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au.\*:("SHAWHAN SD")

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DESCRIPTION OF THE ISEE SATELLITE-TO-SATELLITE KILOMETRIC WAVELENGTH INTERFEROMETER SYSTEM = DESCRIPTION DU SYSTEME D'INTERFEROMETRIE ENTRE LES 2 SATELLITES ISEE EN ONDES KILOMETRIQUESSHAWHAN SD.1979; ANN. TELECOMMUNIC.; FRA; DA. 1979; VOL. 34; NO 3-4; PP. 266-272; ABS. FRE; BIBL. 15 REF.Article

MAGNETOSPHERIC PLASMA WAVE RESEARCH 1975-1978SHAWHAN SD.1979; REV. GEOPHYS. SPACE PHYS.; USA; DA. 1979; VOL. 17; NO 4; PP. 705-724; BIBL. 10 REF.Article

POLARIZATION MEASUREMENTS OF AURORAL KILOMETRIC RADIATION BY DYNAMICS EXPLORER-1SHAWHAN SD; GURNETT DA.1982; GEOPHYS. RES. LETT.; ISSN 0094-8276; USA; DA. 1982; VOL. 9; NO 9; PP. 913-916; BIBL. 11 REF.Article

A SEARCH FOR SLOWLY VARYING RADIO CONTINUUM EMISSION FROM UV CETI STARS.SPANGLER SR; SHAWHAN SD.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 205; NO 2 PART. 1; PP. 472-474; BIBL. 10 REF.Article

THE ANGULAR DISTRIBUTION OF AURORAL KILOMETRIC RADIATION.GREEN JL; GURNETT DA; SHAWHAN SD et al.1977; J. GEOPHYS. RES.; U.S.A.; DA. 1977; VOL. 82; NO 13; PP. 1825-1838; BIBL. 20 REF.Article

FOUR-STOKES-PARAMETER RADIOFREQUENCY POLARIMETRY OF A FLORE FROM AD LEONIS.SPANGLER SR; RANKIN JM; SHAWHAN SD et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 194; NO 1 PART. 2; PP. 43-46; BIBL. 14 REF.Article

MODELS FOR QUASI-PERIODIC ELECTRIC FIELDS AND ASSOCIATED ELECTRON PRECIPITATION IN THE AURORAL ZONE.PETELSKI EF; FAHLESON U; SHAWHAN SD et al.1978; J. GEOPHYS. RES.; USA; DA. 1978; VOL. 83; NO 6; PP. 2489-2498; BIBL. 42 REF.Article

STRUCTURE AND EVOLUTION OF SOLAR RADIO BURSTS AT 26.4 MHZ.SHA LIN CHEN H; SHAWHAN SD.1978; SOLAR PHYS.; NLD; DA. 1978; VOL. 57; NO 1; PP. 205-227; BIBL. 42 REF.Article

THE 1975.9 JOVIAN DECIMETRIC SPECTRUMSHAWHAN SD; HODGES MW; SPANGLER SR et al.1977; J. GEOPHYS. RES.; USA; DA. 1977; VOL. 82; NO 13; PP. 1901-1905; BIBL. 18 REF.Article

SHORT-DURATION RADIO FLARES OF UV CETI STARS.SPANGLER SR; SHAWHAN SD; RANKIN JM et al.1974; ASTROPHYS. J.; U.S.A.; DA. 1974; VOL. 190; NO 3 PART. 2; PP. 129-131; BIBL. 13 REF.Article

INTERPLANETARY SCINTILLATION OBSERVATIONS WITH THE COCOA CROSS RADIO TELESCOPE.CRONYN WM; SHAWHAN SD; ERSKINE FT et al.1976; J. GEOPHYS. RES.; U.S.A.; DA. 1976; VOL. 81; NO 4; PP. 695-697; BIBL. 17 REF.Article

OBSERVATION USING INTERPLANETARY SCINTILLATIONS AT 34.3 MHZ OF THE EFFECT OF A SOLAR WIND DISTURBANCE ON A SOLAR ENERGETIC PARTICLE EVENT.ROELOF EC; KRIMIGIS SM; CRONYN WM et al.sdIN: INT. COSMIC RAY CONF. 14; MUENCHEN; 1975; MUENCHEN; MAX PLANCK INST.; DA. S.D.; VOL. 5; PP. 1692-1697; BIBL. 8 REF.Conference Paper

INTERPLANETARY SCINTILLATION AT LARGE ELONGATION ANGLES: RESPONSE TO SOLAR WIND DENSITY STRUCTUREERSKINE FT; CRONYN WM; SHAWHAN SD et al.1978; J. GEOPHYS. RES.; USA; DA. 1978; VOL. 83; NO 9; PP. 4153-4164; BIBL. 45 REF.Article

SYNOPTIC ANALYSIS OF INTERPLANETARY RADIO SCINTILLATION SPECTRA OBSERVED AT 34 MHZGOTWOLS BL; MITCHELL DG; ROELOF EC et al.1978; J. GEOPHYS. RES.; USA; DA. 1978; VOL. 83; NO 9; PP. 4200-4206; BIBL. 14 REF.Article

CHARACTERISTICS OF A STABLE AURORAL RED ARC EVENTKOZYRA JU; CRAVENS TE; NAGY AF et al.1982; GEOPHYS. RES. LETT.; ISSN 0094-8276; USA; DA. 1982; VOL. 9; NO 9; PP. 973-976; BIBL. 17 REF.Article

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