SH023
Solar and Heliospheric Physics: General Contributions

Session ID#: 72655

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.
Index Terms:

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

Primary Convener:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
Conveners:  Elizabeth MacDonald, National Aeronautics and Space Administration, Minneapolis, MN, United States and Romina Nikoukar, Johns Hopkins Applied Physics Laboratory, Laurel, MD, United States
Primary Liaison:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
 
Changing linear polarization properties in the dust tail of comet C/2012 S1 (ISON) (485738)
William T Thompson, ADNET Systems Inc. Greenbelt, Greenbelt, MD, United States
 
The Earth's axial tilt is 23.84 degrees. Thus, empirically-researched and published reports of such as 23.40 degrees are incorrectly reported. The standard international system of measure for Time is included in this mathematical proof. (486257)
Michael Anthony Norton, Retired, Washington, DC, United States
 
Re-analysis of the Wolfer Group Number Backbone (487048)
Leif Svalgaard, Stanford University, Stanford, CA, United States
 
Plasma structure of the deep solar interior (489467)
Robert Dean Loper Jr, Air Force Institute of Technology, Dept of Engineering Physics, Wpafb, OH, United States
 
The Emergence of Weakly Twisted Flux Ropes Without Convection (491473)
Kalman Joshua Knizhnik, US National Research Council of the National Academies, Washington, DC, United States, James Edward Leake, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Mark Linton, US Naval Research Laboratory, Washington, DC, United States
 
Heating Features of Interesting Supra-arcade Downflows (491484)
Zhuofei Li, Nanjing University, Nanjing, China, DeOndre Kittrell, Morgan State University, Physics, Baltimore, MD, United States, Katharine Reeves, Smithsonian Institution, Cambridge, MA, United States, Mark Weber, Smithsonian Astrophys Observ, Cambridge, MA, United States, David E. McKenzie, NASA Marshall Space Flight Center, Huntsville, AL, United States and Michael Freed, Montana State University, Bozeman, MT, United States
 
Perpendicular heating or apparent heating? Preparing Helios E2 magnetic field observations for wave particle interaction simulations (492883)
Duncan Keilbach1, Verena Heidrich-Meisner1, Jan Steinhagen1, Lars Berger2 and Robert F Wimmer-Schweingruber3, (1)University of Kiel, Kiel, Germany, (2)Institute for Experimental and Applied Physics (IEAP), Christian-Albrechts-University of Kiel, Kiel, Germany, (3)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
 
Primary and Secondary Solar Polar Crown PILs over Five Solar Cycles (493377)
Barbara A Emery-Geiger1, David F Webb2, Sarah E Gibson3, Ian McDonald Hewins1, Robert McFadden1 and Thomas A Kuchar2, (1)ISR, Boston College at HAO/NCAR, Boulder, CO, United States, (2)Boston College, ISR, Chestnut Hill, MA, United States, (3)NCAR, HAO, Boulder, CO, United States
 
Study of solar radio spikes properties observed at frequencies 0.01-8.4 GHz (495688)
Gilberto Armando Casillas-Perez, Universidad Nacional Autonoma de Mexico, Instituto de Geofisica, Mexico City, Mexico, Solai Jeyakumar, Universidad de Guanajuato, Departamento de Astronomia, Guanajuato, Mexico, Roman Perez-Enriquez, UNAM, Queretaro, Mexico and Armando Carrillo-Vargas, Instituto de Geofisica, Ciencias Espaciales, Morelia, Michoacan, Mexico
 
The Sensitivity of AIA Observations to Coronal Heating Parameters (496825)
Samuel Schonfeld, Universities Space Research Association Greenbelt, Greenbelt, MD, United States and James A Klimchuk, NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States
 
First Detection of Plasmoids from Breakout Reconnection (499137)
Pankaj Kumar1, Judy Karpen1, Spiro K Antiochos1, Peter Fraser Wyper2 and C Richard DeVore1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Durham, Durham, United Kingdom
 
Coronal Origins of the Alfvénic Slow Solar Wind (499834)
Olga Panasenco, Advanced Heliophysics, Pasadena, CA, United States, Marco Velli, University of California Los Angeles, Los Angeles, CA, United States and Raffaella D'Amicis, INAF-Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy
 
