iCal export
Event calendar file
I have read and understood the above.
I have read and understood the above.
Download current event:
Event calendar file
In order to enable an iCal export link, your account needs to have a key created. This key enables other applications to access data from within Indico even when you are neither using nor logged into the Indico system yourself with the link provided. Once created, you can manage your key at any time by going to 'My Profile' and looking under the tab entitled 'HTTP API'. Further information about HTTP API keys can be found in the Indico documentation.
In conjunction with a having a key associated with your account, to have the possibility of exporting private event information necessitates the creation of a persistent key. This new key is also associated with your account and whilst it is active the data which can be obtained through using this key can be obtained by anyone in possession of the link provided. Due to this reason, it is extremely important that you keep links generated with this key private and for your use only. If you think someone else may have acquired access to a link using this key in the future, you must immediately remove it from 'My Profile' under the 'HTTP API' tab and generate a new key before regenerating iCalendar links.
Permanent link for public information only:
Permanent link for all public and protected information:
Please use CTRL + C to copy this URL
Detailed timetable
More
3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
PDF |
iCal
Calendar file
I have read and understood the above.
I have read and understood the above.
Download current session:
Calendar file
In order to enable an iCal export link, your account needs to have a key created. This key enables other applications to access data from within Indico even when you are neither using nor logged into the Indico system yourself with the link provided. Once created, you can manage your key at any time by going to 'My Profile' and looking under the tab entitled 'HTTP API'. Further information about HTTP API keys can be found in the Indico documentation.
In conjunction with a having a key associated with your account, to have the possibility of exporting private event information necessitates the creation of a persistent key. This new key is also associated with your account and whilst it is active the data which can be obtained through using this key can be obtained by anyone in possession of the link provided. Due to this reason, it is extremely important that you keep links generated with this key private and for your use only. If you think someone else may have acquired access to a link using this key in the future, you must immediately remove it from 'My Profile' under the 'HTTP API' tab and generate a new key before regenerating iCalendar links.
Permanent link for public information only:
Permanent link for all public and protected information:
Please use CTRL + C to copy this URL
HE 1.2.A
Place
Location: Merida, Mexico
Room: Yucatan II+III+IV (Fiesta Americana)
Date:
6 Jul 08:30 - 12:30
Timetable | Contribution List
We present the all-particle primary cosmic ray energy spectrum obtained by a
parametric event-by-event determination of the primary energy. The results are
obtained on the basis of an expanded experimental data from the GAMMA
experiment. The method was developed using the CORSIKA EAS simulation
code with the SYBILL interaction model and taking into account the response of
the GAMMA detec
... More
Presented by Dr. R.M. MARTIROSOV
on
6/7/2007
at
13:30
LOPES is one the pioneering experiments for the measurement of radio emission
from air showers with digital radio receivers. It is set up at the site of the
KASCADE-Grande air shower array and takes data in conjunction with it. This
gives us the unique possibility to combine LOPES and KASCADE-Grande data.
In its second phase LOPES has been extended to 30 antennas, which increases
the detect
... More
Presented by Dr. Andreas HORNEFFER
on
6/7/2007
at
15:30
Cosmic ray showers that trigger the IceTop surface array generate high energy muons
that are measured by the IceCube in-ice detector. The large surface and underground
area of this 3-dimensional instrument at completion guaranties significant statistics
for shower energy up to about 1 EeV. Since the number of muons is sensitive to the
type of the primary cosmic ray nucleus these events can be
... More
Presented by Dr. Chihwa SONG
on
6/7/2007
at
14:06
The dependence of the intensity of muon bundles detected at the Earth's surface by
means of the coordinate-tracking detector DECOR on the angle between muon arrival
direction and geomagnetic field vector (pitch angle) has been analysed. It is found
that muon bundle intensity decreases with the increase of the transverse component of
the magnetic field in comparison with calculations performed
... More
Presented by Dr. Igor YASHIN
on
6/7/2007
at
16:06
LOPES30 is a digital radio antenna array working in the frequency range 40 -- 80 MHz
with 30 dipole antennas triggered by the air shower experiment KASCADE-Grande. From
an absolute calibration the measured field strength of the LOPES30 antenna system is
known and the invesitigation of a large data set taken in east-west polarisation is
performed.
The reconstructed pulse height of the radio em
... More
Presented by Mr. Steffen NEHLS
on
6/7/2007
at
14:30
A large area streamer tube detector (128m^2), located within the KASCADE-
Grande Experiment, has been built with the aim to identify muons
(E>0.8GeV) and their direction in extensive air showers. Besides the
investigation of the muon pseudorapitity in EAS, the application of the
tracking detector in reconstructing the muon production height is
evaluated. The combination of the muon production
... More
Presented by Dr. Paul DOLL
on
6/7/2007
at
17:17
A new approach to investigations of ultra-high energy cosmic rays based on the new
EAS observable - spectra of local density of muons measured at ground level in a wide
range of zenith angles - is considered. It is shown that muon density spectra are
sensitive to the primary cosmic ray spectrum and composition, and to features of the
forward kinematic region of hadronic interaction, and thus p
... More
Presented by Dr. Igor YASHIN
on
6/7/2007
at
15:42
ARGO-YBJ is a "full coverage" air shower detector consisting of
a carpet of Resistive Plate Chambers, located at Yangbajing (4300m a.s.l.).
