Solar Activity in Cycle 24 and Beyond: A Synergistic View from the Convection Zone to the Heliosphere II

Wednesday, 16 December 2015: 13:40-15:40
2011 (Moscone West)
Primary Conveners:  Irina Kitiashvili, NASA Ames Research Center, Moffett Field, CA, United States
Conveners:  Xudong Sun, Stanford University, Stanford, CA, United States, David H Hathaway, NASA Ames Research Center, Moffett Field, CA, United States and Pete Riley, Predictive Science Inc., San Diego, CA, United States
Chairs:  Irina Kitiashvili, NASA Ames Research Center, Moffett Field, CA, United States and Xudong Sun, Stanford University, Stanford, CA, United States
OSPA Liaisons:  David H Hathaway, NASA Marshall Space Flight Center, Huntsville, AL, United States
The Evolution of the Heliosphere Over Decades, Centuries and Millennia (Invited) (63315)
Mathew James Owens, University of Reading, Reading, RG6, United Kingdom, Michael M Lockwood, University of Reading, Reading, Berkshire, United Kingdom, Luke A Barnard, University of Reading, Reading, United Kingdom and Kenneth G McCracken, Organization Not Listed, Washington, DC, United States
Linking Stealthy Signatures of Coronal Mass Ejections at the Sun to 1 AU (75673)
Tamitha Lynne Mulligan, The Aerospace Corp, Los Angeles, CA, United States
Why is the Sun No Longer Accelerating Particles to High Energy in Solar Cycle 24? (75280)
Richard A Mewaldt1, Christina MS Cohen1, Gang Li2, Glenn M Mason3, Charles William Smith4, Tycho T von Rosenvinge5 and Angelos Vourlidas6, (1)California Institute of Technology, Pasadena, CA, United States, (2)University of Alabama in Huntsville, Huntsville, AL, United States, (3)JHU / APL, Laurel, MD, United States, (4)University of New Hampshire Main Campus, Durham, NH, United States, (5)NASA Goddard SFC, Greenbelt, MD, United States, (6)Applied Physics Laboratory Johns Hopkins, Space Department, Laurel, MD, United States
Modified Rossby Waves in the Solar Interior: The Need For A Solar Meteorology Mission (Invited) (58539)
Scott William Mcintosh, High Altitude Observatory, Boulder, CO, United States
Relationship Between Subsurface Flows and Magnetic Field Evolution in Solar Cycle 24 (76200)
Alexander G Kosovichev, New Jersey Institute of Technology, Department of Physics, Edison, NJ, United States and Junwei Zhao, Stanford University, Stanford, CA, United States
Contextualizing Solar Cycle 24: Report on the Development of a Homogenous Database of Bipolar Active Regions Spanning Four Cycles (Invited) (59136)
Andres Munoz-Jaramillo1,2, Zachary A Werginz3, Michael D DeLuca4, Juan Pablo Vargas-Acosta5, Dana W Longcope1, John W Harvey6, Piet Martens2, Jie Zhang7, Santiago Vargas-Dominguez5, Craig E DeForest8 and Derek A Lamb9, (1)Montana State University, Bozeman, MT, United States, (2)Georgia State University, Atlanta, GA, United States, (3)Saint Norbert College, De Pere, WI, United States, (4)University of Colorado at Boulder, Boulder, CO, United States, (5)Universidad Nacional de Colombia, Bogota, Colombia, (6)Natl Solar Observatory, Tucson, AZ, United States, (7)George Mason Univ, Fairfax, VA, United States, (8)Southwest Research Institute, Boulder, CO, United States, (9)Southwest Research Institute Boulder, Boulder, CO, United States
The Solar Non-activity Cycle of Polar Coronal Holes (73786)
Michael S Kirk1, William Dean Pesnell2 and C Alex Young1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)NASA / GSFC, Greenbelt, MD, United States
Photospheric and coronal magnetic fields in 1974 – 2015: A comparison of six magnetographs (81613)
Ilpo Virtanen, University of Oulu, Oulu, Finland and Kalevi Mursula, Univ Oulu, Oulu, Finland