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.
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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:
Strong signals of energetic neutrons associated with the solar flare of 7
September 2005 were detected by using the Solar Neutron Telescopes located at
Mt. Chacaltaya in Bolivia and Mt. Sierra Negra in Mexico, Neutron Monitors
located at Mt. Chacartaya and Mexico City. The observed profiles
indicate a continuous emission of neutrons. In this paper, we present the
results of combined anal
... More
Presented by Dr. Takashi SAKO
on
4/7/2007
at
14:30
In association with an X17.0 flare on 2005 September 7, strong neutral
emissions were detected both in space and on the ground. In space, intense
emissions of gamma-rays were registered by INTEGRAL and by RHESSI during
the decay phase. Gamma-ray lines at 0.511, 2.2, 4.4, and 6.1 MeV were
observed and there was evidence for pion-decay radiation. On the ground,
relativistic neutrons were o
... More
Presented by Dr. Kyoko WATANABE
on
4/7/2007
at
14:18
It was surprising that Gigantic solar flares exceeding X-class occurred 10 times
in September, 2005, because the activity of the Sun had already been in the
declining period. More surprisingly, 4 X-class solar flares occurred in December,
2006, when the activity of the Sun was at the minimum. It is expected that
some of these flares were accompanied by the acceleration of ions, which
wou
... More
Presented by Dr. Yutaka MATSUBARA
on
4/7/2007
at
14:42
We have studied some characteristics of solar flares and surrounding medium (solar
plasma) by means of 2.223 MeV line time profile of gamma-emission from neutron
captures by hydrogen nuclei. It was composed the code with making allowance for the
main processes of neutron interactions and deceleration in the solar atmosphere,
character of neutron source, losses of neutrons and density model of
... More
Presented by Dr. Leonty MIROSHNICHENKO
on
4/7/2007
at
14:06
The solar flare of 20.01.2005 (class X7.1) was the biggest one in January
2005. It was started at 06:36 UT by GOES data, ended at 07:26 UT and the
maximum of X-ray emission was at 07:01 UT. AVS-F apparatus (CORONAS-F)
registered gamma-ray emission during rising phase of this flare in two
energy bands: 0.1-20 MeV and 2-140 MeV. The highest gamma-ray energy was
registered during this flare w
... More
The spectra and light curve of near a hundred Solar X-ray Flare events, which
were observed by SZ2/XD in the energy band of 10-800 keV during 2001, have
been investigated. The events covered from C to X-class flares, which are
shown different characters of high energy photons emission. The results will be
presented in this paper. The discussions will be made especially for 3 of the
brigh
... More
Presented by Prof. Huanyu WANG
on
4/7/2007
at
13:54
We study the Sun as an extended source of gamma-ray
emission, produced by
inverse-Compton scattering of cosmic-ray electrons with the
solar radiation. This
emission contributes to the diffuse gamma-ray background
even at large angular
distances from the Sun. While this emission is expected to
be readily detectable by
the upcoming gamma-ray satellite GLAST, the situation for
available E
... More
Presented by Mrs. Elena ORLANDO
on
4/7/2007
at
13:42
The hard X-ray (>150 keV, ACS SPI) emission during the X-class solar flares of
2006
December 5 and 6 lasted about 5 and 15 min respectively and the time profiles
show
several distinct peaks of about 1-2 min. If the time-profiles are plotted relatively
the onset of 15.4 GHz radio emission, then the hard X-ray emission of the
December 6
event would be delayed by 4 minutes in comparison wit
... More
Presented by Dr. Alexei STRUMINSKY
on
4/7/2007
at
13:30
Event calendar file
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