{"id":32,"date":"2015-09-22T15:33:53","date_gmt":"2015-09-22T13:33:53","guid":{"rendered":"http:\/\/wp.local\/ahead\/?page_id=32"},"modified":"2020-05-07T10:36:42","modified_gmt":"2020-05-07T08:36:42","slug":"larix-ferrara","status":"publish","type":"page","link":"http:\/\/ahead.astropa.inaf.it\/index.php\/infrastructures\/larix-ferrara\/","title":{"rendered":"LARIX Ferrara &#8211; AHEAD 2015-2019"},"content":{"rendered":"<h2 style=\"text-align: center;\"><span style=\"color: #ff0000;\"><strong>AHEAD 2015-2019<\/strong><\/span><\/h2>\n<p>&nbsp;<\/p>\n<p>Web page:\u00a0<a href=\"http:\/\/larixfacility.unife.it\/\">LARIX Facility<\/a><\/p>\n<p><strong>Description of the infrastructure<\/strong><br \/>\nThe<a href=\"http:\/\/larixfacility.unife.it\/\"> LARIX<\/a> (LARge Italian X-ray facility) laboratory is located in the Scientific-Technological Pole of the\u00a0University of Ferrara in an underground building that includes a 100 m long tunnel with two large<br \/>\nexperimental rooms on each side. It hosts two hard X-ray installations, the 12 m long LARIX-A located in\u00a0the experimental room A, and the 50 m long gamma-ray facility, LARIX-T, installed in the tunnel. LARIX A\u00a0is ideal for performing linearity tests of hard X-ray detectors (e.g., Zavattini et al. 1997, NIM A 401, 206), for\u00a0reflectivity measurements of X-ray reflector samples (e.g., Frontera et al. 1991, SPIE Procs. 1549, 113,\u00a0Frontera et al. 2008, SPIE Procs. 7011, 52) and to perform ground calibration of entire hard X-ray\u00a0experiments (e.g., Loffredo et al. 2003, A&amp;A 411, L239\u2013L242, about JEM-X calibration for INTEGRAL\u00a0satellite). LARIX-T is suitable for testing gamma-ray reflectors (e.g., crystals) and low-weight gamma-ray\u00a0detector prototypes. The normal manned operating hours of the test facilities are 08:00 to 19:00 Monday to\u00a0Friday. It will not normally be possible for visitors to access the test facility out of these hours. It is not\u00a0possible to control the facility using a remote connection, all measurement sequences have to be set up via\u00a0local access. For additional informations please visit the <a href=\"http:\/\/larixfacility.unife.it\/\">LARIX<\/a> web site.<\/p>\n<p><strong><a href=\"#LARIXA\">Installation 1: LARIX-A<\/a><\/strong><br \/>\n<strong><a href=\"#LARIXT\">Installation 2: LARIX-T<\/a><\/strong><\/p>\n<p><a name=\"LARIXA\"><\/a><br \/>\n<strong>Installation 1: LARIX-A<\/strong><\/p>\n<p>LARIX-A can be operated from about 10 keV to 140 keV. its main components are described below.<br \/>\n<strong>X-ray Sources<\/strong> Two X&#8211;ray tubes, with different operational voltage, are mounted onto an optical table and powered by independent high voltage supplies. One tube is equipped with a Molybdenum anode, operating from 20 to 60 kV and current from 10 to 60 mA (Maximum operational power: 3.6 kW). The spot size is 0.5 x 0.5 mm2. The other tube is equipped with a Tungsten anode, operating from 40 to 140 kV and current from 0.1 to 5 mA (Maximum operational power: 70 W). The minimum spot size is 0.5 x 0.5 mm2. The output window of the first tube is equivalent to a 0.3 mm thick Beryllium foil, while that of the second tube is equivalent to a 1.5 mm thick aluminium foil. By means of remote controlled manipulators, both tubes can be moved up and down and translated along a direction perpendicular to the X&#8211;ray beam. Both X&#8211;ray tubes plus their translation stages are contained in a box made of a 5 mm thick Pb layer.<br \/>\n<strong>Collimators and filters<\/strong> A set of two collimators limits the divergence of the X&#8211;ray beam. Filters are available for selecting the band of interest and related fluorescence lines. Filters include different thickness high purity Copper and Aluminium tails.