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ON THE POLARIZATION CHARACTERISTICS OF MOVING TYPE IV SOLAR RADIO BURSTS.ROBINSON RD.1974; ASTR. SOC. AUSTRAL., PROC.; AUSTRAL.; DA. 1974; VOL. 2; NO 5; PP. 258-261; BIBL. 12 REF.; (ASTRON. SOC. AUSTRALIA. 8TH ANNU. GEN. MEET. PROC.; HOBART, TASMANIA; 1974)Conference Paper

MICROWAVE PULSATIONS FROM SOLAR FLARESMAXWELL A; FITZWILLIAM J.1973; ASTROPHYS. LETTERS; U.S.A.; DA. 1973; VOL. 13; NO 4; PP. 237-242; BIBL. 18REF.Serial Issue

DESCRIPTION DE GROUPES DE SURSAUTS RADIO TYPE IVAKIN'YAN ST.1972; ASTR. ZH.; S.S.S.R.; DA. 1972; VOL. 49; NO 3; PP. 579-587; BIBL. 17REF.Serial Issue

THE TIME BEHAVIOUR OF THE CONTINUA DURING THE INITIAL STAGE OF TYPE IV BURSTSBOEHME A.1972; SOLAR PHYS.; NETHERL.; DA. 1972; VOL. 24; NO 2; PP. 457-474; BIBL. 30REF.Serial Issue

THE TIME-LATITUDE DISTRIBUTION OF SOLAR FLARES ACCOMPANIED BY TYPE IV RADIO BRUSTS DURING THE PERIOD 1956 TO 1969PAPAGIANNIS MD; ZEREFOS CS; REPAPIS CC et al.1972; SOLAR PHYS.; NETHERL.; DA. 1972; VOL. 27; NO 1; PP. 208-216; BIBL. 29REF.Serial Issue

A LONG-ENDURING MULTI-SOURCE BURST AT 17 GHZ AND ITS RELATION TO A TYPE IVM-DM BURST WITH SPECTRAL FINE FEATURESKOSUGI T.1982; SOL. PHYS.; ISSN 0038-0938; NLD; DA. 1982; VOL. 75; NO 1-2; PP. 293-304; BIBL. 31 REF.Article

CORRELATION BETWEEN BANDWIDTH AND FREQUENCY DRIFT VELOCITY OF INTERMEDIATE DRIFT BURSTSELGAROY O; SOLDAL O.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 104; NO 1; PP. 99-100; BIBL. 4 REF.Article

DEVELOPMENT OF MOVING TYPE IV SOLAR RADIO BURSTS AND RELATION TO EXPANDING MAGNETIC BOTTLES FROM FLARE REGIONSSAKURAI K.1973; NATURE PHYS. SCI.; G.B.; DA. 1973; VOL. 243; NO 125; PP. 46-48; BIBL. 13REF.Serial Issue

ON MODULATIONS OF RADIO TYPE IV BURSTSTROTTET G; KERDRAON A.1980; INTERNATION. ASTR. UN., SYMP.; NLD; DA. 1980; NO 86; PP. 329-332; BIBL. 6 REF.Conference Paper

INTERFEROMETER OBSERVATION OF PULSATING SOURCES ASSOCIATED WITH A TYPE IV SOLAR RADIO BURSTKAI K; TAKAYANAGI A.1973; SOLAR PHYS.; NETHERL.; DA. 1973; VOL. 29; NO 2; PP. 461-475; BIBL. 11 REF.Serial Issue

PECULIAR ABSORPTION AND EMISSION MICROSTRUCTURES IN THE TYPE IV SOLAR RADIO OUTBURST OF MARCH 2, 1970SLOTTJE C.1972; SOLAR PHYS.; NETHERL.; DA. 1972; VOL. 25; NO 1; PP. 210-231; BIBL. 20REF.Serial Issue

A UNIFIED EXPLANATION OF SOLAR TYPE IV DM CONTINUA AND ZEBRA PATTERNS.KUIJPERS J.1975; ASTR. AND ASTROPHYS.; GERM.; DA. 1975; VOL. 40; NO 4; PP. 405-410; BIBL. 11 REF.Article

THE 350MHZ RADIO SUN DURING 1972 NOVEMBER-TWO INTERESTING EVENTSKELLY AN.1973; MONTH. NOTES ASTR. SOC. SOUTH. AFR.; S. AFR.; DA. 1973; VOL. 32; NO 3; PP. 9-10Serial Issue

