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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.
I have read and understood the above.
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.
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The balloon-borne cosmic-ray experiment CREAM-I (Cosmic-Ray Energetics And Mass)
completed a successful 42-day flight during the 2004-2005 NASA/NSF/NSBF Antarctic
expedition. CREAM-I combines an imaging calorimeter with charge detectors and a
precision transition radiation detector (TRD). The TRD component of CREAM-I is
targeted at measuring the energy of cosmic-ray particles with charges grea
... More
Presented by Prof. Scott WAKELY
on
6/7/2007
at
13:30
This talk present preliminary results for the time-dependent cosmic-ray
propagation in the Galaxy by a fully 3-dimensional Monte Carlo simulation.
The distribution of cosmic-rays (both protons and helium nuclei) in
the Galaxy is studied on various spatial scales for both constant and variable
cosmic-ray sources.
The continuous diffuse gamma-ray emission produced by cosmic-rays during the
... More
Presented by Prof. Martin POHL
on
6/7/2007
at
14:18
The propagation of UHECRs is affected by the intergalactic magnetic
field that was produced during the course of the large scale structure
formation of the universe. Adopting a novel model based on turbulent
dynamo, the strength of the intergalactic magnetic field is estimated
from local dynamic properties of the gas flows in hydrodynamic
simulations of a concordance LCDM universe. The direc
... More
Presented by Prof. Hyesung KANG
on
6/7/2007
at
13:42
Different locations in the galaxy are unequally participating into the production
of elements and isotopes observed in the solar system. In this work, we
present a model that includes spatial dimensions as a basic element. The
backward stochastic solution introduced in this paper will allow us to determine
the abundance of each nucleus at certain energy and a single location in the
galax
... More
Presented by Dr. Ashraf FARAHAT
on
6/7/2007
at
14:06
After successful recovery of the first CREAM (Cosmic Ray Energetics And Mass)
instrument during the 2004/5 Antarctic campaign, the calorimeter was
refurbished for the third launch, planned for December 2007. In this CREAM-III
calorimeter, the optics were replaced with multi-clad fiber ribbons to enhance
the light signal. New readout electronics boards reduce noise even further than
the
... More
Many experimental results around and above the energies where the solar
modulation affects cosmic ion fluxes were quantified, debated and
conceptualized using leaky box models. These models basically exploit the
notion of equilibrium between creation and destruction processes of cosmic
ions in an undifferentiated arbitrary volume representing the Galaxy, ignoring
the galactic magnetic fi
... More
Presented by Dr. Antonio CODINO
on
6/7/2007
at
13:54
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