Bradley Hindman/University of Colorado Helioseismic Tools that Incorporate Corrections Arising from Magnetic Active Regions One of the primary goals of the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamic

Source URL: lws-trt.gsfc.nasa.gov

• Space
• Helioseismology
• Plasma physics
• Space plasmas
• Solar telescopes
• Solar Dynamics Observatory
• Sunspot
• Magnet
• Absorption
• Physics
• Astronomy
• Sun

New Light on Loop Prominence Systems Flare loops appear in the solar corona under a variety of descriptions, to which we now add a completely new one provided by HMI. Although not a coronagraph, this small optical telesc

Source URL: www.mssl.ucl.ac.uk

Microsoft Word - HMI Fact Sheet FY13 (3).doc

Source URL: www.hermanmiller.com

• Michigan
• Herman Miller
• D. J. DePree
• Design
• Robert Propst
• Geography of Michigan
• Ottawa County
• Michigan
• Zeeland
• Michigan

HMI/SCADA IECslave

Source URL: www.copalp.com

Bullying: effective action in secondary schools HMI 465 ERRATUM

Source URL: www.yourhealthsunderland.com

HMI Camera 2 Solar Radius (CDELT1*RSUNREF

Source URL: jsoc.stanford.edu

Studies of the Solar Shape by HMI on SDO R. I. Bush Solar Physics Group, Stanford University, Stanford, CA

Source URL: smsc.cnes.fr

• Solar Dynamics Observatory
• Plasma physics
• Space plasmas
• Space telescopes
• Sun
• Solar and Heliospheric Observatory
• Spacecraft
• Spaceflight
• Solar telescopes
• Space

SDO radial orbital velocity - HMI raw velocity medianmeters/second

Source URL: jsoc.stanford.edu

HMI Cal Mode Intensities for Side (red) & Front (greenIntensity normalized to 1 May 2010 intensity = 1.006 + -0.064*year + 0.0069*year^2

Source URL: jsoc.stanford.edu

SDO and HMI mean radial velocity 1000 meters/second 500

Source URL: jsoc.stanford.edu