Several different activities are performed at the QEL, mainly related to the so-called VacuumUltraViolet (VUV) instrumentation. They can be divided in different sections:
Space InstrumentationAnother space mission in which QEL was indirectly interested is the Far Ultraviolet Spectroscopic Explorer (FUSE ). For this space mission, a researcher of the group spent a period of time at the Experimental Astrophysics Group of the Space Sciences Laboratory of the University of California Berkeley (USA) participating at the realization, characterization, test and alignment of the photon counting detectors of the instrument.
Another space mission in which QEL is presently involved is the realization
of the Wide Angle Camera (
WAC
) for the
OSIRIS
imager on board of the ESA
Rosetta
mission to comet P/Wirtanen. This project is a collaboration among several
departments of the University and it is coordinated by the Center for Space
Activity of the University (CISAS
). The activity related to this instrument had consisted in the definition
of the optical design of the camera, and in all the optical activities related
to its integration: from the acceptance tests of the optics (realized by
Galileo Avionica
), to the tests of the breadboard optics, to the Qualification Model alignment
and integration, to the Flight Model alignment, integration and verification
tests. The camera is planned to be launched in 2003.
Some members of QEL are also involved in the optical study and design (Phase
A) of the UV spectrometers on the Ultra-Violet Italian Sky Surveryor (UVISS)
telescope, which should be installed on the International Space Station (
ISS
).
Another space mission proposal in which QEL is involved is
Kronos
. If the mission will be approved by NASA, QEL will be responsible of the
realization of the UV/Vis spectrograph of the satellite.
Power Pulsed Lasers and Laser Produced Plasmas
Synchrotron Radiation Instrumentation
QEL is involved in the study of optical configurations for monochromators
for synchrotron radiation application. This activity has began several years
ago, with the beginning of the construction of the synchrotron ring
ELETTRA
in Trieste. One of the proposed monochromators has been approved and built
and is now working at the beamline
ALOISA
in Trieste. The monochromator design (patented) is based on the idea of using
sagittal focusing for some of the optics: this has the consequence of strongly
reducing the so-called slope error aberrations in the dispersion plane,
giving a very high resolution. Moreover, owing to its particular design,
it is the only monochromator working on synchrotron radiation beamlines which
allows the use of both gratings and crystals, so covering a very wide energy
range, with very high resolution. The actual performance of this monochromator
are extremely good, showing resolution values also beyond the expected ones.
QEL is also responsible of another monochromator at ELETTRA, namely the one
for the X-Moss beamline. Also this monochromator adopts the sagittal focusing
for reducing the slope error aberrations in the dispersione plane;
but in this case, owing to the reduced energy range of operation of the beamline,
only gratings are used as dispersive elements (no crystal). This monochromator
has been recently completed, and QEL has been the main responsible of its
alignment.
Techniques for X-ray diagnostics
Lab Activities and Miscellaneous
Several activities can be cited: