34th Solar Physics Division Meeting, June 2003
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All findings are embargoed until the time of presentation at the meeting.


Session 17 Corona III

Poster, Wednesday, June 18, 2003, 3:30-5:00pm, Mezzanine

17.01 A New Method to Constrain the Iron Abundance from Cooling Delays in Coronal Loops
M.J. Aschwanden, C.J. Schrijver (Locheed Martin, Solar & Astrophysics Lab.), A.R. Winebarger, H.P. Warren (Naval Research Laboratory)
17.02 Hydrodynamic Model of Loops Heated by Microflares at the Footpoints
P. Testa (Dip. Scienze Fisiche e Astron., Univ. di Palermo; Harvard-Smithsonian CfA), G. Peres (Dip. Scienze Fisiche e Astron., Univ. di Palermo)
17.03 Effects of Large-Scale Flows on Coronal Abundances: Multispecies Models and TRACE Observations
D.D. Lenz (RSI/SAO)
17.04 Moss Loop Cooling in the TRACE 171A Passband
M.A. Weber, D.B. Seaton, E.E. DeLuca (CFA/SAO), E. Lee (Harvard U.)
17.05 TRACE and CDS: JOP 146 Data Analysis Part I
J.T. Scott, J.W. Cirtain, P.C.H. Martens (Montana State University)
17.06 Properties of the Lower Transition Region Deduced from Widths of Optically Allowed Lines in SUMER Spectra
G. A. Doschek (Naval Research Laboratory)
17.07 Coronal Loop Differential Emission Measures from TRACE and CDS Observations
P. S. Hamilton, E. E. DeLuca, K. Johnson (CfA)
17.08 Limb Looking: The effects of background subtraction on the temperature of SXT loops.
D.A. Medlin, H.T. Blevins, J.T. Schmelz (University of Memphis)
17.09 SOHO-CDS Coronal Loops: Multi-thermal Analysis and Background Subtraction
K. Nasraoui, J.T. Schmelz, C.R. Nevels (University of Memphis)
17.10 TRACE Image Flat Field and Sensitivity Corrections
R.W. Nightingale, T.D. Tarbell, C.J. Wolfson (LMSAL)
17.11 To BG or not to BG: Background Subtraction for EIT Coronal Loops
J.E. Beene, J.T. Schmelz (University of Memphis)
17.12 A New Fitting Procedure for the Blended He I 1083 nm Multiplet
H.P. Jones (NASA's GSFC), O,V. Malanushenko (NSO)


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