TANTALUM. THE MULTI-PURPOSE METALSCHUSSLER M.1972; PRECIS-METAL; U.S.A.; DA. 1972; VOL. 30; NO 11; PP. 64-66Serial Issue

THE SOLAR TORSIONAL OSCILLATION AND DYNAMO MODELS OF THE SOLAR CYCLESCHUSSLER M.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 94; NO 2; PP. L17-L18; BIBL. 16 REF.Article

NON-LINEAR DYNAMO THEORY: FINITE AMPLITUDE MAGNETIC FIELDS WITH LARGE SCALE CIRCULATION IN A COMPRESSIBLE STRATIFIED MEDIUMSCHUSSLER M.1979; ASTR. AND ASTROPHYS.; DEU; DA. 1979; VOL. 72; NO 3; PP. 348-355; BIBL. 38 REF.Article

ON BUOYANT MAGNETIC FLUX TUBES IN THE SOLAR CONVECTION ZONE.SCHUSSLER M.1977; ASTR. AND ASTROPHYS.; GERM.; DA. 1977; VOL. 56; NO 3; PP. 439-442; BIBL. 16 REF.Article

Is there a phase constraint for solar dynamo models?SCHÜSSLER, M.Astronomy and astrophysics (Berlin. Print). 2005, Vol 439, Num 2, pp 749-750, issn 0004-6361, 2 p.Article

Solar magnetic elementsSCHÜSSLER, M.Geophysical and astrophysical fluid dynamics. 1991, Vol 62, Num 1-4, pp 271-281, issn 0309-1929Article

The interchange instability of small flux tubesSCHÜSSLER, M.Astronomy and astrophysics (Berlin. Print). 1984, Vol 140, Num 2, pp 453-458, issn 0004-6361Article

AXISYMMETRIC ALPHA ^2-DYNAMOS IN THE HAYASHIPHASE.SCHUSSLER M.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 38; NO 2; PP. 263-270; BIBL. 27 REF.Article

Simulating solar MHD : Theory and simulation of solar system plasmasSCHÜSSLER, M.Annales geophysicae (1988). 1999, Vol 17, Num 5, pp 578-582, issn 0992-7689Article

DIFFUSION OF A STRONG INTERNAL MAGNETIC FIELD THROUGH THE RADIATIVE ENVELOPE OF A 2.25 M _CERCLE.-STAR.SCHUSSLER M; PAHLER A.1978; ASTR. AND ASTROPHYS.; DEU; DA. 1978; VOL. 68; NO 1-2; PP. 57-62; BIBL. 28 REF.Article

SELECTIVE DISSOLUTION OF THE BINDER PHASE ALLOY (CO-W) FROM WC-CO CEMENTED CARBIDES IN PARTICULATE BED ELECTRODE SYSTEMS = DISSOLUTION SELECTIVE DE LA PHASE ASSURANT LA LIAISON CO-W DANS LES ALLIAGES WC-COGHANDEHARI MH; FAULKNER JK; SCHUSSLER M et al.1982; J. ELECTROCHEM. SOC.; ISSN 0013-4651; USA; DA. 1982; VOL. 129; NO 12; PP. 2666-2668; BIBL. 4 REF.Article

Are the strengths of solar cycles determined by converging flows towards the activity belts?CAMERON, R. H; SCHÜSSLER, M.Astronomy and astrophysics (Berlin. Print). 2012, Vol 548, issn 0004-6361, A57.1-A57.7, 1Article

Solar cycle prediction using precursors and flux transport modelsCAMERON, R; SCHÜSSLER, M.The Astrophysical journal. 2007, Vol 659, Num 1, pp 801-811, issn 0004-637X, 11 p., 1Article

A solar surface dynamoVÖGLER, A; SCHÜSSLER, M.Astronomy and astrophysics (Berlin. Print). 2007, Vol 465, Num 3, issn 0004-6361, L43-L46Article

Continuum intensity of magnetic flux concentrations: are magnetic elements bright points?SCHÜSSLER, M; SOLANKI, S. K.Astronomy and astrophysics (Berlin. Print). 1988, Vol 192, Num 1-2, pp 338-342, issn 0004-6361Article

The dynamical disconnection of sunspots from their magnetic rootsSCHÜSSLER, M; REMPEL, M.Astronomy and astrophysics (Berlin. Print). 2005, Vol 441, Num 1, pp 337-346, issn 0004-6361, 10 p.Article

A ROBUST CORRELATION BETWEEN GROWTH RATE AND AMPLITUDE OF SOLAR CYCLES : CONSEQUENCES FOR PREDICTION METHODSCAMERON, R; SCHÜSSLER, M.The Astrophysical journal. 2008, Vol 685, Num 2, pp 1291-1296, issn 0004-637X, 6 p., 1Article

Steuert die Sonne das Erdklima? = Does the Sun control the Earth climate ?SCHÜSSLER, M; SCHMITT, D.KI. Luft- und Kältetechnik. 2000, Vol 36, Num 2, pp 63-67, issn 0945-0459Article

Model calculations of magnetic flux tubes. IV: Convective energy transport and the nature of intermediate size flux concentrationsKNÖLKER, M; SCHÜSSLER, M.Astronomy and astrophysics (Berlin. Print). 1988, Vol 202, Num 1-2, pp 275-283, issn 0004-6361Article

Strong horizontal photospheric magnetic field in a surface dynamo simulation : Science with hinodeSCHÜSSLER, M; VÖGLER, A.Astronomy and astrophysics (Berlin. Print). 2008, Vol 481, Num 1, issn 0004-6361, L5-L8Article

Does the butterfly diagram indicate a solar flux-transport dynamo?SCHÜSSLER, M; SCHMITT, D.Astronomy and astrophysics (Berlin. Print). 2004, Vol 421, Num 1, pp 349-351, issn 0004-6361, 3 p.Article

Non-linear dynamos. I: One-dimensional model of a thin layer dynamoSCHMITT, D; SCHÜSSLER, M.Astronomy and astrophysics (Berlin. Print). 1989, Vol 223, Num 1-2, pp 343-351, issn 0004-6361Article

Flow instabilities of magnetic flux tubes I. Perpendicular flowSCHÜSSLER, M; FERRIZ MAS, A.Astronomy and astrophysics (Berlin. Print). 2007, Vol 463, Num 1, pp 23-29, issn 0004-6361, 7 p.Article

Modeling the Sun's open magnetic fluxSCHÜSSLER, M; BAUMANN, I.Astronomy and astrophysics (Berlin. Print). 2006, Vol 459, Num 3, pp 945-953, issn 0004-6361, 9 p.Article

Evidence for the 22-year-cycle in the longitudinal distribution of sunspotsBALTHASAR, H; SCHÜSSLER, M.Solar physics. 1984, Vol 93, Num 1, pp 177-179, issn 0038-0938Article