Event calendar file
4-12 November 2010
Morelia, Michoacan
Mexico/General timezone
- arteaga@ifm.umich.mx
Support
Session I I.E.PP
Place
Location: Morelia, Michoacan
Room: Hall A, Hotel Fiesta Inn
Date:
11 Nov 16:00 - 20:00
Conveners
-
- Dr. Villaseñor, Luis (UMSNH)
Timetable | Contribution List
Displaying 7
contributions
out of
7
Type: Oral contribution
Session:
Session I I.E.PP
Track: Instrumentation and experimental particle physics
La colposcopía y la prueba de Papanicolau son estándares
mundiales (incluyendo a México) para la detección de
displasias genitales en la mujer y cáncer cervical. Los altos
costos de las tecnologías para la detección y tipificación de
VPH resulta en una falta generalizada de atención médica
oportuna. Las técnicas de amplificación de ácidos nucleicos
nos brindan informació
... More
Presented by Dr. Luis Manuel MONTANO ZETINA
on
12/11/2010
at
1:00
Type: Oral contribution
Session:
Session I I.E.PP
Track: Instrumentation and experimental particle physics
Presented by Dr. Luis Manuel VILLASEÑOR CENDEJAS
on
12/11/2010
at
0:00
Type: Invited talk
Session:
Session I I.E.PP
Track: Instrumentation and experimental particle physics
A detailed description of the MINERvA detector is presented as well as a v data set analysis for the full detector. The detector working energy range, its performance characteristics, and current analysis efforts are shown.
The Test Beam facility and its role for calibration purposes is also discussed.
Presented by Gerardo ZAVALA-GUZMAN
on
11/11/2010
at
22:00
Type: Oral contribution
Session:
Session I I.E.PP
Track: Instrumentation and experimental particle physics
We present the results of the studies of UV atmospheric flashes as a source of background in the detection of Ultra High Cosmic Rays from space. The data were obtained by using a UV detector in the Tatyana satellites I and II. Plans for near future in the new Satellite Lomonosov are presented.
Presented by Dr. Humberto SALAZAR
on
11/11/2010
at
22:30
Session:
Session I I.E.PP
We present the results of the studies of UV atmospheric flashes as a source of background in the detection of Ultra High Cosmic Rays from space. The data were obtained by using a UV detector in the Tatyana satellites I and II. Plans for near future in the new Satellite Lomonosov are presented.
Presented by Dr. Humberto SALAZAR
Type: Oral contribution
Session:
Session I I.E.PP
Track: Instrumentation and experimental particle physics
This work es centered en the study of the magnetic spectrometer used in the MINERvA Experiment (E-938 at FERMILAB), this analysis it is done from the first beginning by means of the simulation of the magnetic field in 3D view and the simulation of the pass of the charged particles across of the magnetic field generated by the two identical dipole magnets. Also the comparison appears between of an
... More
Presented by Mr. Edgar VALENCIA RODRÍGUEZ
on
11/11/2010
at
23:00
Type: Oral contribution
Session:
Session I I.E.PP
Track: Instrumentation and experimental particle physics
Presented by Dr. Ildefonso LEON MONZON
on
12/11/2010
at
0:30