Diagnostics of nanoflare heating in active region core loops from chromospheric and transition region observations and modeling (499850)
Paola Testa1, Vanessa Polito1, Bart De Pontieu2, Fabio Reale3 and David Graham4, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)University of Palermo, Dipartimento di Fisica & Chimica, Palermo, Italy, (4)Bay Area Environmental Research Institute Moffett Field, Moffett Field, CA, United States
 
The Evolution of Solar Coronal Holes Over Two Solar Cycles (500348)
Larisza D Krista, University of Colorado at Boulder, CIRES, Boulder, CO, United States; NOAA, NCEI, Boulder, CO, United States
 
Why Are Solar Filaments Filamentary? (502710)
Gwang-Son Choe1, Inhyeok Song2, Sibaek Yi1 and Hongdal Jun1, (1)Kyung Hee University, School of Space Research, Yongin, Korea, Republic of (South), (2)Kyung Hee University, School of Space Research, Yongin, South Korea
 
Solar Cycle 25 Consensus Prediction Update (502832)
Douglas Alan Biesecker, NOAA Boulder, Boulder, CO, United States, Lisa Upton, Space Systems Research Corporation, Alexandria, VA, United States and Solar Cycle 25 Prediction Panel Team
 
Proton-proton collisional age as a tracer for solar wind type (505796)
Verena Heidrich-Meisner, University of Kiel, Kiel, Germany, Lars Berger, Institute for Experimental and Applied Physics (IEAP), Christian-Albrechts-University of Kiel, Kiel, Germany and Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
 
The solar wind speed – expansion factor (v - fs) relationship at the inner boundary (18 R⊙) of the heliosphere (506404)
Kan Liou, JHU/Applied Physics Lab, Laurel, MD, United States, Chin-Chun Wu, Naval Research Lab DC, Washington, DC, United States and Harry Warren, Naval Research Laboratory, Washington, DC, United States
 
Magnetic Field Intensity Modification to Force Free Model of Magnetic Clouds: Wind Examples since Launch (507375)
Chin-Chun Wu, US Naval Research Laboratory, Washington, DC, United States, Ronald P Lepping, NASA Goddard Space Flight Center, Emeritus, Greenbelt, MD, United States and Daniel Benjamin Berdichevsky, Berdichevsky Daniel B, Greenbelt, MD, United States
 
The SOHO/EIT solar flare catalog (510168)
Sumanth Rotti and Petrus C Martens, Georgia State University, Physics and Astronomy, Atlanta, GA, United States
 
Critical Parameters of Photospheric Magnetic Field to Produce Eruptive Flares in Solar Active Regions (510799)
Pei Hsuan Lin1, Kanya Kusano1, Daikou Shiota2, Satoshi Inoue1, K D Leka1,3 and Yuta Mizuno1, (1)Nagoya University, ISEE, Nagoya, Japan, (2)National Institute of Information and Communications Technology, Tokyo, Japan, (3)NorthWest Research Associates Boulder, Boulder, CO, United States
 
Estimating the temperature and density of a spicule from 100 GHz data obtained with ALMA (513771)
Masumi Shimojo, National Astronomical Observatory of Japan, Tokyo, Japan, Tomoko Kawate, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan, Takenori J. Okamoto, National Astronomical Observatory of Japan, Mitaka, Tokyo, Japan and Takaaki Yokoyama, University of Tokyo, Department of Earth and Planetary Science, Bunkyo-ku, Japan
 
A Study of Equatorial Coronal Holes during the Maximum Phase of Four Solar Cycles (516584)
Nishu Karna, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, Mahendra Lal Karna, Retired, Janakpur Dham, Nepal, Steven H. Saar, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, William Dean Pesnell, NASA / GSFC, Greenbelt, MD, United States and Edward DeLuca, SAO, Cambridge, MA, United States
 
On the emission region of Type II Radio Bursts in interplanetary shock fronts (517372)
Ernesto Aguilar-Rodriguez, Universidad Nacional Autonoma de Mexico, Instituto de Geofisica, Unidad Michoacan, Morelia, Mexico and Pedro Corona-Romero, CONACyT - Servicio de Clima Espacial Mexico - Laboratorio Nacional de Clima Espacial, SCiESMEX – LANCE, Morelia, Mexico
 
