In order to get higher efficiencies for detecting hadrons and to make technical improvements in the chamber structure, the Mt. Kambala Emulsion Chamber Collaboration constructed 57 sq. m. of Fe chamber, with thickness 29 c.u.(1c.u.=17.6 mm Fe), using 300 tons of Fe plates and made the first exposure from Sept., 1982 to May, 1984. The photosensitive layers consist of X-ray films of Sakura N type, Fuji No. 100 type and Tianjin III type, some of them contain also emulsion plates of Fuji ET7B type. They are inserted between the Fe plates at 2 c.u., beginning at 5 c.u. from the chamber top. In a number of blocks, 3 mm spacings are provided at every 2 c.u. of Fe plates to facilitate the replacement of photosensitive layers, without disassembling ...
The penetrating nature of the cascade showers observed in the Chacaltaya two-storey chamber is compa...
Gamma-families with total energy greater than 10 TeV, found in the EX chamber which was cooperated w...
A high energy event of a bundle of electrons, gamma rays and hadronic gamma rays in an air shower co...
The energy spectra of atmospheric cosmic rays at Mt. Kanbala (520 g/sq cm.) are measured with emulsi...
A detailed description of the event detected in the second chamber of Japan-URSS Collaboration is pr...
Information on the fragmentation region in super high energy hadronic interactions can be obtained t...
At present the study of nuclear interactions induced by cosmic rays is the unique source of informat...
The results of analysis on a cosmic-ray induced nuclear event with the total visible energy approx. ...
The energy spectra of high energy gamma-rays and hadrons were obtained by the emulsion chamber with ...
Experimental results from Emulsion Chamber (EC) experiments at mountain altitudes or at higher level...
Much efforts have been expended to observe the spectrum of electrons in the high energy region with ...
The results are presented for the systematic measurement of cosmic ray showers in the first carbon c...
About 30% of single core showers with E (sup gamma) 10 TeV have stronger penetrating power than tha...
The characteristics of hadrons of energy > 300 Gev in extensive air showers of size 5.10(^4) - 1.6.1...
In 1982 a hybrid electronic counter-emulsion chamber experiment was flown on a balloon to study heav...
The penetrating nature of the cascade showers observed in the Chacaltaya two-storey chamber is compa...
Gamma-families with total energy greater than 10 TeV, found in the EX chamber which was cooperated w...
A high energy event of a bundle of electrons, gamma rays and hadronic gamma rays in an air shower co...
The energy spectra of atmospheric cosmic rays at Mt. Kanbala (520 g/sq cm.) are measured with emulsi...
A detailed description of the event detected in the second chamber of Japan-URSS Collaboration is pr...
Information on the fragmentation region in super high energy hadronic interactions can be obtained t...
At present the study of nuclear interactions induced by cosmic rays is the unique source of informat...
The results of analysis on a cosmic-ray induced nuclear event with the total visible energy approx. ...
The energy spectra of high energy gamma-rays and hadrons were obtained by the emulsion chamber with ...
Experimental results from Emulsion Chamber (EC) experiments at mountain altitudes or at higher level...
Much efforts have been expended to observe the spectrum of electrons in the high energy region with ...
The results are presented for the systematic measurement of cosmic ray showers in the first carbon c...
About 30% of single core showers with E (sup gamma) 10 TeV have stronger penetrating power than tha...
The characteristics of hadrons of energy > 300 Gev in extensive air showers of size 5.10(^4) - 1.6.1...
In 1982 a hybrid electronic counter-emulsion chamber experiment was flown on a balloon to study heav...
The penetrating nature of the cascade showers observed in the Chacaltaya two-storey chamber is compa...
Gamma-families with total energy greater than 10 TeV, found in the EX chamber which was cooperated w...
A high energy event of a bundle of electrons, gamma rays and hadronic gamma rays in an air shower co...