1. Investigation of cosmic ray intensity variation at primary rigidity above 1.7 TV - Lee, Yiu-wa

2. The structure of the electronic component of cosmic-ray small air showers - Leung, Kon-chong

3. Emisión galáctica difusa y medida de anisotropías en la radiación cósmica de microondas en escalas angulares intermedias - Fernández Cerezo, Silvia

4. Emisión galáctica difusa y medida de anisotropías en la radiación cósmica de microondas en escalas angulares intermedias - Fernández Cerezo, Silvia

5. Estructura multifractal y aplicaciones de las fluctuaciones en cascadas atmosféricas producidas por rayos cósmicos - Faleiro Usanos, Eduardo
En este trabajo se realiza un análisis de las fluctuaciones en la distribución de partículas secundarias producidas por radiación cósmica en su interacción con la atmósfera terrestre.

6. Modelling the uv/x-ray cosmic background with CUBA - Haardt, Francesco; Madau, Piero
In this paper, I will describe the features of the numerical code CUBA, aimedat the solution of the radiative transfer equation in a cosmological context.

7. Cosmic Ray Antiprotons - Kennedy, Dallas C.
Standard particle and astrophysics predict a conventionalspectrum and abundance of secondary antiprotons consistent with all currentmeasurements.

8. Analysis of cosmic ray data - Orford, K. J.
Reviews statistical methods for 1- and 2-dimensional analysis of cosmic raydata including recent Bayesian analyses.

9. Gamma Ray Bursts and Cosmic Ray Origin - Dermer, C. D.
This paper presents the theoretical basis of the fireball/blast wave model,and some implications of recent results on GRB source models and cosmic-rayproduction from GRBs.

10. Cosmic Ray particle production - Ranft, J.
The status of some popular models to simulate hadronic and nuclearinteractions at Cosmic Ray energies is reviewed.

11. Interactions of Cosmic Ray Nuclei - Mannheim, K.; Schlickeiser, R.
We present convenient formulae for the energy losses of energetic atomicnuclei over the entire energy range relevant to the physics of cosmic rays.

12. Search for Cosmic-Ray Antideuterons - Fuke, H.; Maeno, T.; Abe, K.; Haino, S.; Makida, Y.; Matsuda, S.; Matsumoto, H.; Mitchell, J. W.; Moiseev, A. A.; Nishimura, J.; Nozaki, M.; Orito, S.; Ormes, J. F.; Sasaki, M.; Seo, E. S.; Shikaze, Y.; Streitmatter, R. E.; Suzuki, J.; Tanaka, K.; Tanizaki, K.; Yamagami, T.; Yamamoto, A.; Yamamoto, Y.; Yamato, K.; Yoshida, T.; Yoshimura, K.
We performed a search for cosmic-ray antideuterons using data collectedduring four BESS balloon flights from 1997 to 2000.

13. Models for cosmic ray interactions - Ostapchenko, S.
Special attention is payed to the remainingdiscrepancies between present hadronic MC generators and cosmic ray data.

14. Australian Cosmic Ray Modulation Research - Duldig, M. L.
Australian research into variations of the cosmic ray flux arriving at theEarth has played a pivotal role for more than 50 years.

15. Energies of Cosmic-Ray Particles - Anderson, Carl D.
Cloud chamber photographs of cosmic-ray tracks in a magnetic field up to 17,000 gauss are shown.

16. Cosmic-Ray Detection System using Internet - Hamaguchi, T.; Katsumata, M.; Nakano, E.; Takahashi, T.; Teramoto, Y.; Saito, Y.; Sasaki, Y.; Honda, M.; Honda, Y. S.
A cosmic ray detection system, consisting of standardized detector stationsconnected through the Internet, is described.

17. Cosmic Ray Acceleration at Relativistic Shock Waves - Ostrowski, M.
We consider shocks with parallel andoblique, sub- and super-luminal magnetic field configurations and withfinite-amplitude magnetic field perturbations.

18. Interpreting the Cosmic Ray Composition - Drury, L. O'C; Meyer, J. P.; Ellison, D. C
Detailed composition measurements can be a very powerful means of tracingorigins, a fact used regularly by forensic scientists and art historians.

19. Cosmic Ray Astrophysics with AMS-02 - Casadei, Diego
The AMS-02 detectorwill provide measurements with unprecedented statistics of the hadronic andleptonic cosmic rays, allowing for a better study of the Earth magnetospherethrough the secondaries produced by CR interactions in the atmosphere; of thesolar system environment through the measurement of the solar modulation over along period; of the solar system neighborhood through the measurement of theratio between unstable isotopes and stable elements; of the interstellar mediumof our Galaxy through the ratio between secondary and primary isotopes and themeasurement of proton and helium spectra.

20. Interstellar Gamma Ray Lines from Low Energy Cosmic Ray Interactions - Ramaty, Reuven
Evidence for the existence of low energy cosmic rays in the Galaxy comes fromthe COMPTEL observations of gamma ray line emission from Orion, and also fromlight element abundance data which seem to suggest a low energy rather than arelativistic Galactic cosmic ray origin for most of the light elements.

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