Further development of data acquisition system of AGASA

por Ohoka, H, Takeda, M, Yoshida, S
Publicado 1996

The cosmic ray energy spectrum above 3 x 10$^{18}$eV measured by the Akeno Giant Air Shower Array

por Yoshida, S, Hayashida, N, Honda, K, Honda, M, Imaizumi, S, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Teshima, M, Tsushima, I, Yoshii, H
Publicado 1994

Muons ($\geq$ 1 GeV) in large extensive air showers of energies between 10$^{16.5}$eV and 10$^{19.5}$eV observed at Akeno

por Hayashida, N, Honda, K, Honda, M, Imaizumi, S, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Teshima, M, Tsushima, I, Yoshida, S, Yoshii, H
Publicado 1995

Lateral distribution of charged particles in giant air showers above 1 EeV observed by AGASA

por Yoshida, S, Hayashida, N, Honda, K, Honda, M, Imaizumi, S, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Suzuki, Y, Teshima, M, Tsushima, I, Yoshii, H
Publicado 1994

Observation of a very energetic cosmic ray well beyond the predicted 2.7 K cutoff in the primary energy spectrum

por Hayashida, N, Honda, K, Honda, M, Imaizumi, S, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Takeda, M, Teshima, M, Tsushima, I, Yoshida, S, Yoshii, H
Publicado 1994

Characteristics of Giant air showers of energies around 50 EeV observed by AGASA

por Doi, T, Hayashida, N, Honda, K, Honda, M, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Takeda, M, Teshima, M, Tsushima, I, Yoshida, S, Yoshii, H
Publicado 1996

Point source search for cosmic rays above 3 x 10$^{17}$ eV by AGASA

por Doi, T, Hayashida, N, Honda, K, Honda, M, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Takeda, M, Teshima, M, Tsushima, I, Yoshida, S, Yoshii, H
Publicado 1996

Composition of cosmic rays between 10$^{16.5}$ eV and 10$^{19.0}$ eV observed at Akeno

por Doi, T, Hayashida, N, Honda, K, Honda, M, Imaizumi, S, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Takeda, M, Teshima, M, Tsushima, I, Yoshida, S, Yoshii, H
Publicado 1996

The cosmic ray energy spectrum above 10$^{19}$ eV determined by AGASA

por Doi, T, Hayashida, N, Honda, K, Honda, M, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Takeda, M, Teshima, M, Tsushima, I, Uchihori, Y, Yoshida, S, Yoshii, H
Publicado 1997

Inclined giant air showers with energies above 10$^{19.5}$ eV observed by AGASA

por Doi, T, Hayashida, N, Honda, K, Honda, M, Inoue, N, Kadota, K, Kakimoto, F, Kamata, K, Kawaguchi, S, Kawasumi, N, Matsubara, Y, Murakami, K, Nagano, M, Ohoka, H, Souma, N, Takeda, M, Teshima, M, Tsushima, I, Uchihori, Y, Yoshida, S, Yoshii, H
Publicado 1996