COMMENT ON CORONAL MAGNETIC FIELD MODELS (RESEARCH NOTE)SCHATTEN KH.1979; SOLAR PHYS.; NLD; DA. 1979; VOL. 63; NO 2; PP. 275-277; BIBL. 6 REF.Article

PREDICTION OF CORONAL AND INTERPLANETARY MAGNETIC FILEDSSCHATTEN KH.1972; PROGR. ASTRONAUT. AERONAUT.; U.S.A.; DA. 1972; VOL. 30; PP. 179-196; BIBL. 2P.1/2Conference Paper

THE ORIGIN OF INTERPLANETARY SECTORSSCHATTEN KH.1980; SYMP. - INT. ASTRON. UNION; ISSN 0074-1809; NLD; DA. 1980; NO 91; PP. 67-72; BIBL. 9 REF.Conference Paper

ELECTROMAGNETIC-GRAVITATIONAL ENERGY SYSTEMSSCHATTEN KH.1981; GEN. RELATIV. GRAVIT.; ISSN 0001-7701; GBR; DA. 1981; VOL. 13; NO 6; PP. 561-567; BIBL. 10 REF.Article

WHY THE SUN MAY APPEAR OBLATE.SCHATTEN KH.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 34; NO 2; PP. 467-480; BIBL. 27 REF.Article

TIME VARIATIONS OF THE ANGULAR MOMENTUM OF THE SUN.SCHATTEN KH.1977; ASTROPHYS. J.; U.S.A.; DA. 1977; VOL. 216; NO 2, PART. 1; PP. 650-653; BIBL. 15 REF.Article

CORONAL MAGNETIC FIELD MODELS.SCHATTEN KH.1975; REV. GEOPHYS. SPACE PHYS.; U.S.A.; DA. 1975; VOL. 13; NO 4; PP. 589-592; BIBL. 27 REF.Article

FAST AZIMUTHAL TRANSPORT OF SOLAR COSMIC RAYS VIA A CORONAL MAGNETIC BOTTLE.SCHATTEN KH; MULLAN DJ.1977; J. GEOPHYS. RES.; U.S.A.; DA. 1977; VOL. 82; NO 35; PP. 5609-5620; BIBL. 2 P.Article

THE FAINT YOUNG SUN-CLIMATE PARADOX: VOLCANIC INFLUENCESSCHATTEN KH; ENDAL AS.1982; GEOPHYSICAL RESEARCH LETTERS; ISSN 0094-8276; USA; DA. 1982; VOL. 9; NO 12; PP. 1309-1311; BIBL. 12 REF.Article

THE SCHWARZSCHILD CRITERION FOR CONVECTION IN THE PRESENCE OF A MAGNETIC FIELDSCHATTEN KH; SOFIA S.1981; ASTROPHYS. LETT.; ISSN 0004-6388; USA; DA. 1981; VOL. 21; NO 3-4; PP. 93-96; BIBL. 20 REF.Article

THE FAINT YOUNG SUN-CLIMATE PARADOX: CONTINENTAL INFLUENCESENDAL AS; SCHATTEN KH.1982; JOURNAL OF GEOPHYSICAL RESEARCH; ISSN 0022-1406; USA; DA. 1982; VOL. 87; NO C9; PP. 7295-7302; BIBL. 2 P.Article

REPLY TO GILMAN CONCERNING "SOLAR POLAR SPIN-DOWN".SCHATTEN KH; GILMAN PA.1974; SOLAR PHYS.; NETHERL.; DA. 1974; VOL. 37; NO 2; PP. 487-492; BIBL. 13 REF.Article

RESPONSE OF THE GEOMAGNETIC ACTIVITY INDEX KP TO THE INTERPLANETARY MAGNETIC FIELD.SCHATTEN KH; WILCOX JM.1967; J. GEOPHYS. RES.; USA; 1967(11), VOL. 72, NUM. 0021, P. 5185 A 5191Miscellaneous

A SUNSPOT PERIODICITY AND ITS POSSIBLE RELATION TO SOLAR ROTATIONKNIGHT JW; SCHATTEN KH; STURROCK PA et al.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 227; NO 3 PART. 2; PP. L153-L156; BIBL. 13 REF.Article

SOLAR IRRADIANCE VARIATIONS DUE TO ACTIVE REGIONSOSTER L; SCHATTEN KH; SOFIA S et al.1982; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1982; VOL. 256; NO 2; PART 1; PP. 768-773; BIBL. 15 REF.Article

PHOTOSPHERIC SUBROTATION, DIFFERENTIAL ROTATION AND ZONAL WIND BANDS: A REVERSE PIROUETTESCHATTEN KH; MAYR HG; LEVINE RH et al.1981; SOL. PHYS.; ISSN 0038-0938; NLD; DA. 1981; VOL. 71; NO 1; PP. 169-173; BIBL. 18 REF.Article

USING DYNAMO THEORY TO PREDICT THE SUNSPOT NUMBER DURING SOLAR CYCLE 21SCHATTEN KH; SCHERRER PH; SVALGAARD L et al.1978; GEOPHYS. RES. LETTERS; USA; DA. 1978; VOL. 5; NO 5; PP. 411-414; BIBL. 20 REF.Article

SOLAR IRRADIANCE MODULATION BY ACTIVE REGIONS FROM 1969 THROUGH 1980SCHATTEN KH; MILLER N; SOFIA S et al.1982; GEOPHYS. RES. LETT.; ISSN 0094-8276; USA; DA. 1982; VOL. 9; NO 1; PP. 49-51; BIBL. 4 REF.Article

INTERPLANETARY MAGNETIC FIELD POLARITY AND THE SIZE OF LOW-PRESSURE TROUGHS NEAR 180^O W LONGITUDEWILCOX JM; DUFFY PB; SCHATTEN KH et al.1979; SCIENCE; USA; DA. 1979; VOL. 204; NO 4388; PP. 60-62; BIBL. 6 REF.Article