SM51A:
Novel Instrument Techniques for Heliophysics: In Situ and Remote Sensing I Posters

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Session ID#: 12906

Session Description:
This session will focus on novel instrument techniques to observe the sun and geospace from the heliosphere to the interstellar media. Challenging science targets in the field of Heliophysics have been advanced by emerging technologies throughout the space era, and recent technological advances provides low-cost, low-power, light-weight, high-resolution, high-accuracy, and wide-dynamic range investigations that can enhance the technological capabilities and scientific closure of next generation missions. Abstracts are solicited that investigate and develop instruments or their fundamental subsystems for in-situ studies of particles (thermal, suprathermal to energetic plasmas ranging eV to MeV, and neutral gas including bulk features and mass spectrometry) and fields (electric and magnetic fields from low to high frequencies), and remote studies of energetic neutral atoms and photons (from the near infrared to x-rays).
Primary Convener:  Keiichi Ogasawara, Southwest Research Institute, San Antonio, TX, United States
Conveners:  Elizabeth MacDonald, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Michael Wayne Davis, Southwest Research Institute, San Antonio, TX, United States and John W Bonnell, University of California Berkeley, Berkeley, CA, United States
Chairs:  John W Bonnell, University of California Berkeley, Berkeley, CA, United States and Elizabeth MacDonald, NASA Goddard Space Flight Center, Greenbelt, MD, United States
OSPA Liaison:  Keiichi Ogasawara, Southwest Research Institute, San Antonio, TX, United States

Cross-Listed:
  • P - Planetary Sciences
  • SA - SPA-Aeronomy
  • SH - SPA-Solar and Heliospheric Physics
Index Terms:

2194 Instruments and techniques [INTERPLANETARY PHYSICS]
2494 Instruments and techniques [IONOSPHERE]
2794 Instruments and techniques [MAGNETOSPHERIC PHYSICS]
7594 Instruments and techniques [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Abstracts Submitted to this Session:

Giuseppe Romeo1, Robert K Schaefer2, Larry J Paxton3, Brian C Wolven3 and Orlando Romeo4, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (2)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (3)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (4)University of Maryland, College Park, College Park, United States
Edward DeLuca1, Jenna Samra2, Leon Golub1 and Peter Cheimets1, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, United States
Eder Cervantes Alcala1, Giora Guth1, Samuel Fedeler2, Jenna Samra3, Peter Cheimets1, Edward DeLuca1 and Leon Golub1, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)North Carolina State University Raleigh, Raleigh, NC, United States, (3)Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, United States
David Calvin Clark1, Edmund A Spencer2, Ravi Gollapalli1 and Brannon Kerrigan1, (1)University of South Alabama, Mobile, AL, United States, (2)University of South Alabama, Electrical and Computer Engineering, Mobile, AL, United States
Darren Chaddock1, Eric Donovan1, Emma Spanswick1, David J Knudsen1, Harald U Frey2, Kirsti Kauristie3, Noora Partamies4, Brian J Jackel1, Megan Gillies1 and Poul Erik Holmdahl Olsen5, (1)University of Calgary, Calgary, AB, Canada, (2)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)Finnish Meteorological Institute, Helsinki, Finland, (4)University Centre in Svalbard, Longyearbyen, Norway, (5)DTU Space, Lyngby, Denmark
Gian Domenic Andreone, University of Iowa, Physics and Astronomy, Iowa City, IA, United States and Jasper S Halekas, University of Iowa, Iowa City, IA, United States
Ashley Carlton1, Maria de Soria-Santacruz Pich2, Insoo Jun3, Wousik Kim4 and Kerri Cahoy1, (1)Massachusetts Institute of Technology, Cambridge, MA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, United States
David K Olson, Los Alamos National Laboratory, Los Alamos, NM, United States, Brian Larsen, The New Mexico Consortium, Los Alamos, NM, United States and Brian Phillip Weaver, Los Alamos National Laboratory, Los Alamos, United States
Jia Yu1, Robert F Wimmer-Schweingruber2, Christine Hellweg3, Thomas Berger3, Shenyi Zhang4, Soenke Burmeister1, Lars Seimetz2, Björn Schuster1, Stephan I Boettcher2, Hauke Woyciechowski1, Jingnan Guo5, Henning Lohf1 and Violetta Knierim6, (1)University of Kiel, Kiel, Germany, (2)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (3)German Aerospace Center DLR Cologne, Institute of Aerospace Medicine, Radiation Biology Department, Cologne, Germany, (4)NSSC National Space Science Center, CAS, Beijing, China, (5)University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, (6)IEAP, University of Kiel, Kiel, Germany
Jenna Lynn Zink, University of Texas at San Antonio, San Antonio, TX, United States, Frederic Allegrini, Southwest Research Institute, San Antonio, United States and Keiichi Ogasawara, Southwest Research Institute, San Antonio, TX, United States