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HMI
Results: 520

#	Item
221	Global Helioseismology Pipeline Tim Larson [removed] HMI Team Meeting September 2009 Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2009-09-16 11:36:48 Software Scripting languages Helioseismology Sun Concurrent Versions System Pipeline Shell script Inter-process communication Computing Computer programming
222	Source Code Version Management and Configuration Control Art Amezcua Status[removed] Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2007-11-05 12:08:24 Concurrent Versions System Revision control Software Computing Version control
223	PDF Document Add to Reading List Source URL: hmi.stanford.edu Language: Vietnamese - Date: 2006-03-15 15:29:39
224	SESSION C7/M5: CONNECTIONS TO GEOSPACE STEPHEN FUSELIER ZORAN MIKIC´ HMI/AIA Science Teams Meeting Monterey, CA, February 13–17, 2006 Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2006-06-05 16:35:18 Physics Sun Astronomy Light sources Corona Extreme ultraviolet Solar wind Heliosphere Solar Dynamics Observatory Space plasmas Plasma physics Astrophysics
225	Solar Subsurface Flows from Ring-Diagram Analysis Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2006-04-05 14:25:06 Anticyclones Vorticity High-pressure area Diagram Ring Meteorology Fluid dynamics Ring theory
226	Implementation of TravelTime Measurements in the HMI pipeline S. Couvidat and the HMI Time-Distance Pipeline Team HMI Team Meeting --- Stanford, 2009 September Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2009-09-14 20:41:49
227	Progress in Helioseismic Holography Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2006-04-05 14:26:03 Supergranulation Braun Vorticity Physics Space Fluid dynamics Helioseismology Sun
228	PDF Document Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2006-02-08 14:18:30 Space plasmas Astrophysics Acoustics Waves in plasmas Coronal seismology Corona Harmonic Normal mode Overtone Physics Sun Plasma physics
229	Connecting Magnetic Clouds to Solar Surface Features Vasyl Yurchyshyn Big Bear Solar Observatory • Coronal mass ejecta (CMEs) are known to cause strongest Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2009-09-17 15:45:25 Physics Astronomy Magnetic cloud Corona Geomagnetic storm Sun Heliosphere Coronal mass ejection Space plasmas Plasma physics Astrophysics
230	Errors on Doppler Velocity, l.o.s. Magnetic Field Strength, and Continuum Intensity (G) Add to Reading List Source URL: hmi.stanford.edu Language: English - Date: 2009-09-14 20:41:23 Leptons Spintronics Limb darkening Plasma physics Physics Condensed matter physics Electron

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