Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp43a..05s&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SP43A-05
Astronomy and Astrophysics
Astrophysics
7500 Solar Physics, Astrophysics, And Astronomy, 7522 Helioseismology, 7524 Magnetic Fields, 7594 Instruments And Techniques
Scientific paper
The primary goal of the Helioseismic and Magnetic Imager (HMI) investigation is to study the origin of solar variability and to characterize and understand the Sun's interior and the various components of magnetic activity. The HMI investigation is based on measurements obtained with the HMI instrument as part of the Solar Dynamics Observatory (SDO) mission. HMI makes measurements of the motion of the solar photosphere to study solar oscillations and measurements of the polarization in a spectral line to study all three components of the photospheric magnetic field. Here we will give an overview of the HMI science goals, the HMI instrument and its expected performance, the science products produced and the ways in which the science community and public will be able to utilize HMI data.
HMI Team
Scherrer Philip H.
No associations
LandOfFree
The Helioseismic and Magnetic Imager for the Solar Dynamics Observatory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Helioseismic and Magnetic Imager for the Solar Dynamics Observatory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Helioseismic and Magnetic Imager for the Solar Dynamics Observatory will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1699363