The solar oxygen crisis : Probably not the last wordSOCAS-NAVARRO, H; NORTON, A. A.The Astrophysical journal. 2007, Vol 660, Num 2, issn 0004-637X, L153-L156, 2Article

HELIUM LINE FORMATION AND ABUNDANCE DURING A C-CLASS FLAREANDRETTA, Vincenzo; MAUAS, Pablo J. D; FALCHI, Ambretta et al.The Astrophysical journal. 2008, Vol 681, Num 1, pp 650-663, issn 0004-637X, 14 p., 1Article

Coronal element comparison observed by SOHO SUMER in the quiet southeast and northwest limb regions at 1.04 R_○. above the solar diskWIDING, K. G; LANDI, E; FELDMAN, U et al.The Astrophysical journal. 2005, Vol 622, Num 2, pp 1211-1215, issn 0004-637X, 5 p., 1Article

Metallic abundances of 2002 leonid meteoroids in two dust trails formed in different epochs : No evidence of solar heating effectKASUGA, T; WATANABE, J; YAMAMOTO, T et al.The Astrophysical journal. 2006, Vol 638, Num 2, pp 1176-1179, issn 0004-637X, 4 p., 1Article

NON-WKB MODELS OF THE FIRST IONIZATION POTENTIAL EFFECT: IMPLICATIONS FOR SOLAR CORONAL HEATING AND THE CORONAL HELIUM AND NEON ABUNDANCESMARTIN LAMING, J.The Astrophysical journal. 2009, Vol 695, Num 2, pp 954-969, issn 0004-637X, 16 p., 1Article

SOLAR FORBIDDEN OXYGEN, REVISITEDAYRES, Thomas R.The Astrophysical journal. 2008, Vol 686, Num 1, pp 731-740, issn 0004-637X, 10 p., 1Article

The discrepancy between solar abundances and helioseismologyANTIA, H. M; BASU, Sarbani.The Astrophysical journal. 2005, Vol 620, Num 2, pp L129-L132, issn 0004-637X, 2Article

The helium abundance of quiescent coronal loopsKILLIE, Mari Anne; LIE-SVENDSEN, Øystein; LEER, Egil et al.The Astrophysical journal. 2005, Vol 632, Num 2, pp L155-L158, issn 0004-637X, 2Article

MODELING IRON ABUNDANCE ENHANCEMENTS IN THE SLOW SOLAR WINDBYHRING, H. S; CRANMER, S. R; LIE-SVENDSEN, Ø et al.The Astrophysical journal. 2011, Vol 732, Num 2, issn 0004-637X, 732119.1-732119.12, 1Article

OXYGEN ISOTOPIC COMPOSITIONS OF SOLAR CORUNDUM GRAINSMAKIDE, Kentaro; NAGASHIMA, Kazuhide; KROT, Alexander N et al.The Astrophysical journal. 2009, Vol 706, Num 1, pp 142-147, issn 0004-637X, 6 p., 1Article

Modeling minor ion abundances in quiescent coronal loopsKILLIE, Mari Anne; LIE-SVENDSEN, Øystein.The Astrophysical journal. 2007, Vol 666, Num 1, pp 501-515, issn 0004-637X, 15 p., 1Article

OBSERVATIONAL EVIDENCE SUPPORTING CROSS-FIELD DIFFUSION OF NEUTRAL MATERIAL IN SOLAR FILAMENTSGILBERT, Holly; KILPER, Gary; ALEXANDER, David et al.The Astrophysical journal. 2007, Vol 671, Num 1, pp 978-989, issn 0004-637X, 12 p., 1Article

THE PHYSICAL PROPERTIES OF CORONAL STREAMERS. IIUZZO, M; STRACHAN, L; VOURLIDAS, A et al.The Astrophysical journal. 2007, Vol 671, Num 1, pp 912-925, issn 0004-637X, 14 p., 1Article

Oxygen abundance in coronal streamersVASQUEZ, Alberto M; RAYMOND, John C.The Astrophysical journal. 2005, Vol 619, Num 2, pp 1132-1141, issn 0004-637X, 10 p., 1Article

Helium line formation and abundance in a solar active regionMAUAS, P. J. D; ANDRETTA, V; FALCHI, A et al.The Astrophysical journal. 2005, Vol 619, Num 1, pp 604-612, issn 0004-637X, 9 p., 1Article

A NEW APPROACH TO THE SOLAR OXYGEN ABUNDANCE PROBLEMCENTENO, R; SOCAS-NAVARRO, H.The Astrophysical journal. 2008, Vol 682, Num 1, issn 0004-637X, L61-L64, 2Article

How do uncertainties in the surface chemical composition of the sun affect the predicted solar neutrino fluxes?BAHCALL, John N; SERENELLI, Aldo M.The Astrophysical journal. 2005, Vol 626, Num 1, pp 530-542, issn 0004-637X, 13 p., 1Article

Seismic study of the chemical composition of the solar convection zoneLIN, Chia-Hsien; ANTIA, H. M; BASU, Sarbani et al.The Astrophysical journal. 2007, Vol 668, Num 1, pp 603-610, issn 0004-637X, 8 p., 1Article

Solar models with revised abundances and opacitiesYANG, W. M; BI, S. L.The Astrophysical journal. 2007, Vol 658, Num 1, issn 0004-637X, L67-L70, 2Article

The detectability of neon fluorescence and measurement of the solar photospheric neon abundanceDRAKE, Jeremy J; ERCOLANO, Barbara.The Astrophysical journal. 2007, Vol 665, Num 2, issn 0004-637X, L175-L178, 2Article

Abundance variation at the vicinity of an active region and the coronal origin of the slow solar windKO, Yuan-Kuen; RAYMOND, John C; ZURBUCHEN, Thomas H et al.The Astrophysical journal. 2006, Vol 646, Num 2, pp 1275-1287, issn 0004-637X, 13 p., 1Article

Rhessi observations of the solar flare iron-line feature at 6.7 keVPHILLIPS, K. J. H; CHIFOR, C; DENNIS, B. R et al.The Astrophysical journal. 2006, Vol 647, Num 2, pp 1480-1490, issn 0004-637X, 11 p., 1Article

Can enhanced diffusion improve helioseismic agreement for solar models with revised abundances?GUZIK, Joyce A; WATSON, L. Scott; COX, Arthur N et al.The Astrophysical journal. 2005, Vol 627, Num 2, pp 1049-1056, issn 0004-637X, 8 p., 1Article

ARGON ABUNDANCES IN THE SOLAR NEIGHBORHOOD : NON-LTE ANALYSIS OF ORION ASSOCIATION B-TYPE STARSLANZ, Thierry; CUNHA, Katia; HOLTZMAN, Jon et al.The Astrophysical journal. 2008, Vol 678, Num 2, pp 1342-1350, issn 0004-637X, 9 p., 1Article

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