3D Reconstruction from SECCHI-EUVI Images Using an Optical-Flow Algorithm: Method Description and Observation of an Erupting Filament

Gissot, S.; Antoine, J.-P.; Hochedez, J.-F.; Chainais, P.

doi:10.1007/s11207-008-9270-0

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Home > Science Articles > Peer Reviewed Articles > 3D Reconstruction from SECCHI-EUVI Images Using an Optical-Flow Algorithm: Method Description and Observation of an Erupting Filament

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2008

Ref: SIDCimport-340

3D Reconstruction from SECCHI-EUVI Images Using an Optical-Flow Algorithm: Method Description and Observation of an Erupting Filament

Gissot, S. ; Hochedez, J.-F. ; Chainais, P. ; Antoine, J.-P.

published in Solar Physics, 252, pp. 397-408 (2008)

DOI: 10.1007/s11207-008-9270-0
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The record appears in these collections:
Royal Observatory of Belgium > Solar Physics & Space Weather (SIDC)
Science Articles > Peer Reviewed Articles
Solar-Terrestrial Centre of Excellence

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Record created 2016-02-22, last modified 2022-09-20

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