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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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As part of our on-going investigation of the charge-sign dependence in solar
modulation, we measured the cosmic ray positron abundance (~1GeV) on a
long duration balloon flight from Kiruna, Sweden to Victoria Island, Canada
during June 2006. Preliminary results from this flight will be presented and
compared to previous results.
Presented by Prof. Paul EVENSON
on
9/7/2007
at
16:42
The diurnal variations of GCR intensity observed by the ground NM stations
represent the anisotropic GCR flow at 1 AU. It is generally believed that the
variation of the local time of the GCR maximum intensity (phase) has 22-year
period of two sunspot cycles. However, there even exists doubt on such
anisotropy variation cycle. Those different interpretations come from the lack of
enough
... More
A bimodal distribution around the sunspot cycle maximum was suggested to
exit for solar-terrestrial parameters (Storini et al., Adv. Space Res. 31, n° 4, 895-
900, 2003). The period between the two activity peaks was called the
Gnevyshev Gap by the Rome Cosmic Ray Group (Storini and Pase, GBRSC News
5, Special Issue, 255-258, 1995) and it is world-wide accepted by the scientific
communit
... More
Presented by Dr. MARISA STORINI
on
9/7/2007
at
16:30
We calculate the temporal changes of the exponent g of the power law rigidity
R spectrum of the GCR isotropic intensity variations using neutron monitors
experimental data for four 11-year cycles of solar activity (1960–2002). The
temporal changes of the power law rigidity spectrum exponent g of the GCR
isotropic intensity variations are inversely correlated with the changes of the
GCR
... More
Presented by Prof. Michael ALANIA
on
9/7/2007
at
16:06
The relationship of long-term cosmic ray modulation with solar activity parameters
such as sunspot group number, their average heliolatitude, tilt of current sheet, and
solar magnetic field strength is analyzed. The period of 1957 - present time is under
consideration. We have used cosmic ray data obtained in the atmosphere at polar and
middle latitudes and the neutron monitor data. It is sho
... More
Presented by Prof. Yuri STOZHKOV
on
9/7/2007
at
15:54
Long-term variations and short-term fluctuations of cosmic rays affect observations
on board long-lived space missions. We have developed a parameterization of Galactic Cosmic-Ray (GCR) fluxes
for various levels of solar modulation during opposite polarity periods on the basis of experimental data.
In spite of a general agreement among different results on protons, antiprotons, electrons and p
... More
Presented by Dr. Catia Grimani GRIMANI
on
9/7/2007
at
15:30
The Altcriss project aims perform long term measurement of the radiation environment
in different points of the International Space Station. To achieve this goal, it
employs an active silicon detector, Sileye-3/Alteino, to monitor nuclei up to Iron in
the energy range above 40 MeV/n. Both long term modulation of galactic cosmic rays
going toward solar minimum and solar particles events will
... More
Presented by Dr. Marco CASOLINO
on
9/7/2007
at
15:42
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