Fine-scale explosive energy release at sites of magnetic flux cancellation in the core of the solar active region observed by Hi-C 2.1, IRIS and SDO (518850)
Sanjiv K Tiwari1, Navdeep Kaur Panesar2, Ronald Lee Moore3, Bart De Pontieu1, Amy R Winebarger4 and HiC-2.1 Science Team, (1)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, AL, United States, (3)NASA MSFC, Huntsville, AL, United States, (4)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
Onset of the Magnetic Explosion in On-disk Solar Coronal Jets (519554)
Navdeep K. Panesar, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Ronald Lee Moore, NASA MSFC, Huntsville, AL, United States and Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States
 
Further Evidence for Magnetic Flux Cancelation as the Build-up and Trigger Mechanism for Eruptions in Isolated Solar Active Regions (521249)
Amelia Buell, University of Alabama in Huntsville, Huntsville, AL, United States, Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States, Ronald L Moore, NASA Marshall Space Flight Center, Huntsville, United States and David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States
 
Using Ephemeral Coronal Holes to Validate the SPOCA Database of Coronal Holes (522115)
William Dean Pesnell1, Niraj Pant2, Michael S Kirk1 and Andrew R Inglis2, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic University of America, Washington, DC, United States
 
A Two-Sided-Loop X-Ray Solar Coronal Jet and a Sudden Photospheric Magnetic-field Change, Both Driven by a Minifilament Eruption (524204)
Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States, Louise K Harra, ETH Zurich, Zurich, Switzerland; PMOD WRC Physical Meteorological Observatory Davos and World Radiation Center, Davos Dorf, Switzerland, Ronald Lee Moore, NASA MSFC, Huntsville, AL, United States and David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States
 
Time dependent properties of Inverse Evershed Flow and Perspectives with Daniel K. Inouye Solar Telescope (DKIST) (529098)
Debi Prasad Choudhary, California State University Northridge, Northridge, CA, United States and Christian Beck, National Solar Observatory, Boulder, CO, United States
 
Optical observation of neutral helium distribution in interplanetary space by Hisaki satellite (535034)
Atsushi Yamazaki1, Go Murakami1, Kazuo Yoshioka2, Tomoki Kimura3, Fuminori Tsuchiya4, Masato Kagitani4, Takeshi Sakanoi4, Naoki Terada5, Yasumasa Kasaba5, Ichiro Yoshikawa2 and Hisaki (SPRINT-A) Project team, (1)JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan, (2)The University of Tokyo, Tokyo, Japan, (3)Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai, Japan, (4)PPARC, Tohoku University, Sendai, Japan, (5)Tohoku University, Sendai, Japan
 
Solar oblateness variations in phase with the 22 year-magnetic cycle (536893)
Abdanour Irbah, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France and Luc Damé, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France
 
New Elliptical Flux Tube Model to Explain Sunspot Oscillations (539836)
Anwar Ali Aldhafeeri, University of Sheffield, Sheffield, United Kingdom, Viktor Fedun, The University of Sheffield, Sheffield, United Kingdom, David B Jess, Queen's University Belfast, School of Mathematics and Physics, Belfast, United Kingdom, Wernher Brevis, Pontificia Universidad Catolica de Chile, Santiago, Chile and Gary Verth, University of Sheffield, School of Mathematics and Statistics, Sheffield, S10, United Kingdom
 
Solar Sources of Coronal Mass Ejections (545000)
Sachiko Akiyama1, Nat Gopalswamy2, Seiji Yashiro1 and G. (Grzegorz Joze) Michalek3, (1)Catholic University of America, Washington, DC, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States, (3)Astronomical Observatory of Jagiellonian University, Krakow, Poland
 
Center-to-Limb Variation of the polarization of Mg II h & k lines as measured by CLASP2 (547426)
Laurel Rachmeler1, David E. McKenzie1, Ryohko Ishikawa2, Ryouhei Kano2, Javier Trujillo Bueno3, Ken Kobayashi1, Donguk Song2, Masaki Yoshida2, Frederic Auchere4 and Joten Okamoto2, (1)NASA Marshall Space Flight Center, Huntsville, AL, United States, (2)NAOJ National Astronomical Observatory of Japan, Tokyo, Japan, (3)Instituto Astrofísica Canarias, La Laguna - Tenerife, Spain, (4)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France
 
