalie Krivova2 and Sami K Solanki2, (1)INAF Osservatorio Astronomico di Roma, Rome, Italy, (2)Max Planck Institute for Solar System Research, Göttingen, Germany, (3)Istituto Nazionale di Astrofisica Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy
Synergy of observations and dynamo models to understand and predict solar activity cycles (452012)
Irina Kitiashvili, NASA Ames Research Center, Moffett Field, CA, United States
Predicting Sunspot Cycle 25 Using a Data Driven Solar Magnetic Field Simulations of Century Scale (434022)
Prantika Bhowmik, University of Durham, Durham, United Kingdom and Dibyendu Nandy, Indian Institute of Science Education and Research Kolkata, Center of Excellence in Space Sciences India and Department of Physical Sciences, Kolkata, India

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