Primary Convener: Nicolas Lee, Stanford University, Aeronautics and Astronautics, Stanford, CA, United States
Conveners: Sean Hsu, University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, Richard Jerousek, University of Central Florida, Florida Space Institute, Orlando, FL, United States and Andrew R Poppe, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
Primary Liaison: Nicolas Lee, Stanford University, Aeronautics and Astronautics, Stanford, CA, United States
Chairs: Nicolas Lee, California Institute of Technology, Pasadena, CA, United States and Andrew R Poppe, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
OSPA Liaison: Nicolas Lee, California Institute of Technology, Pasadena, CA, United States
Pyrolysis of Meteoritic Organics and Fragmentation of Cosmic Dust during Atmospheric Entry (732866)
John M C Plane1, David Lawrence Bones2, Alexander D James2, Benjamin John Murray3, Juan Diego Carrillo-Sánchez4, Graham W Mann1 and Simon D A Connell5, (1)University of Leeds, Leeds, LS2, United Kingdom, (2)University of Leeds, School of Chemistry, Leeds, United Kingdom, (3)University of Leeds, Leeds, United Kingdom, (4)NASA Goddard Space Flight Center, Ionosphere-Thermosphere-Mesosphere Physics Lab (code 675), Greenbelt, MD, United States, (5)University of Leeds, School of Physics and Astronomy, Leeds, United Kingdom
Dust detection by antenna instruments: the effect of impact location (699359)
Ming-Hsueh Shen1,2, Zoltan Sternovsky1,2, Mihaly Horanyi2,3, Sean Hsu2 and David Malaspina2,4, (1)University of Colorado, Smead Aerospace Engineering Sciences Department, Boulder, CO, United States, (2)University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (3)University of Colorado, Physics Department, Boulder, CO, United States, (4)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, CO, United States
Characteristics of Ring Particles and Clumping in Peaks and Troughs of Density Waves from Cassini UVIS Ring Occultation Statistics (761736)
Stephanie Eckert1, Joshua E Colwell1, Larry W Esposito2, Richard Jerousek3 and Melody Green4, (1)University of Central Florida, Orlando, FL, United States, (2)Univ of Colorado, Boulder, CO, United States, (3)University of Central Florida, Florida Space Institute, Orlando, FL, United States, (4)University of Central Florida, Physics, Orlando, FL, United States
Temporally and azimuthally averaged mesoscale structures in Saturn's rings from Cassini UVIS occultations (734358)
Richard Jerousek, University of Central Florida, Florida Space Institute, Orlando, FL, United States, Lamia Benyamine, University of Central Florida, Physics, Orlando, FL, United States, Mark Lewis, Trinity University, Computer Sciences, San Antonio, TX, United States, Joshua E Colwell, University of Central Florida, Orlando, FL, United States, Matthew S Tiscareno, Carl Sagan Center for Study of life in the universe, Mountain View, CA, United States; SETI Institute, Mountain View, CA, United States and Klaus-Michael Aye, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States