Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
LMATC
LMSAL
Lockheed Martin
Lockheed Martin Advanced Technology Center, Palo Alto, CA
Department ADBS, Lockheed Martin Advanced Technology Center
Lockheed Martin Advanced Technology Ctr., USA
Lockheed Martin Advanced Technology Center, Department L9-41, Building 252, 3251 Hanover Street, Palo Alto, CA 94304 Institute for Space Research, Department L9-41, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
Stanford-Lockheed Institute for Space Research, 3251 Hanover Street, Palo Alto, CA 94304, USA
Lockheed Martin Solar Astrophysics Laboratory, Org. L9-41, Bldg. 252, 3251 Hanover Street, Palo Alto, CA 94304, USA
Lockheed Martin Advanced Technology Center, 3251 Hanover Street, Palo Alto, CA 94304, USA Martin Advanced Technology Center
Department H1-12, Stanford-Lockheed Institute for Space Research
Lockheed Martin Advanced Technology Center, Solar & Astrophysics Laboratory, Department L9-41, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
Stanford-Lockheed Institute for Space Research, Department L9-41, Building 252, 3251 Hanover Street, Palo Alto, CA 94304 Martin Advanced Technology Center, Department L9-41, Bldg. 252, 3251 Hanover Street
Stanford-Lockheed Institute for Space Research, Department L9-41, Bldg. 252, 3251 Hanover Street, Palo Alto, CA 94304, USA
Lockheed Martin Advanced Technology Center, 3251 Hanover Street, Palo Alto, CA 94304
Lockheed Martin Adv. Tech. Ctr.
Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, Department L941, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
Stanford University, California
Lockheed Martin Advanced Technology Center, Org. ADBS, Building 252, 3251 Hanover Street, Palo Alto, CA 94304
(Erratum) Rotating, magnetic braking, and dynamos in cool giants and subgiants.
A Case for Resonant Scattering in the Quiet Solar Corona in Extreme-Ultraviolet Lines with High Oscillator Strengths
A Characteristic Magnetic Field Pattern Associated with All Major Solar Flares and Its Use in Flare Forecasting
A construction kit for atmospheric activity of cool stars based on solar characteristics
A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953
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