Modeling the onset of solar eruptions in active regions (548076)
James Edward Leake1, Mark Linton2, Spiro K Antiochos3 and Peter W Schuck3, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)US Naval Research Laboratory, Washington, DC, United States, (3)NASA GSFC, Silver Spring, MD, United States
 
Examination of Separator Reconnection Rates in a Series of Adjacent Emerging/Existing Active Region Pairs (550362)
Marika McCarthy, Montana State University, Bozeman, MT, United States, Dana W Longcope, Montana State University Bozeman, Bozeman, MT, United States, Anna V Malanushenko, LMSAL, Palo Alto, CA, United States and David E. McKenzie, NASA Marshall Space Flight Center, Huntsville, AL, United States
 
Cradle-to-Grave Evolution and Explosiveness of the Magnetic Field from Bipolar Ephemeral Active Regions (BEARs) in Solar Coronal Holes (552559)
Caroline Nagib, University of California Los Angeles, Astronomy and Astrophysics, Los Angeles, CA, United States, Navdeep K. Panesar, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Ronald L Moore, NASA Marshall Space Flight Center, Huntsville, United States and Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States
 
The Chromospheric Layer Spectro-Polarimeter (CLASP2) Sounding Rocket Mission: First Results (555414)
David E. McKenzie1, Ryohko Ishikawa2, Javier Trujillo Bueno3, Frederic Auchere4, Laurel Rachmeler1, Ryouhei Kano2, Donguk Song2, Joten Okamoto2, Ken Kobayashi1 and Masaki Yoshida2, (1)NASA Marshall Space Flight Center, Huntsville, AL, United States, (2)NAOJ National Astronomical Observatory of Japan, Tokyo, Japan, (3)Instituto Astrofísica Canarias, La Laguna - Tenerife, Spain, (4)IAS Institut d'Astrophysique Spatiale, Orsay Cedex, France
 
Spicule jets in the chromosphere-corona interface modeled with resistive MHD with thermal conductivity (556041)
José Juan González, CONACyT - Servicio de Clima Espacial Mexico - Laboratorio Nacional de Clima Espacial, SCiESMEX – LANCE, Instituto de Geofísica, Unidad Michoacán, UNAM, Morelia, Mexico, Francisco Guzmán, Universidad Michoacana de San Nicolás de Hidalgo, Instituto de Física y Matemáticas, Morelia, Mexico, Viktor Fedun, The University of Sheffield, Sheffield, United Kingdom and Gary Verth, University of Sheffield, School of Mathematics and Statistics, Sheffield, S10, United Kingdom
 
Realistic, three-dimensional sensitivity kernels for measuring solar interior flows (556206)
Thomas Hartlep, Bay Area Environmental Research Institute, Moffett Field, CA, United States and Junwei Zhao, Stanford Univ, HEPL, Stanford, CA, United States
 
Progression of Solar Cycle 24 As Seen in Acoustic Mode Frequencies of the Sun (557092)
Brianna Undzis1, Sushanta C Tripathy2 and Kiran Jain2, (1)University of Illinois at Urbana Champaign, Urbana, IL, United States, (2)National Solar Observatory, Tucson, AZ, United States
 
Developing Fast Solar Wind Modeling with EUHFORIA (560730)
Evangelia Samara1,2, Jasmina Magdalenic3, Luciano Rodriguez3, Stephan G. Heinemann4 and Stefaan Poedts2, (1)Observatoire Royal de Belgique, Brussel, Belgium, (2)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium, (3)SIDC, Royal Observatory of Belgium, Brussels, Belgium, (4)University of Graz, Institute of Physics, Graz, Austria
 
NuSTAR observations of the quietest Sun (574482)
Iain G Hannah, University of Glasgow, Glasgow, G12, United Kingdom, Kristopher Cooper, University of Glasgow, Glasgow, United Kingdom, Brian Grefenstette, Space Radiation Laboratory, Pasadena, CA, United States, Lindsay Glesener, University of Minnesota, Twin Cities, MN, United States, Sam Krucker, UC Berkeley, Space Science Lab, Berkeley, CA, United States, David Miles Smith, Univ of California Santa Cruz, Santa Cruz, CA, United States, Hugh S Hudson, UC Berkeley, Space Sciences Lab, Berkeley, CA, United States, Stephen M White, Air Force Research Laboratory, Albuquerque, NM, United States and Matej Kuhar, University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland
 
