Observational manifestations of solar magnetoconvection: Center-to-limb variationCARLSSON, Mats; STEIN, Robert F; NORDLUND, Ake et al.The Astrophysical journal. 2004, Vol 610, Num 2, pp L137-L140, issn 0004-637X, 2Article

High resolution solar physicsHIRZBERGER, Johann.Recent research developments in astronomy and astrophysics (Vol. 2 (2004)). Recent research developments in astronomy and astrophysics. 2004, pp 153-171, isbn 81-7736-202-X, 19 p.Book Chapter

Nonlinear evolution of magnetic and Kelvin-Helmholtz instabilities in the solar coronaEINAUDI, G.Plasma physics and controlled fusion. 1999, Vol 41, Num 3A, pp A293-A305, issn 0741-3335, SUPConference Paper

Observations of the limb effect in potassium λ7699LOPRESTO, J. C; KRAUS, P. M; PIERCE, A. K et al.Solar physics. 1994, Vol 149, Num 2, pp 243-247, issn 0038-0938Article

A revision of the solar abundance of dysprosiumGREVESSE, N; NOELS, A; SAUVAL, A. J et al.Astronomy and astrophysics (Berlin. Print). 1993, Vol 271, Num 2, pp 587-588, issn 0004-6361Article

A study of the asymmetry of FE I lines in the solar spectrumSTATHOPOULOU, M; ALISSANDRAKIS, C. E.Astronomy and astrophysics (Berlin. Print). 1993, Vol 274, Num 2, pp 555-562, issn 0004-6361Article

Filigree, magnetic fields, and flows in the photosphereZHANG YI; ENGVOLD, O.Solar physics. 1993, Vol 144, Num 1, pp 1-14, issn 0038-0938Article

Radiative lifetime measurements in Dy II and the solar abundance of dysprosiumBIEMONT, E; LOWE, R. M.Astronomy and astrophysics (Berlin. Print). 1993, Vol 273, Num 2, pp 665-670, issn 0004-6361Article

Dynamics of the solar granulation. II: A quantitative approachNESIS, A; HANSLMEIER, A; HAMMER, R et al.Astronomy and astrophysics (Berlin. Print). 1993, Vol 279, Num 2, pp 599-609, issn 0004-6361Article

About spectroscopic measurements of the solar meridional motionCAVALLINI, F; CEPPATELLI, G; RIGHINI, A et al.Astronomy and astrophysics (Berlin. Print). 1992, Vol 254, Num 1-2, pp 381-386, issn 0004-6361Article

Is mesogranulation a distinct regime of convection?STRAUS, T; DEUBNER, F.-L; FLECK, B et al.Astronomy and astrophysics (Berlin. Print). 1992, Vol 256, Num 2, pp 652-659, issn 0004-6361Article

On the evidence for mesogranules in solar power spectraGINET, G. P; SIMON, G. W.The Astrophysical journal. 1992, Vol 386, Num 1, pp 359-363, issn 0004-637X, p.1Article

Power spectra of median- and small-scale solar convectionCHOU, D.-Y; OU, K.-T; WANG, C.-C et al.The Astrophysical journal. 1992, Vol 396, Num 1, pp 333-339, issn 0004-637X, p.1Article

On the role of the motion of the photospheric footpoints of the magnetic field linesWU LIN-XIANG.Chinese astronomy and astrophysics. 1992, Vol 16, Num 4, pp 427-433, issn 0275-1062Article

High spatial resolution solar photospheric line observations in Ca⁺ active regionsHANSLMEIER, A; MATTIG, W; NESIS, A et al.Astronomy and astrophysics (Berlin. Print). 1991, Vol 244, Num 2, pp 521-532, issn 0004-6361, 12 p.Article

Multicolor continuum analysis of the solar granulation in quiet and active regionsKELLER, C. U; KOUTCHMY, S.The Astrophysical journal. 1991, Vol 379, Num 2, pp 751-757, issn 0004-637X, p.1Article

The double magnification bias by gravitational lensingBORGEEST, U; V. LINDE, J; REFSDAL, S et al.Astronomy and astrophysics (Berlin. Print). 1991, Vol 251, Num 2, pp L35-L38, issn 0004-6361Article

The photospheric dynamo. I : Magnetic flux-tube generationHENOUX, J. C; SOMOV, B. V.Astronomy and astrophysics (Berlin. Print). 1991, Vol 241, Num 2, pp 613-617, issn 0004-6361Article

Possibilité de détermination de la distribution en brillance du bord de la photosphère solaire à partir des données observationnelles d'éclipseBELKINA, I. L; DYATEL, N. P; POSPERGELIS, M. M et al.Kinematika i fizika nebesnyh tel. 1990, Vol 6, Num 2, pp 53-60, issn 0233-7665Article

An analysis of the formation in magnetic field and the formation depth of seven solar photospheric FEI lines. ISONG WEI-HONG; AI GUO-XIANG; ZANG HONG-QI et al.Chinese astronomy and astrophysics. 1990, Vol 14, Num 2, pp 155-166Article

Determination of force-free magnetic fields above the photosphere using three-component boundary conditions: moderately non-linear caseCUPERMAN, S; OFMAN, L; SEMEL, M et al.Astronomy and astrophysics (Berlin. Print). 1990, Vol 230, Num 1, pp 193-199, issn 0004-6361Article

Mesogranulation: a convective phenomenonDEUBNER, F.-L.Astronomy and astrophysics (Berlin. Print). 1989, Vol 216, Num 1-2, pp 259-264, issn 0004-6361Article

Perturbation of the granular pattern by the presence of magnetic flux tubesMULLER, R; ROUDIER, T; HULOT, J. C et al.Solar physics. 1989, Vol 119, Num 2, pp 229-243, issn 0038-0938Article

The effect of an interaction of magnetic flux and supergranulation on the decay of magnetic plagesSCHRIJVER, C. J.Solar physics. 1989, Vol 122, Num 2, pp 193-208, issn 0038-0938Article

How deep can one see into the sun?AYRES, T. R.Solar physics. 1989, Vol 124, Num 1, pp 15-22, issn 0038-0938Article