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.
Permanent link for public information only:
Permanent link for all public and protected information:
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.
Permanent link for public information only:
Permanent link for all public and protected information:
Impulsive solar energetic particle (SEP) events often show a high e/p ratio and
over-abundance of He3. The underlying acceleration mechanism of particles (electrons
and ions) in these events is still unknown. One crucial step in advancing our
understanding of the acceleration process is to deduce precisely the injection time
of electrons and ions from the observed time-intensity profiles and p
... More
Normalized cumulative particle fluence plots are very useful for characterizing the
variability of interplanetary suprathermal and energetic particle fluxes on various
time scales. For some applications it is practicable to describe the deviations of
annual fluence plots from straight lines by a single parameter (the Kolmogorov or K
parameter), and then check the dependence of that parameter o
... More
Gradual solar energetic particle (SEP) events is a major space hazard. In these
events, energetic particles (protons and heavy ions) are accelerated at propagating
CME-driven shocks, reaching energies as high as ~1 GeV/nucleon. Understanding the
acceleration and transport of these particles in the inner heliosphere is an active
research in space physics. Observationally, a tremendous amount of
... More
Ulysses, the first spacecraft ever to fly over the poles of the Sun, plays a central
role in the Heliospheric Network, the international fleet of spacecraft to explore
the Sun and Heliosphere. In November 2006, Ulysses, began its passage over
the Sun’s south pole for the third time. Although like during the first polar
passes in 1994/1995 the Sun is again close to its activity minimum, a
... More
Presented by Dr. Olga MALANDRAKI
on
5/7/2007
at
14:42
Recently, the times from CME to onset, the rise times and durations of 20 MeV
proton events observed on the Wind spacecraft during 1998-2002 were
compared with ambient solar wind O+7/O+6 values to search for correlations
with solar-wind (SW) stream types. Here we compare the same three SEP
timescales with their associated SW components classified as high-speed
streams, slow wind, and tr
... More
Based on numerical solutions of the focused transport equation we
study the question whether pitch angle diffusion coefficients calculated
from various suggested models for wave-particle interactions and different
assumptions about the nature of magnetic fluctuations in the solar wind can
lead to measurable differences in observables such as the rigidity
dependence of the mean free path and t
... More
In mid December 2006 several flares on the Sun occurred in rapid succession,
spawning several CMEs and bathing the Earth in multiple solar energetic
particle (SEP) events. One such SEP occurring on December 15th was observed
at the Earth just as an interplanetary CME (ICME) from a previous flare on
December 13th was transiting the Earth. Although solar wind observations
during this time
... More
Presented by Tamitha MULLIGAN
on
5/7/2007
at
14:18
Event calendar file
Powered by Indico