Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Department ADBS, Palo Alto, CA
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, O / ADBS B / 252, 3251 Hanover Street, Palo Alto, California 94304, USA
Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Palo Alto, California 94304, USA
Lockheed-Martin Solar & Astrophysics Lab., USA
Solar and Astrophysics Laboratory, Dept. ADBS, Lockheed Martin Advanced Technology Center
Solar and Astrophysics Laboratory, Dept ADBS Bldg 252, Lockheed Martin Advanced Technology Center
Lockheed Martin Advanced Technology Ctr., USA
LMSAL, 3251 Hanover Street, Palo Alto, CA 94304
Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover St, Palo Alto, CA 94304, USA and Astrophysics Laboratory, Lockheed Martin Space Systems Company, Palo Alto, CA, USA; Martin ATC
Lockheed-Martin Solar and Astrophysics Laboratory
Stanford University
Göttingen, Univ.-Sternwarte, Germany
Lockheed Martin Advanced Technology Center, 3251 Hanover St O / ADBS B / 252, Palo Alto, CA 94304, USA Martin Solar and Astrophysics Laboratory, 3251 Hanover St O / ADBS B / 252, Palo Alto, CA 94304, USA Martin Solar & Astrophysics Laboratory, 3251 Hanover Drive Bldg. 252, Org. ADBS, Palo Alto, CA 94304, USA Martin Solar & Astrophysics Laboratory, Palo Alto, CA, USA Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, USA and Astrophysics Laboratory, Lockheed Martin, Palo Alto, CA, USA Martin Advanced Technology Center, Palo Alto, CA, USA Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Organization ADBS, Building 252, Palo Alto, CA 94304, USA
LMSAL, Department ADBS Bldg. 252 3251 Hanover Street, Palo Alto, CA 94304, USA Martin Solar
A Statistical Model of the Inhomogeneous Corona Constrained by Triple-Filter Measurements of Elementary Loop Strands with TRACE
Alfvénic waves with sufficient energy to power the quiet solar corona and fast solar wind
Automated Temperature and Emission Measure Analysis of Coronal Loops and Active Regions Observed with the Atmospheric Imaging Assembly on the Solar Dynamics Observatory (SDO/AIA)
Calibration of AIA/SDO: Accessing and implementing the response functions
Coordinated observations of solar prominences with Hinode/SOT and SDO/AIA
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