<br \/>\n<strong>The Monochromator system<\/strong> The polychromatic source spectrum can be monochromatized with a double crystal diffractometer (Bragg-Bragg configuration) (see Figure) providing a fixed-exit beam independently of the selected photon energy. The monochromator is installed inside a sealed plexiglass box, where helium can be pumped. The box X&#8211;ray entrance and exit windows are made of polyethylene terephthalate (PET) 0.075 mm thick with a very high transparency at the operation energies. The output X&#8211;ray beam travels in evacuated tubes (10-3 mbar) up to the sample to be tested.<br \/>\n<strong>Sample holder and Manipulators<\/strong> The sample to be tested is positioned on a pedestal equipped with manipulators that allow to move the sample in three perpendicular directions (X,Y,Z) and rotate it around the vertical and the horizontal axes. An angular position accuracy of 3&#8221; can be achieved with a repeatability of 1&#8221;.<br \/>\n<strong>X-ray detectors<\/strong> The available detectors include: 1) a large area (30 cm diameter) CsI X-ray imager, with pixel size of 300 \u00b5m; 2) a Nitrogen cooled spectrometer of high purity HPGe with a surface area of about 78 cm2, a thickness of 13 mm and an X&#8211;ray entrance window of 0.254 mm Beryllium foil; 3) a NaI(Tl) scintillator detector of 42&#215;42 mm2 and 3 mm thickness, with imaging (a few mm) and spectral (resolution of 25% at 60 keV) capabilities. The detector holder can be moved in three perpendicular axes (X,Y,Z) and is equipped with a rotation stage (3.6\u201d resolution) around the vertical.<br \/>\n<strong>Other features and remote console<\/strong> Both the sample and detector pedestals can be translated along the X-ray beam direction on 6 m long rails. An overhead travelling crane (1000 kg weight&#8211;bearing, 20 m long) is installed parallel to the rails. A clean room of 100.000 class of 12 meters square hosts the sample; it can host also the detector when the distance between sample and detector is less than 2 m. The sample holder, the detector holder and the holder of the position gauge of the sample holder, can be moved on 10 m long rails as shown in Fig. 2. The control room, equipped with a PC-based interface running under LabView, is separated from LARIX A by means of a wall 2.1 m high, made of Al+Pb. It is possible to locate the X&#8211;ray beam, measuring its energy resolution.<\/p>\n<div id='gallery-1' class='gallery galleryid-32 gallery-columns-2 gallery-size-medium'><figure class='gallery-item'>\n\t\t\t<div class='gallery-icon portrait'>\n\t\t\t\t<a href='http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image9.jpeg' title=\"\" data-rl_title=\"\" class=\"rl-gallery-link\" data-rl_caption=\"\" data-rel=\"lightbox-gallery-1\"><img loading=\"lazy\" decoding=\"async\" width=\"202\" height=\"300\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image9-202x300.jpeg\" class=\"attachment-medium size-medium\" alt=\"LARIX-A\" aria-describedby=\"gallery-1-60\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image9-202x300.jpeg 202w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image9.jpeg 537w\" sizes=\"(max-width: 202px) 100vw, 202px\" \/><\/a>\n\t\t\t<\/div>\n\t\t\t\t<figcaption class='wp-caption-text gallery-caption' id='gallery-1-60'>\n\t\t\t\tA view of the LARIX-A hard X-ray facility\n\t\t\t\t<\/figcaption><\/figure><figure class='gallery-item'>\n\t\t\t<div class='gallery-icon landscape'>\n\t\t\t\t<a href='http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image10.jpeg' title=\"\" data-rl_title=\"\" class=\"rl-gallery-link\" data-rl_caption=\"\" data-rel=\"lightbox-gallery-1\"><img loading=\"lazy\" decoding=\"async\" width=\"300\" height=\"173\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image10-300x173.jpeg\" class=\"attachment-medium size-medium\" alt=\"\" aria-describedby=\"gallery-1-61\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image10-300x173.jpeg 300w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image10.jpeg 627w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a>\n\t\t\t<\/div>\n\t\t\t\t<figcaption class='wp-caption-text gallery-caption' id='gallery-1-61'>\n\t\t\t\tLARIX-A