CONFIGURATION OF THE INTERSTELLAR MAGNETIC FIELD NEAR THE HELIOSPHERE FROM POLARIZED STARLIGHT
CONFIGURATION OF THE INTERSTELLAR MAGNETIC FIELD NEAR THE HELIOSPHERE FROM POLARIZED STARLIGHT
Priscilla C Frisch1, Vilppu Piirola2, Andrei Berdyugin2, Antonio Mario Magalhaes3, Svetlana Berdyugina4, Caisey Harlingten5, Kym Hill6, Andrew Cole6, Sloane Wiktorowicz7, Daniel Cotton8, Jeremy Bailey9, Lucyna Kedziora-Chudczer9, J Marshall10, Kimberly Bott11, David J McComas12, Nathan Schwadron13, Herbert O Funsten14, Daiane Seriacopi3, Seth Redfield15, Carl Heiles16 and George Livadiotis17, (1)University of Chicago, Chicago, IL, United States, (2)University of Turku, Finnish Centre for Astronomy with ESO, Turku, Finland, (3)University de Sao Paulo, Inst. de Astronomia, Geofisica, Sao Paulo, Brazil, (4)Kiepenheuer Institute of Solar Physics, Freiburg, Germany, (5)University of Tasmania, Hobart, TAS, Australia, (6)University of Tasmania, Hobart, Australia, (7)The Aerospace Corporation, El Segundo, CA, United States, (8)University of New South Wells, Sydney, Australia, (9)University of New South Wells, Sydney, NSW, Australia, (10)Academia Sinica, Institute of Astronomy and Astrophysics, Taipei, Taiwan, (11)Virtual Planetary Laboratory, Seattle, WA, United States, (12)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (13)University of New Hampshire, Durham, NH, United States, (14)Los Alamos National Laboratory, Los Alamos, NM, United States, (15)Wesleyan University, Middletown, CT, United States, (16)University of California Berkeley, Berkeley, CA, United States, (17)Southwest Research Institute, San Antonio, TX, United States