Analysis of Voyager 1 Magnetic Field Data From 1977 to 1990 (579050)
Renier Adriaan Burger, North-West University, Mahikeng, South Africa and Sarah R McKee, North-West University, Physics, Potchefstroom, South Africa
 
Evolution of Microwave blob observed by Nobeyama Radioheliogrph (580659)
Sujin Kim, Korea Astronomy and Space Science Institute (KASI), Daejeon, South Korea
 
Temporal relations between total solar irradiance and photometric indices during the last two solar cycles. (580719)
Ana Cristina Cadavid1, Debi Prasad Choudhary2, Gary A Chapman1 and Angie Cookson1, (1)California State University Northridge, Northridge, CA, United States, (2)California St Univ Northrigde, Northridge, CA, United States
 
Are the brightest coronal loops always rooted in mixed-polarity magnetic flux? (583452)
Caroline Evans, Organization Not Listed, Washington, DC, United States, Sanjiv K. Tiwari, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, Navdeep K. Panesar, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Avijeet Prasad, University of Alabama in Huntsville, Huntsville, United States and Ronald Lee Moore, NASA MSFC, Huntsville, AL, United States
 
Tracking supergranulation near the poles with SDO/HMI (586423)
Raphael Attié1, Michael S Kirk1, Benoit Tremblay2, Karin Muglach3, Shea A. Hess Webber4, William Dean Pesnell5 and Barbara J Thompson6, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Montreal, Physics department, Montreal, QC, Canada, (3)Catholic University of America, Washington, DC, United States, (4)Stanford University, HEPL, Stanford, CA, United States, (5)NASA / GSFC, Greenbelt, MD, United States, (6)NASA/GSFC, Greenbelt, MD, United States
 
The Effect of Lorentz Stresses on the Solar Frequency Spectrum: The Forward Problem. (587050)
Srijan Bharati Das1, Tuneer Chakraborty2, Shravan Hanasoge2 and Jeroen Tromp1, (1)Princeton University, Princeton, NJ, United States, (2)Tata Institute of Fundamental Research, Mumbai, India
 
Searching for a Boundary Layer as a Source of the Slow Solar Wind (588184)
Yuan-Kuen Ko, US Naval Research Laboratory, Washington, DC, United States, Karin Muglach, Catholic University of America, Washington, DC, United States, Pete Riley, Predictive Science Inc., San Diego, CA, United States and Yi-Ming Wang, Naval Research Lab, Washington, DC, United States
 
Calculating the Emission Measure and Average Weighted Temperature of Supra-Arcade Downflows (595866)
DeOndre Kittrell1, Zhuofei Li2, Katharine Reeves3 and Mark Weber3, (1)Morgan State University, Physics, Baltimore, MD, United States, (2)Nanjing University, Nanjing, China, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
 
Radial variation in energetic ion composition from 1 AU to the Termination Shock (596643)
J. Douglas Patterson and Jerry Wayne Manweiler, Fundamental Technologies, LLC, Lawrence, KS, United States
 
Ellerman bombs and UV bursts: reconnection at different atmospheric layers (597906)
Viggo Haraldson Hansteen1, Ada N Ortiz-Carbonell, Daniel Elias Nobrega3 and Luc Rouppe van der Voort3, (1)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, (2)University of Oslo, Oslo, Norway
 
Properties of Delta Spots Observed with HMI (598483)
Aimee Ann Norton1, Kalman Joshua Knizhnik2, Mark Linton2 and Lucas Tarr3, (1)Stanford University, Stanford, CA, United States, (2)US Naval Research Laboratory, Washington, DC, United States, (3)Naval Research Laboratory, Washington, DC, United States
 
Solar Polar Brightening and Radius at 100 and 230 GHz Observed by ALMA (598738)
Caius Selhorst, Universidade Cruzeiro do Sul, NAT - Núcleo de Astrofísica, São Paulo, Brazil
 
Estimating the Visibility Function of Modern Coronagraphs (601689)
Laura Antonia Balmaceda, George Mason University Fairfax, Fairfax, United States, Hong Xie, Catholic University of America, Washington, DC, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and O C St Cyr, NASA GSFC, Greenbelt, MD, United States
 
A Catalogue of Coronal Mass Ejections Observed by the Heliospheric Imagers throughout the STEREO Mission (601900)
David Barnes, Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom
 
