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:
Charged particle acceleration in plasmas is a phenomenon that is rich in basic physics and also has great practical importance. In space plasmas the acceleration is often a result of a violent event, with the energy coming from magnetic fields, e.g. solar flares, or from strong electric fields produced in atmospheric discharges. In the laboratory plasmas, acceleration can be the result of injection of high intensity electromagnetic radiation into the plasma, as in laser-driven acceleration schemes, or the electric field induced in rapidly cooling plasmas, as in tokamak disruptions. In this talk we will describe two examples of electron beams in laboratory plasmas: runaway electrons in magnetic fusion devices and electron jets produced as a result of magnetic reconnection in laser-produced plasmas. We will discuss the characteristics and consequences of these processes, as well as their relevance for astrophysical scenarios.