VISIBLE LIGHT OBSERVATIONS OF A DENSE PLASMOID ASSOCIATED WITH A MOVING TYPE IV SOLAR RADIO BURSTSTEWART RT; DULK GA; SHERIDAN KV et al.1982; ASTRONOMY AND ASTROPHYSICS; ISSN 0004-6361; DEU; DA. 1982; VOL. 116; NO 2; PP. 217-223; BIBL. 27 REF.Article

THEORIE DE LA RADIOEMISSION SOLAIRE DE TYPE IVLEDENEV VG.1982; ASTRON. Z.; ISSN 504831; SUN; DA. 1982; VOL. 59; NO 4; PP. 742-749; ABS. ENG; BIBL. 17 REF.Article

RADIO BURSTS FROM THE SOLAR CORONAWILD JP; SMERD SF.1972; ANNU. REV. ASTR. ASTROPHYS.; U.S.A.; DA. 1972; VOL. 10; PP. 159-196; BIBL. 2P.Serial Issue

A STATISTICAL STUDY OF MOVING TYPE IV BURSTS BASED ON CULGOORA RADIOHELIOGRAPH OBSERVATIONSKAI K.1979; SOLAR PHYS.; NLD; DA. 1979; VOL. 61; NO 1; PP. 187-199; BIBL. 32 REF.Article

RADIO EVIDENCE FOR AN EXPANDING MAGNETIC ARCH BEYOND 20 SOLAR RADII.STONE RG; FAINBERG J.1975; SOLAR PHYS.; NETHERL.; DA. 1975; VOL. 42; NO 1; PP. 179-181; BIBL. 7 REF.Article

LANGMUIR-WAVE CONVERSION AS THE EXPLANATION OF MOVING TYPE IV SOLAR METER-WAVE RADIO ONTBURSTSDUNCAN RA.1981; SOL. PHYS.; ISSN 0038-0938; NLD; DA. 1981; VOL. 73; NO 1; PP. 191-204; BIBL. 40 REF.Article

RELATIONS ENTRE LES ERUPTIONS CHROMOSPHERIQUES, LES SURSAUTS RADIO DE TYPE II ET IV ET LES EPURATIONS DE RAYONS COSMIQUES SOLAIRES)ZEL'DOVICH MA; KUZHEVSKIJ BM; SAVENKO IA et al.1975; IN: ISSLED. KOSM. LUCHEJ; MOSKVA; NAUKA; DA. 1975; PP. 133-153; BIBL. 10 REF.Book Chapter

A MODEL FOR THE DEVELOPMENT OF A SOLAR OUTBURST BASED ON OBSERVATIONS WITH THE CULGOORA RADIO SPECTROGRAPH AND HELIOGRAPH.KAI K.1975; SOLAR PHYS.; NETHERL.; DA. 1975; VOL. 45; NO 1; PP. 217-226; BIBL. 18 REF.Article

ANALYSIS AND INTERPRETATION OF THE QUASIPERIODICAL STRUCTURE OF A TYPE IV BURSTPRACKA M; KARLICKY M.1979; BULL. ASTR. INST. CZECHOSL.; CSK; DA. 1979; VOL. 30; NO 5; PP. 257-273; ABS. RUS; BIBL. 53 REF.Article

A MODEL EXPLAINING TYPE IV CONTINUUM BURSTS BY COHERENT NONLINEAR INTERACTION OF BERNSTEIN WAVES.MOLLWO L; SAUER K.1977; SOLAR PHYS.; NETHERL.; DA. 1977; VOL. 51; NO 2; PP. 435-458; BIBL. 49 REF.Article

STRUCTURE FINE DE L'EMISSION CONTINU DES SURSAUTS TYPE IV AUX LONGUEURS D'ONDE METRIQUES. OBSERVATIONS ET MODELE DE SOURCECHERNOV GP.1976; ASTR. ZH.; S.S.S.R.; DA. 1976; VOL. 28; NO 4; PP. 798-811; H.T. 5; ABS. ANGL.; BIBL. 37 REF.Article

GENERATION OF INTERMEDIATE DRIFT BURSTS IN SOLAR TYPE IV RADIO CONTINUA THROUGH COUPLING OF WHISTLERS AND LANGMUIR WAVES.KUIJPERS J.1975; SOLAR PHYS.; NETHERL.; DA. 1975; VOL. 44; NO 1; PP. 173-193; BIBL. 29 REF.Article

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