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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.
I have read and understood the above.
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Problems in observation of extensive air showers generated by neutrinos are connected
with an extremely small cross section of inelastic collisions of neutrinos with
nuclei. However, two facts allow to search for showers generated by neutrinos: (1) a
hadron cascade with the primary energy of more than 10^13 eV leaves a mountain ridge
to the atmosphere from the depth ~ 300g/cm^2 without an esse
... More
Presented by Prof. Vera Georgievna SINITSYNA
on
9/7/2007
at
17:41
We calculate the flux of neutrinos generated by the propagation of
ultra-high energy nuclei over cosmological distances. The propagation takes into
account the interactions with cosmic background radiations including the CMB
and the most recent estimates of higher energy (infra-red, optical, and ultra violet)
backgrounds. We assume that the composition of ultra-high energy cosmic rays
(UHECRs
... More
Presented by Dr. Nicolás BUSCA
on
9/7/2007
at
18:17
We calculate the yield and flavor content of high energy neutrinos
produced in astrophysical sources with and without magnetic fields
varying their interaction depth.
We pay special attention to the multiple scattering of secondaries
on background photons as well as the direct production of neutrinos
in decays of charm mesons.
If multiple scattering of nucleons becomes important, the ne
... More
Presented by Dr. Ricard TOMAS
on
9/7/2007
at
18:05
Potential sources for the ultrahigh energy cosmic ray flux are
extragalactic source types such as active galactic nuclei and gama ray
busts. With the prediction of hadronic processes in these sources, a
diffuse neutrino flux ca be produced together with the charged cosmic ray
component. To measure this diffuse neutrino flux is one of the main goals
of the Antarctic Muon And Neutrino Detector
... More
A series of ice properties' measurements were made in December, 2006 in support of
the balloon-borne ANITA neutrino detection effort. Of particular importance is the
electric field attenuation length in the range 200-1000 MHz as well as signal
transmission across the air-ice boundary. We present measurements of the temperature
profile over the upper 100 meters of ice, radiofrequency attenuatio
... More
Presented by Steven W. BARWICK
on
9/7/2007
at
17:17
The RICE experiment, located at the South Pole, seeks detection of ultra-high energy
neutrinos based on measurement of the coherent radiofrequency Cherenkov pulse created
by an englacial neutrino-ice collision. Based on the eight-year dataset now
accumulated by RICE, we report on updated results on the neutrino flux in the >100
PeV energy range, limits on neutrino production from gamma-ray bur
... More
The ANTARES collaboration is building an undersea neutrino telescope at 2400
m depth in the Mediterranean Sea. The experiment aims to detect high-energy
cosmic neutrinos using a 3D array of 900 photomultipliers (PMTs) arranged in
12 strings. The advantages of neutrinos as astrophysical and cosmic
messengers are that they open a new window to observe known astrophysical
objects as well as to l
... More
Presented by Dr. Elisa FALCHINI
on
9/7/2007
at
17:29
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