MEAN ISOTOPIC COMPOSITION OF COSMIC RAYS WITH 12<Z <OU= 26 AT 2.7 TO 3.0 GV.MAEHL RC; ISRAEL MH; KLARMANN J et al.sdIN: 13TH INT. COSMIC RAY CONF.; DENVER, COLO.; 1973; DENVER, COLO.; UNIV. DENVER; DA. S.D.; VOL. 1; PP. 115-119; BIBL. 6 REF.Conference Paper

RELATIVISTIC HEAVY COSMIC RAYSMEWALDT RA; FERNANDEZ II; ISRAEL MH et al.1973; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1973; VOL. 22; NO 1; PP. 45-65; BIBL. 1P.Serial Issue

ENERGY SPECTRA OF INDIVIDUAL COSMIC RAY ELEMENTS WITH 12<Z<28.ISRAEL MH; KLARMANN J; MAEHL RC et al.sdIN: 13TH INT. COSMIC RAY CONF.; DENVER, COLO.; 1973; DENVER, COLO.; UNIV. DENVER; DA. S.D.; VOL. 1; PP. 255-259; BIBL. 8 REF.Conference Paper

CONSTRUCTION AND PERFORMANCE OF A LARGE-AREA MULTIWIRE IONIZATION HODOSCOPE FOR USE IN A COSMIC-RAY DETECTOR.LOVE PL; TUELLER J; EPSTEIN JW et al.1977; NUCL. INSTRUM. METHODS; NETHERL.; DA. 1977; VOL. 140; NO 3; PP. 569-576; BIBL. 5 REF.Article

CHARGE AND ENERGY SPECTRA OF HEAVY COSMIC RAYS.BENEGAS JC; ISRAEL MH; KLARMANN J et al.sdIN: INT. COSMIC RAY CONF. 14; MUENCHEN; 1975; MUENCHEN; MAX PLANCK INST.; DA. S.D.; VOL. 1; PP. 251-255; BIBL. 10 REF.Conference Paper

OBSERVATION OF VH AND VVH COSMIC RAYS WITH AN IONIZATION-CERENKOV DETECTOR SYSTEMBINNS WR; FERNANDEZ JI; ISRAEL MH et al.sdIN: COSMIC RAYS. 12TH INT. CONF. HOBART, TASMANIA, AUST., 1971; HOBART, TASMANIA; MERCURY WALCH; DA. S.D.; VOL. 1; PP. 260-265; BIBL. 9REF.Conference Paper

ABUNDANCES OF COSMIC RAY NUCLEI HEAVIER THAN 50^SNWADDINGTON CJ; FICKLE RK; GARRARD TL et al.1982; INTERNATIONAL COSMIC CONFERENCE. 17/1981-07-13/PARIS; FRA; SACLAY: COMMISSARIAT A L'ENERGIE ATOMIQUE; DA. 1982; PP. 109-112; BIBL. 7 REF.Conference Paper

COMMENT ON THE OBSERVATION OF TRANSURANIC NUCLEI IN THE PRIMARY COSMIC RADIATIONBLANFORD GE JR; FRIEDLANDER MW; KLARMANN J et al.sdIN: COSMIC RAYS. 12TH INT. CONG. HOBART, TASMANIA, AUST., 1971; HOBART, TASMANIA; MERCURY WALCH; DA. S.D.; VOL. 1; PP. 269-272; BIBL. 4REF.Conference Paper

COSMIC-RAY ABUNDANCES OF ELEMENTS WITH ATOMIC NUMBER 26 <OU= Z <OU= 40 MEASURED ON HEAO 3BINNS WR; FICKLE RK; GARRARD TL et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 247; NO 3; PART. 2; PP. L115-L118; BIBL. 19 REF.Article

ABUNDANCES OF COSMIC RAY NUCLEI FOR 26 <OU= Z <OU= 40 FROM THE HEAO-3 HEAVY NUCLEI EXPERIMENTKLARMANN J; BINNS WR; ISRAEL MH et al.1981; INTERNATIONAL COSMIC RAY CONFERENCE. 17/1981/PARIS; FRA; SACLAY: COMMISSARIAT A L'ENERGIE ATOMIQUE; DA. 1981; PP. 13-16; BIBL. 5 REF.Conference Paper

THE ORIGIN AND PROPAGATION OF VVH PRIMARY COSMIC RAY PARTICLES.BLANFORD GE JR; FRIEDLANDER MW; KLARMANN J et al.sdIN: 13TH INT. COSMIC RAY CONF.; DENVER, COLO.; 1973; DENVER, COLO.; UNIV. DENVER; DA. S.D.; VOL. 1; PP. 275-279; BIBL. 12 REF.Conference Paper

IMPLICATIONS OF ULTRAHEAVY COSMIC-RAY SOURCE COMPOSITION DERIVED FROM OBSERVATIONS BY THE HEAO-3 HEAVY NUCLEI EXPERIMENTISRAEL MH; KLARMANN J; BINNS WR et al.1981; INTERNATIONAL COSMIC RAY CONFERENCE. 17/1981/PARIS; FRA; SACLAY: COMMISSARIAT A L'ENERGIE ATOMIQUE; DA. 1981; PP. 36-39; BIBL. 9 REF.Conference Paper

OBSERVATION OF LOW-CHARGE LOW-ENERGY GEOMAGNETICALLY FORBIDDEN PARTICLESBLANFORD GE JR; FRIEDLANDER MW; KLARMANN J et al.1972; J. GEOPHYS. RES.; U.S.A.; DA. 1972; VOL. 77; NO 31; PP. 6037-6041; BIBL. 11 REF.Serial Issue

PRIMARY COSMIC RAY PARTICLES WITH Z>35 (VVH PARTICLES).BLANFORD GE JR; FRIEDLANDER MW; HOPPE M et al.sdIN: 13TH INT. COSMIC RAY CONF.; DENVER, COLO.; 1973; DENVER, COLO.; UNIV. DENVER; DA. S.D.; VOL. 1; PP. 265-269; BIBL. 5 REF.Conference Paper

Rapid two-dimensional dose measurement in brachytherapy using plastic scintillator sheet : linearity, signal-to-noise ratio, and energy response characteristicsPERERA, H; WILLIAMSON, J. F; MONTHOFER, S. P et al.International journal of radiation oncology, biology, physics. 1992, Vol 23, Num 5, pp 1059-1069, issn 0360-3016Article

Cosmic-ray energy spectra between 10 and several hundred GeV per atomic mass unit for elements from ₁₈Ar to ₂₈Ni: results from HEAO 3BINNS, W. R; GARRARD, T. L; ISRAEL, M. H et al.The Astrophysical journal. 1988, Vol 324, Num 2, pp 1106-1117, issn 0004-637X, 1Article