- WHAT DETERMINES THE INTENSITY OF SOLAR FLARE/CME EVENTS? Yingna Su,1,2
- NLFFF X17
- POLARIZATION OF LOOP-TOP AND FOOTPOINT SOURCES IN MICROWAVE BURSTS
- A STATISTICAL STUDY OF SHEAR MOTION OF THE FOOTPOINTS IN TWO-RIBBON FLARES Yingna Su,1,2
- PASJ: Publ. Astron. Soc. Japan 59, S785S791, 2007 November 30 c 2007. Astronomical Society of Japan.
- Magnetic Shear in Two-ribbon Solar Flares M.S., Purple Mountain Observatory (2004)
- Yingna Su CV Postdoctoral Researcher
- The Astrophysical Journal, 734:53 (17pp), 2011 June 10 doi:10.1088/0004-637X/734/1/53 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- Structure and Dynamics of Quiescent Filament Channels Observed by Hinode/XRT and STEREO/EUVI
- The Astrophysical Journal, 704:341353, 2009 October 10 doi:10.1088/0004-637X/704/1/341 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- The Astrophysical Journal, 691:105114, 2009 January 20 doi:10.1088/0004-637X/691/1/105 c 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- Solar Physics (2006) 236: 325349 DOI: 10.1007/s11207-006-0039-z C Springer 2006
