'Coronal magnetic field' presentation slideshows

21 March 2003

Solar Dynamics Observatory. Solar Dynamics Observatory System Concept Review Helioseismic and Magnetic Imager Draft Presentation. 21 March 2003. Stanford University Hansen Experimental Physics Laboratory Stanford, CA. Lockheed Martin Space Systems Company Advanced Technology Center

692 views • 53 slides

Lockheed Martin Space Systems Company Advanced Technology Center Solar & Astrophysics Laboratory

Solar Dynamics Observatory. Solar Dynamics Observatory System Concept Review Helioseismic and Magnetic Imager Presenters: P. Scherrer R. Bush L. Springer. Stanford University Hansen Experimental Physics Laboratory Stanford, CA.

613 views • 43 slides

Proxies of the Entire Surface Distribution of the Photospheric Magnetic Field

Proxies of the Entire Surface Distribution of the Photospheric Magnetic Field. Xuepu Zhao http://sun.stanford.edu/~xuepu/PUBLICATION NAOC, Oct. 18, 2011. 1. Introduction.

416 views • 30 slides

THE RELATION BETWEEN CORONAL EIT WAVE AND MAGNETIC CONFIGURATION

THE RELATION BETWEEN CORONAL EIT WAVE AND MAGNETIC CONFIGURATION. Speakers: Xin Chen. 1. INTRODUCTION. Coronal extrapolated magnetic fields EIT wave The relation of CME and EIT wave (mechanism). 1.1 Coronal extrapolated magnetic fields

316 views • 30 slides

Incorporating Magnetogram Data into Time-Dependent Coronal Field Models

Incorporating Magnetogram Data into Time-Dependent Coronal Field Models.

383 views • 25 slides

HMI Data Products: Plan and Status

HMI Data Products: Plan and Status. Primary goal: origin of solar variability.

333 views • 20 slides

Mei Zhang ? National Astronomical Observatory of China ?

Coronal Mass Ejection As a Result of Magnetic Helicity Accumulation. Mei Zhang ? National Astronomical Observatory of China ?. Collaborators : BC Low (HAO/NCAR) Natasha Flyer (SCD/NCAR). References : Zhang, Flyer & Low 2006, ApJ, 644, 575 Zhang & Flyer 2008, ApJ, 683, 1160.

357 views • 20 slides

Nour-Eddine R aouafi

Polar Holes: Latest Results SUMER: The Polarimeter Conclusions. Outline. Magnetic and Velocity Fields in the Solar Corona. Nour-Eddine R aouafi. Area of interest : polar coronal holes. LOS. Open superradial expanding field lines Source of the fast solar wind. UVCS Results.

383 views • 18 slides

3D Inversion of the Magnetic Field from Polarimetry Data of Magnetically Sensitive Coronal Ions

3D Inversion of the Magnetic Field from Polarimetry Data of Magnetically Sensitive Coronal Ions. M. Kramar, B. Inhester Max-Planck Institute for Solar System Research GERMANY. COSPAR, July 2004, Paris. Coronal Magnetic Field.

308 views • 13 slides

Heliospheric Magnetic Field 1835-2010

125 views • 11 slides

HMI Major Science Objectives

HMI Standard Data Products.

130 views • 1 slides