Three-dimensional polarimetric imaging of coronal mass ejections

Science

Volumn 305, Issue 5680, 2004, Pages 66-70

  Moran, Thomas G ^a,b   Davila, Joseph M ^a  

^a NASA GODDARD SPACE FLIGHT CENTER   (United States)

^b CATHOLIC UNIVERSITY OF AMERICA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

IMAGING TECHNIQUES; LIGHT POLARIZATION; POLARIMETERS; SPACECRAFT; SPECTROMETRY;

CORONAGRAPHS; THREE-DIMENSIONAL STRUCTURES;

ELECTRIC CORONA;

SOLAR ACTIVITY;

ARTICLE; CORONAL MASS EJECTION; IMAGE ANALYSIS; MAGNETIC FIELD; MAGNETISM; PHENOMENOLOGY; POLARIZATION; PRIORITY JOURNAL; SOLAR ENERGY; SPACE FLIGHT; SPECTROMETRY; STRUCTURE ANALYSIS; THREE DIMENSIONAL IMAGING; THREE DIMENSIONAL POLARIMETRIC IMAGING;

EID: 3042752564     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1098937     Document Type: Article

References (13)

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13. This work was carried out at the SOHO Experimenter's Analysis Facility at NASA Goddard Space Flight Center. The SOHO/LASCO data used here were produced by a consortium of the U.S. Naval Research Laboratory, Max-Planck-Institut fuer Aeronomie (Germany), Laboratoire d'Astronomie (France), and the University of Birmingham (United Kingdom). SOHO is a project of international cooperation between the European Space Agency and NASA. B. Fleck made useful suggestions for improving this manuscript. This research was funded through NASA grant number 10307.