In order to enable an iCal export link, your account needs to have an API 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.
Additionally to having an API key associated with your account, exporting private event information requires the usage of a persistent signature. This enables API URLs which do not expire after a few minutes so while the setting is active, anyone in possession of the link provided can access the information. Due to this, it is extremely important that you keep these links 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 create a new key pair on the 'My Profile' page under the 'HTTP API' and update the iCalendar links afterwards.
Permanent link for public information only:
Permanent link for all public and protected information:
Relativistic microturbulent flares can be present in many astrophysical plasmas found e.g., in accretion disk coronae, pulsar wind nebulae, and gamma-ray bursts. In a diluted, magnetically-dominated plasma, an ensemble of these flares can produce a constant transfer of energy from large-scale bulk/shear motions into thermal and non-thermal particles. In a presence of a strong radiation field, the kinetic turbulent cascade is modified due to radiation drag experienced by the particles. The radiation alters the dynamics of the particle acceleration and in the extreme case even the turbulent cascade itself. In my presentation, I'll discuss our recent large-scale supercomputer simulations of these turbulent flares and their physics.