layout, with the double crystal monochromator, the sample  and detector pedestals, and the clean room area are visible\n\t\t\t\t<\/figcaption><\/figure>\n\t\t<\/div>\n\n<p><a name=\"LARIXT\"><\/a><br \/>\n<strong>Installation 2: LARIX-T<\/strong><\/p>\n<p>LARIX-T is installed in the 100 m tunnel with a controlled access. Its operational energy range is from 60 keV to 1 MeV. Safety doors separate the tunnel from the experimental room A where the console room is located. In Figure below it is shown a sketch of the installed facility in the current configuration. Its main components are described below.<br \/>\n<strong>Gamma-ray source<\/strong> A portable betatron (Vmax = 2.5 MV, Pmax = 310 W) or an gamma-ray generator (Vmax = 320 Volts, Pmax = 1800 W) are available. The gamma-ray generator is equipped with a tube with a Tungsten anode (fine focus of 0.3 mm diameter). For the current application (Laue lens development), the source adopted is the X-ray tube (see Fig. 2.2, left panel). A 20 mm thick Tungsten plate with a 3 mm diameter hole, followed by a 50 mm thick Lead shield with a 1 mm diameter hole limit the beam divergence (Fig. 2.2, right). Either source can be translated in the plane Y-Z (X being the beam axis), and rotated around the Z and Y-axes.<br \/>\n<strong>Beamline<\/strong> The photons coming from the gamma-ray source through the initial collimator enter (X-ray entrance and exit windows of carbon fiber 3 mm thick) into a 21 m long beam-line under vacuum (of \u22641 mbar) of stainless steel with an internal diameter of 60 cm. The beamline is planned to be extended up to 70 m.<br \/>\n<strong>Final slit collimator<\/strong> A final slit collimator (see Fig. 2.3 left), mounted on a pedestal, can be translated in the Y-Z plane and rotated around the X, Y and Z axes, to get a gamma-ray pencil beam always parallel to itself and to a given direction. The slit aperture can be varied by means of four crossed and independent 20 mm thick blades of Tungsten Carbide.<br \/>\n<strong>Sample carriage and holder<\/strong> The sample to be tested is placed on a holder, that can be coarsely translated in the (X,Y) plane, and finely positioned and oriented by means of a 6-axis hexapod system. The hexapod allows uncertainties in the sample orientation of 1 arcsec and in the sample translation of 1 \u00b5m. A view of the hexapod is shown in Fig. 2.3 (right).<br \/>\n<strong>Detector system<\/strong> It includes two detectors (a gamma-ray imager and a solid-state spectrometer) placed on a carriage that can move back and forth on a 15 m long rail along the X-axis. The carriage allows also the translation of the detectors in the Y-Z plane with an uncertainties of 0.5 mm in each direction. The gamma-ray imaging detector (CsI(Tl) scintillator viewed from an array of photodiodes) has a useful area 20 x 20 cm2, with a spatial resolution 200 \u00b5m. The gamma-ray spectrometer is a cooled HPGe detector with 2.5 cm diameter with an energy resolution about 500 eV at 122 keV.<br \/>\n<strong>Clean room<\/strong> The final slit collimator, along with the sample holder, are located in a clean room (class better than 105, US FED STD 209E Cleanroom Standards) endowed with a thermal and hygrometric control (temperature within 1 C, relative humidity = 60% within 10%).<br \/>\n<strong>Gamma-ray beam monitor<\/strong> The beam intensity at the exit of the beamline is monitored using a calibrated NaI(Tl) scintillator integrated with a photomultiplier tube.<br \/>\n<strong>Console room<\/strong> All movements, except the detector translation along the gamma-ray beam direction, are motorized and remotely controlled, by a LabVIEW software interface. A selection of light indicators makes the X-ray beam (source and collimator slit) and hexapod\/sample holder automatically moving to the desired position.