Review of recent papers resulting on JOP 104 SUMER spectroscopic studies  (17 Jan 2006 updates in red).

Flare observations:

(1) About the explosive start of the M8 flare on May 9, 1999; Innes et al. (2001), ApJ 549, L249: [pdf]

(2) Spectroscopic signatures of a flare observed by SUMER; Dammasch et al. (2001), IAU Symposium 203, 264: [pdf]

(3) The IAU paper and this ApJ Letter are the first communications on hot loop oscillations; Kliem et al. (2002), ApJ 568, L61: [pdf]

(4) Correlated hot and cool plasma dynamics; Kliem et al. (2002), Yohkoh 10th Anniversary Meeting, COSPAR Coll. S. 13,271: [pdf]

(5) Initial features of the April 21, 2002 monster flare; Wang et al. (2002), ESA SP-505, 607: [pdf]

(6) Multi-wavelength observations during the onset of the April 21, 2002 monster flare; Kliem et al. (2003), submitted to ApJ:  [pdf missing]

(7) About the downflow observed during the April 21, 2002 monster flare; Innes et al. (2003), Sol. Phys. 217, 247: [pdf]

(8) Properties of 10 MK flaring plasma observed during the M8 flare on May 9, 1999; Landi et al. (2003), ApJ 582, 506: [pdf]

(9) Non-thermal mass motions above active regions; Feldman et al. (2003), ApJ 585,1087: [pdf]

(10) Doppler flows in 10 MK flare supra-arcade, Innes et al. (2003), Sol. Phys. 217,267: [pdf]

(11) Observation of In-situ Heating; Feldman et al. (2004), ApJ 609, 439: [pdf]

(12) On the Heating and Cooling during  Coronal Micro-Events, Proc. SOHO 13; Curdt et al. (2004), ESA SP-547, 333: [pdf]

Loop oscillations:

(1) SOHO 11 proceedings paper on SUMER loop oscillations; Wang et al. (2002) ESA SP-508, 465: [pdf]

(2) Doppler Oscillations in SUMER flare lines; Wang et al. (2002) ApJ 574, L101: [pdf]

(3) On the wave mode and the damping of hot loop oscillations; Ofman & Wang (2002), ApJ 580, L85: [pdf]

(4) Hot loop oscillations as seen by SUMER: What are they?; Wang et al. (2002), ESA SP-505, 199: [pdf]

(5) Statistical analysis of Doppler oscillation events observed by SUMER; Curdt et al. (2002), ESA SP-506, 581: [pdf]

(6) 54 examples and statistics of SUMER loop oscillations proving the standing wave model; Wang et al. (2003), A&A 406, 1105: [pdf]

(7) Doppler oscillations of AR loops: steps towards coronal seismology; Curdt et al. (2003), Hvar Obs. Bull. 27 (1), 83: [pdf]

(8) SUMER loop oscillations modelled as slow-mode standing axial waves; Wang et al. (2003), A&A 402, L17: [pdf]

(9) AR loop dynamics; Innes & Wang (2004), Proc. SoHO 15, ESA SP 575, 553: [pdf]

(10) Vertical TRACE oscillations; Wang & Solanki (2004), A&A 421, L33:  [pdf]

(11) Numerical Simulations of Axial Loop Oscillations; Selwa et al. (2005), A&A 440, 285: [pdf]

(12) Initiation of hot coronal loop oscillations; Wang et al. (2005), A&A 435, 753: [pdf]

(13) Evidence for In-Situ Heating in AR loops; Curdt et al (2005), Proc. SoHO 16, ESA SP-592, 475: [pdf]

Atomic Physics and Spectroscopy:

(1) Precision measurements of the first resonance transition of He-like Ne IX, Na X, Mg XI, and Si XIII.; Curdt et al. (2000), Phys. Rev. A 62, 022502: [pdf]

(2) A list of flare lines in the SUMER  spectral range has been compiled, identifications and measured wavelengths are given : [html]; the list is taken from Feldmann et al. (2000), ApJ 544, 508: [pdf]

(3) A study of  the Fe XX emission lines in the SUMER spectral range; Kucera et al. (2000), ApJ 538, 424: [pdf]

(4) Bremsstrahlung and related diagnostic methods in flaring plasmas; Feldmann et al. (2003), ApJ 593, 1226: [pdf]

(5) Forbidden Lines of Low Abundant Species; Feldman et al. (2004), ApJ, 607, 1039 [pdf]