Browsing by Autor "Rolando Ticona"
Now showing 1 - 4 of 4
- Results Per Page
- Sort Options
Item type: Item , Combination of emulsion chamber and air shower array at Mt. Chacaltaya(American Institute of Physics, 1993) N. Kawasumi; I. Tsushima; Ken Honda; K. Hashimoto; Tsuneo Matano; K. Mori; Naoya Inoue; Rolando Ticona; Akinori Ohsawa; M. TamadaData of 34 familes with the accompanying air showers, observed by the combination of emulsion chamber and air shower array at Mt. Chacaltaya, are presented. Comparison with the simulation calculation concludes that a change is necessary in the characteristics of hadron interactions in E0≥1015 eV.Item type: Item , Estudio de las fuentes de radiación gamma Escorpión X-1 y Vela X-1 desde 10(Sup 14) eV hasta 10(Sup 17) eV(1997) Rolando Ticona; Ricardo Bustos; Julio Mas GarcíaItem type: Item , Eventos detectados en el Monte Chacaltaya en diciembre de 1996 por 12-NM64 y el experimento INCA(1997) Rolando Ticona; Antonio Carrasco; Osman BurgoaItem type: Item , Simultaneous Observation of Solar Neutrons and Effects on Terrestrial Magnetic Field in Association with a Solar Flare(American Institute of Physics, 2009) Wara Chamani; Rolando Ticona; Edgar Ricaldi; C. J. Solano Salinas; Jose A. Bellido; David Wahl; Óscar SaavedraOn November 2, 2003 at 17:03:00 UT a solar flare, registered by the GOES satellite, was also recorded by the Neutron Monitor (NM64) of Cosmic Ray Laboratory at Mount Chacaltaya. This flare affected the local geomagnetic field (F): there were variations in the intensity of the horizontal component (H), declination component (D) and vertical component (Z). Variations on these components, estimated as 71 nT, 10 deg. and 19 nT, respectively, have been observed with the Patacamaya’s Geomagnetic Observatory; as well as a net increased field (F), estimated as 66 nT, recorded by the Villa Remedios Geomagnetic Observatory. The duration of the magnetic and neutron signals was approximately 40 and 54 minutes, respectively, which shows that the flare was intense and with large emission of neutrons.