WAVE DECAY IN MAGNETOHYDRODYNAMIC TURBULENCEBERESNYAK, Andrey; LAZARIAN, Alex.The Astrophysical journal. 2008, Vol 678, Num 2, pp 961-967, issn 0004-637X, 7 p., 1Article

On the spectrum of magnetohydrodynamic turbulenceBOLDYREV, Stanislav.The Astrophysical journal. 2005, Vol 626, Num 1, pp L37-L40, issn 0004-637X, 2Article

COSMIC RAY GENERATED ANISOTROPIC MAGNETOHYDRODYNAMIC TURBULENCE.SCHWARTZ SJ.1977; MONTH NOT. R. ASTR. SOC.; G.B.; DA. 1977; VOL. 178; NO 2; PP. 399-408; BIBL. 14 REF.Article

A simplified cascade model for M.H.D. turbulenceCARBONE, V; VELTRI, P.Astronomy and astrophysics (Berlin. Print). 1987, Vol 188, Num 1, pp 239-250, issn 0004-6361Article

Star formation efficiency in driven, supercritical, turbulent cloundsVAZQUEZ-SEMADENI, Enrique; KIM, Jongsoo; BALLESTEROS-PAREDES, Javier et al.The Astrophysical journal. 2005, Vol 630, Num 1, pp L49-L52, issn 0004-637X, 2Article

Anisotropy and energy decay in magneto-hydrodynamic turbulence : Theory and solar wind observationsOUGHTON, S; MATTHAEUS, W. H; GHOSH, S et al.Fluid mechanics and its application. 1998, pp 475-478, isbn 0-7923-5115-0Conference Paper

Dynamique des spectres dans une turbulence développéeBERSHADSKIJ, A. G.Magnitnaâ gidrodinamika. 1987, Num 2, pp 71-77, issn 0025-0015Article

Imbalanced strong MHD turbulenceLITHWICK, Y; GOLDREICH, P; SRIDHAR, S et al.The Astrophysical journal. 2007, Vol 655, Num 1, pp 269-274, issn 0004-637X, 6 p., 1Article

Nonlinear cosmic-ray diffusive transport in combined two-dimensional and slab magnetohydrodynamic turbulence : A bgk-boltzmann approachLE ROUX, J. A; WEBB, G. M.The Astrophysical journal. 2007, Vol 667, Num 2, pp 930-955, issn 0004-637X, 26 p., 1Article

Particle acceleration by magnetohydrodynamic turbulenceCHO, Jungyeon; LAZARIAN, A.The Astrophysical journal. 2006, Vol 638, Num 2, pp 811-826, issn 0004-637X, 16 p., 1Article

Rapid pickup of cometary ions due to strong magnetic turbulenceWU, C. S; WINSKE, D; GAFFEY, J. D. JR et al.Geophysical research letters. 1986, Vol 13, Num 8, pp 865-868, issn 0094-8276Article

LOCALITY OF MHD TURBULENCE IN ISOTHERMAL DISKSXIAOYUE GUAN; GAMMIE, Charles F; SIMON, Jacob B et al.The Astrophysical journal. 2009, Vol 694, Num 2, pp 1010-1018, issn 0004-637X, 9 p., 1Article

Simulations of relativistic force-free magnetohydrodynamic turbulenceJUNGYEON CHO.The Astrophysical journal. 2005, Vol 621, Num 1, pp 324-327, issn 0004-637X, 4 p., 1Article

Observations of MHD turbulence in the solar windBRUNO, R.Nuovo cimento della società italiana di fisica. C. 1997, Vol 20, Num 6, pp 881-896, issn 0390-5551Conference Paper

PARTICLE REACCELERATION AND APPARENT RADIO SOURCE STRUCTUREEILEK JA.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 254; NO 2; PART. 1; PP. 472-482; BIBL. 40 REF.Article

TWO-POINT, TWO-TIME ANALYSIS OF THE DECAY OF TURBULENCE IN THE PRESENCE OF A MAGNETIC FIELD.KUMAR P; PATEL SR; RAWAT JS et al.1975; INTERNATION. J. ENGNG SCI.; G.B.; DA. 1975; VOL. 13; NO 4; PP. 393-405; ABS. FR. ITAL. ALLEMArticle

ALFVENIC FLUCTUATIONS AS ASYMPTOTIC STATES OF MHD TURBULENCEGRAPPIN R; FRISCH U; POUQUET A et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 105; NO 1; PP. 6-14; BIBL. 32 REF.Article

MEASUREMENT OF THE RUGGED INVARIANTS OF MAGNETOHYDRODYNAMIC TURBULENCE IN THE SOLAR WINDMATTHAEUS WH; GOLDSTEIN ML.1982; JOURNAL OF GEOPHYSICAL RESEARCH; ISSN 0022-1406; USA; DA. 1982; VOL. 87; NO A8; PP. 6011-6028; BIBL. 1 P.Article

ON THE POLARIZATION STATE OF HYDROMAGNETIC FLUCTUATIONS IN THE SOLAR WINDBAVASSANO B; DOBROWOLNY M; MARIANI F et al.1981; J. GEOPHYS. RES.; ISSN 0022-1406; USA; DA. 1981; VOL. 86; NO A3; PP. 1271-1278; BIBL. 16 REF.Article

PROPERTIES OF MAGNETOHYDRODYNAMIC TURBULENCE IN THE SOLAR WINDDOBROWOLNY M; MANGENEY A; VELTRI PL et al.1980; SYMP.-INT. ASTRON. UNION; ISSN 0074-1809; NLD; DA. 1980; NO 91; PP. 143-146; BIBL. 6 REF.Conference Paper

Polarization intermittency and its influence on MHD turbulenceBERESNYAK, A; LAZARIAN, A.The Astrophysical journal. 2006, Vol 640, Num 2, issn 0004-637X, L175-L178, 2Article

Modeling a coronal loop heated by magnetohydrodynamic turbulence nanoflaresREALE, F; NIGRO, G; MALARA, F et al.The Astrophysical journal. 2005, Vol 633, Num 1, pp 489-498, issn 0004-637X, 10 p., 1Article

Isolated star formation: From cloud formation to core collapseWARD-THOMPSON, Derek.Science (Washington, D.C.). 2002, Vol 295, Num 5552, pp 76-81, issn 0036-8075Article

Subcritical magnetohydrodynamic turbulenceWALTZ, R. E.Physical review letters. 1985, Vol 55, Num 10, pp 1098-1101, issn 0031-9007Article

Un mécanisme possible pour la dissipation de l'énergie cinétique des écoulements de plasma dans les radiogalaxiesMOROZOV, V. N.Astrofizika. 1985, Vol 21, Num 3, pp 475-486, issn 0571-7132Article