Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
LMSAL
Univ. Maryland
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Department ADBS, Palo Alto, CA
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Department L9-41, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Department L9-41, Building 252, 3251 Hanover Street, Palo Alto, CA 94304 Goddard Space Flight Center, Greenbelt, MD; Colorado, University, Boulder; Zürich, Eidgenoessische Technische Hochschule, Zürich, Switzerland
NASA. Goddard Space Flight Center, Greenbelt, MD, US
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Organization ADBS, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
Solar and Astrophysics Laboratory, Lockheed Martin, Advanced Technology Center, 3251 Hanover St., Bldg. 252, Org, ADBS, Palo Alto, CA 94304, USA
Lockheed Martin ATC
University of Maryland, College Park, MD, US
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Organization ADBS, Building 252, 3251 Hanover Street, Palo Alto, CA 94304 and Astrophysics Laboratory, Lockheed Martin Advanced Technology Center, Department ADBS, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
NASA, Goddard Space Flight Center, Greenbelt, MD
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Dept.L9-41, Bldg.252, 3251 Hanover St., Palo Alto, CA 94304, USA
Lockheed Martin Advanced Technology Center, Solar & Astrophysics Laboratory, Department L9-41, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
Solar and Astrophysics Laboratory, Lockheed Martin ATC, 3251 Hanover St., Bldg. 252, Org. ADBS Palo Alto, CA 94304
Solar and Astrophysics Laboratory, Lockheed Martin Advanced Technology Center
Solar and Astr
2D Feature Recognition And 3d Reconstruction In Solar Euv Images
2D MHD modelling of compressible and heated coronal loops obtained via nonlinear separation of variables and compared to TRACE and SoHO observations
2D MHD Modelling of Heated Coronal Loops Compared to TRACE Observations
3-D reconstruction of active regions with STEREO
3-D reconstruction of CME related transient coronal phenomena observed with the STEREO/SECCHI Extreme Ultraviolet Imager
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