Using the data collected by the central detector (5800m^2 area)
the cosmic ray shadowing effect due to the Moon is studied.
The comparison of experimental results with Montecarlo simulations is
also discussed.
Presented by Dr. Bo WANG
on
6/7/2007
at
13:42
The KASCADE-Grande experiment, located at the area of the Forschungszentrum
Karlsruhe, Germany, measures extensive air showers in the energy range between
10^{14} and 10^{18} eV, thus covering the first and the second knee of cosmic rays.
Former analyses of electron and muon data of the original KASCADE experiment revealed
knee-like features in the energy spectra of light elements causing th
... More
Presented by Dr. Holger ULRICH
on
6/7/2007
at
17:05
ARGO-YBJ is a full coverage Extensive Air Shower array located by the
high-altitude cosmic rays laboratory of Yangbajing (4300 m a.s.l., Tibet,
China). The detector consists of a layer of Resistive Plate Counters covering an area of
about 5800 m^2 with 58x62 cm^2 unit cells. This design allows a detailed
characterization of cosmic ray showers induced by primaries with energy in the range
fro
... More
Presented by Dr. Giovanni MARSELLA
on
6/7/2007
at
14:18
We present an updated all-particle energy spectrum using data set collected in the
period from 2000 November through 2004 October by Tibet-III air-shower array. The
energy determination of the air showers is made by fitting the lateral density
distribution of the shower particles to the modified NKG function which is optimized
by simulation calculation using interaction models of QGSJET01c
... More
Presented by Mr. Ding CHEN
on
6/7/2007
at
13:54
Using the data taken by the ARGO-YBJ experiment (606 $g/cm^{2}$, Tibet, P.R.China)
in the period of July to September 2006, the first measurement of
EAS size spectrum in the range of $N_{e}=5\times10^{4}-5\times10^{6}$
is presented at different zenith angles. The attenuation and absorption
lengths have been determined by applying different analysis methods.
Furthermore the proton-air inelasti
... More
Presented by Dr. Min ZHA
on
6/7/2007
at
14:42
The air shower size (Ne) spectrum of cosmic rays around the knee at different zenith
angles has been studied with the Tibet-III air-shower array. The air shower size is
estimated by fitting the lateral density distribution of the shower particles using
the modified NKG function, which is optimized by the Monte Carlo simulation by using
interaction models of QGSJET01c and SIBYLL2.1 taking into
... More
Presented by Dr. Jing HUANG
on
6/7/2007
at
15:54
Previous tabNext tab
Print
Full screen
Filter
08:00
09:00
10:00
11:00
12:00
Dr. R.M. MARTIROSOV
All-particle cosmic ray energy spectrum in the 3-200 PeV energy range
08:30 - 08:42
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Bo WANG
Preliminary results of the Moon shadow using the ARGO-YBJ experiment
08:42 - 08:54
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Mr. Ding CHEN
The cosmic ray all-particle spectrum in the wide energy range from 10^{14} eV to 10^{17} eV observed with the Tibet-III air shower array
08:54 - 09:06
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Chihwa SONG
Cosmic Rays in IceCube: Composition-Sensitive Observables
09:06 - 09:18
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Giovanni MARSELLA
Study of cosmic ray showers front and time structure with ARGO-YBJ
09:18 - 09:30
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Mr. Steffen NEHLS
LOPES30 data analysis
09:30 - 09:42
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Min ZHA
Using the ARGO-YBJ experiment to determine the attenuation and the absorption lengths
09:42 - 09:54
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Andreas HORNEFFER
Calibration of the EAS Radio Pulse Height
10:30 - 10:42
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Igor YASHIN
New approach to UHE cosmic ray investigations in the energy range 10^15 - 10^19 eV
10:42 - 10:54
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Jing HUANG
Zenith angle dependence of the size spectrum of air showers around the knee observed with the Tibet air shower array
10:54 - 11:06
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Igor YASHIN
Evidences for the Influence of the Earth's Magnetic Field on EAS Muon Component
11:06 - 11:18
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Holger ULRICH
Reconstruction of primary mass group energy spectra with KASCADE
12:05 - 12:17
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Dr. Paul DOLL
Muon Production Height in the Air-Shower Experiment KASCADE-Grande.
12:17 - 12:29
Yucatan II+III+IV (Fiesta Americana), Merida, Mexico
Updating the timetable...
