Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Lockheed Martin Advanced Technology Center, 3251 Hanover Street, Palo Alto, CA 94304, USA Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Palo Alto, CA 94304, USA Martin Solar & Astrophysics Lab, Org. ADBS, B252 3251 Hanover St, Palo Alto, CA 94304, USA Martin Adv. Tech. Ctr
Lockheed Solar & Astrophysics Laboratory
Lockheed Martin Solar & Astrophysics Lab, 3251 Hanover Street, Org. ADBS, Bldg. 252, Palo Alto, CA 94304, USA Martin Palo Alto Research Laboratory
Lockheed-Martin
Lockheed-Martin Solar and Astrophysics Lab, Palo Alto, California 94304
Lockheed Martin Solar and Astrophysics Laboratory,
Lockheed-Martin Solar and Astrophysics Laboratory
Stanford-Lockheed Inst.
Lockheed Martin Solar & Astrophysics Lab, Org. L9-41, Bldg. 252 3251 Hanover St., Palo Alto, CA 94304, USA 3251 Hanover Street, Palo Alto, CA 94304, USA Martin Solar and Astrophysics Laboratory, B / 252 3251 Hanover St., Palo Alto, Ca 94304, USA Martin Research Laboratory, Department H1-12, Bldg. 252, Palo Alto, CA 94304, USA
Lockheed-Martin PARL
Lockheed Martin PARL
Lockheed Martin Solar and Astrophysics Lab.
Stanford Lockheed Inst. for Space Research
Lockheed Martin Solar and Astrophysics Lab, 3251 Hanover Street, Palo Alto, CA 94304, USA 3251 Hanover Street, Palo Alto, CA 94304, USA Martin Advanced Technology Center, 3251 Hanover St. B / 252, Palo Alto, CA 94304, USA
Lockheed Martin Solar & Astrophysics Lab, 3251 Hanover St., Palo Alto, CA 94304, USA Martin Solar and Astrophysis Lab, B / 252 O / ADBS 3251 Hanover St., Palo Alto, CA 94304, USA Martin Advanced Technology Center, 3251 Hanover Stree, Palo Alto, CA 94304 Bldg. 252, 3251 Hanover St., Palo Alto, CA 94304, USA
1024 x 1024 CCD Cameras under Development and Operation at Lockheed PARL
A new view of the solar corona from the transition region and coronal explorer (TRACE)
a Simple Image Motion Compensation System for Solar Observations
A Study of Magnetic Reconnection Processes in Solar Active Regions using TRACE, MDI and EIT Data
Active Region Moss as a Diagnostic for the Thermal Evolution of Chromospheric Spicule-Like Jets, and for Coronal Heating.
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