4
Conferences
false
[["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]]
ICN-UNAM
1482bc95ee34f0461176da21871284c8
3
icrc2007@icrc2007.unam.mx
30th International Cosmic Ray Conference
The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.
True
Merida, Mexico
2007-07-03T08:00:00
2007-07-11T19:00:00
2005-09-26T05:04:53
2024-04-12T17:46:55
Mexico/General
Dr.
IGeof-UNAM
40af9343b8bb9d18708b4f0252d5f53c
1347
false
[["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]]
154 (8A)
1
Poster
In-orbit studies of trigger-related activity in the PAMELA anticoincidence system
Mr.
KTH
9d4196bf693f98571321ebf4da25192b
Prof.
Royal Institute of Technology
d41d8cd98f00b204e9800998ecf8427e
Dr.
Royal Institute of Technology
d41d8cd98f00b204e9800998ecf8427e
Mr.
KTH
9d4196bf693f98571321ebf4da25192b
Dr.
Royal Institute of Technology
4cc56a8e3cf2b710fd854e654b099797
Prof.
KTH, Department of Physics
b8056c84778dcbc0d7ab1bf12d008459
Merida, Mexico
Regency (Hyatt)
The PAMELA space experiment was launched into orbit on June 15th from the
Baikonur Cosmodrome, Kazakhstan, on-board a Resurs-DK1 satellite. The
primary objective for PAMELA is to accurately measure the antiproton (80
MeV - 190 GeV) and positron (50 MeV - 270 GeV) component of the cosmic
radiation. PAMELA consists of a permanent magnet spectrometer, a
time-of-flight system, an electromagnetic calorimeter, a neutron detector
and an anticoincidence system. The latter is built from plastic
scintillators which are read out by photomultipliers and is used to help
discriminate against triggers generated by out of acceptance events. The
performance of the anticoincidence system in correlation with activity
measured in the calorimeter and the spectrometer is evaluated using data
from the six first months of PAMELA operations in-orbit. In particular,
the anticoincidence activity for hadron-like and lepton-like events is
studied as a function of reconstructed rigidity, as measured by the
spectrometer.
1
More information about the venue
http://www.icrc2007.unam.mx/
link
http://www.icrc2007.unam.mx/
doc
http://indico.nucleares.unam.mx/images/word.png
word file
ppt
http://indico.nucleares.unam.mx/images/powerpoint.png
powerpoint file
pdf
http://indico.nucleares.unam.mx/images/pdf_small.png
pdf file
odt
http://indico.nucleares.unam.mx/images/writer.png
writer file
odp
http://indico.nucleares.unam.mx/images/impress.png
presentation file
ods
http://indico.nucleares.unam.mx/images/calc.png
spreadsheet file
other
http://indico.nucleares.unam.mx/images/file_small.png
unknown type file
link
http://indico.nucleares.unam.mx/images/link.png
link