A CME-Producing Solar Eruption from the Interior of a Twisted Emerging Bipole (604480)
Mitzi Adams, NASA Marshall Space Flight Center, ST13, Huntsville, AL, United States, Ronald Lee Moore, NASA MSFC, Huntsville, AL, United States, Navdeep K. Panesar, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States and Sanjiv K. Tiwari, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States
 
Multi-spacecraft study of foreshock cavitons with Cluster (605615)
Reynaldo Vite, National Polytechnic Institute of Mexico, Mexico City, Mexico, Julio Cesar Villagran Orihuela, Instituto Politecnico Nacional, Mexico City, Mexico, Primoz Kajdic, UNAM National Autonomous University of Mexico, Department of Space Sciences, Mexico City, Mexico and Xochitl Blanco-Cano, UNAM, Mexico, Mexico
 
From Jets to CMEs: Observations of the Breakout Continuum (606408)
Judith T Karpen1, Pankaj Kumar1, Spiro K Antiochos1, Peter Fraser Wyper2 and C Richard DeVore1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Durham, Durham, United Kingdom
 
Constructing A Physically Motivated Model of Activity-Driven Solar and Stellar Radial Velocities (606638)
Anthony Iampietro, Millersville University of Pennsylvania, Millersville, PA, United States, Steven H. Saar, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, Raphaelle D Haywood, Harvard College Observatory, NASA Sagan Fellow, Cambridge, MA, United States and Timothy W. Milbourne, Harvard University, Department of Physics, Cambridge, MA, United States
 
Can superposition of evaporative flows explain broad IRIS Fe XXI line profiles during flares? (608592)
Vanessa Polito, Bay Area Environmental Research Institute Moffett Field, Moffett Field, CA, United States, Paola Testa, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States and Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
The Effect of Evolution on The Flare Activity of Solar Active Regions (618390)
Suman Kumar Dhakal1, Jie Zhang1 and Panditi Vemareddy2, (1)George Mason University, Fairfax, VA, United States, (2)Indian Institute of Astrophysics, Koramangala, Bengaluru, India
 
VLA Measurements of Faraday Rotation through a Coronal Mass Ejection Using Multiple Lines of Sight (625346)
Jason Earl Kooi, US Naval Research Laboratory, Washington, DC, United States, Madison L Ascione, Georgetown University, Department of Physics, Washington, DC, United States, Lianis V Reyes-Rosa, Fayetteville State University, Department of Chemistry, Physics, and Materials Science, Fayetteville, United States and Sophia K Rier, Bishop Ireton High School, Alexandria, United States
 
Solar Cycle-Related Variability of Sun-as-a-Star Spectral Line Profiles (627454)
Matt Kalscheur1, Serena Criscuoli2, Luca Bertello2 and Alexei A Pevtsov2, (1)University of Wisconsin Madison, Madison, WI, United States, (2)National Solar Observatory, Boulder, CO, United States
 
First Flight of the EUV Snapshot Imaging Spectrograph (628395)
Charles C Kankelborg1, Jacob Douglas Parker1, Roy Smart1, Amy R Winebarger2, Ken Kobayashi2, Hans Courrier1 and Laurel Rachmeler2, (1)Montana State University, Bozeman, MT, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
A Neural Network-based Data Analysis Technique for the EUV Snapshot Imaging Spectrograph (629420)
Roy Smart1, Charles C Kankelborg1, Jacob Douglas Parker1, Hans Courrier1, Amy R Winebarger2, Ken Kobayashi2 and Laurel Rachmeler2, (1)Montana State University, Bozeman, MT, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
A Preliminary Study of the Data From the ESIS/MOSES III Sounding Rocket Flight and Coordinating Observatories (630120)
Jacob Douglas Parker1, Charles C Kankelborg1, Roy Smart1, Hans Courrier1, Amy R Winebarger2, Ken Kobayashi2 and Laurel Rachmeler2, (1)Montana State University, Bozeman, MT, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
Discovery of Long-Period Magnetic Field Oscillations and Motions in Isolate Sunspot (630816)
ANA Belen Grinon MARIN, Stanford University, Stanford, CA, United States
 
The Signature of Explosive Events in the FUV Spectrum of the Sun as a Star (631562)
Catharine E. Bunn and Charles C Kankelborg, Montana State University, Bozeman, MT, United States
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