<\/p>\n<div id='gallery-2' class='gallery galleryid-32 gallery-columns-3 gallery-size-medium'><figure class='gallery-item'>\n\t\t\t<div class='gallery-icon portrait'>\n\t\t\t\t<a href='http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image13.png' title=\"\" data-rl_title=\"\" class=\"rl-gallery-link\" data-rl_caption=\"\" data-rel=\"lightbox-gallery-2\"><img loading=\"lazy\" decoding=\"async\" width=\"127\" height=\"156\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image13.png\" class=\"attachment-medium size-medium\" alt=\"X-ray tube for LARIX-T\" aria-describedby=\"gallery-2-64\" \/><\/a>\n\t\t\t<\/div>\n\t\t\t\t<figcaption class='wp-caption-text gallery-caption' id='gallery-2-64'>\n\t\t\t\tX-ray tube for LARIX-T. The panel shows the mechanical collimator adopted to limit the beam divergence.\n\t\t\t\t<\/figcaption><\/figure><figure class='gallery-item'>\n\t\t\t<div class='gallery-icon landscape'>\n\t\t\t\t<a href='http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image14.jpeg' title=\"\" data-rl_title=\"\" class=\"rl-gallery-link\" data-rl_caption=\"\" data-rel=\"lightbox-gallery-2\"><img loading=\"lazy\" decoding=\"async\" width=\"300\" height=\"171\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image14-300x171.jpeg\" class=\"attachment-medium size-medium\" alt=\"X-ray tube for LARIX-T\" aria-describedby=\"gallery-2-65\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image14-300x171.jpeg 300w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image14.jpeg 522w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a>\n\t\t\t<\/div>\n\t\t\t\t<figcaption class='wp-caption-text gallery-caption' id='gallery-2-65'>\n\t\t\t\tThe slit collimator with variable aperture\n\t\t\t\t<\/figcaption><\/figure><figure class='gallery-item'>\n\t\t\t<div class='gallery-icon landscape'>\n\t\t\t\t<a href='http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image15.jpeg' title=\"\" data-rl_title=\"\" class=\"rl-gallery-link\" data-rl_caption=\"\" data-rel=\"lightbox-gallery-2\"><img loading=\"lazy\" decoding=\"async\" width=\"300\" height=\"175\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image15-300x175.jpeg\" class=\"attachment-medium size-medium\" alt=\"X-ray tube for LARIX-T\" aria-describedby=\"gallery-2-66\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image15-300x175.jpeg 300w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2015\/09\/image15.jpeg 517w\" sizes=\"(max-width: 300px) 100vw, 300px\" \/><\/a>\n\t\t\t<\/div>\n\t\t\t\t<figcaption class='wp-caption-text gallery-caption' id='gallery-2-66'>\n\t\t\t\tThe hexapod\n\t\t\t\t<\/figcaption><\/figure>\n\t\t<\/div>\n\n<p><a name=\"PLAN\"><\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>AHEAD 2015-2019 &nbsp; Web page:\u00a0LARIX Facility Description of the infrastructure The LARIX (LARge Italian X-ray facility) laboratory is located in the Scientific-Technological Pole of the\u00a0University of Ferrara in an underground building that includes a 100 m long tunnel with two large experimental rooms on each side. It hosts two hard X-ray installations, the 12 m &#8230; <a title=\"LARIX Ferrara &#8211; AHEAD 2015-2019\" class=\"read-more\" href=\"http:\/\/ahead.astropa.inaf.it\/index.php\/infrastructures\/larix-ferrara\/\" aria-label=\"More on LARIX Ferrara &#8211; AHEAD 2015-2019\">Read more<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":344,"menu_order":2,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_mi_skip_tracking":false,"footnotes":""},"class_list":["post-32","page","type-page","status-publish"],"_links":{"self":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/32"}],"collection":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/comments?post=32"}],"version-history":[{"count":18,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/32\/revisions"}],"predecessor-version":[{"id":754,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/32\/revisions\/754"}],"up":[{"embeddable":true,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/344"}],"wp:attachment":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/media?parent=32"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}