BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Use of Pattern Recognition Methods in Track Analysis of Solid Dete
 ctors
DTSTART;VALUE=DATE-TIME:20161013T113000Z
DTEND;VALUE=DATE-TIME:20161013T114500Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-770@cern.ch
DESCRIPTION:Speakers: Nikolai Starkov (Lebedev Physical Institute)\nThis r
 eport is based on the results of use the PAVICOM facility in investigation
 s of nuclear and elementary particles tracks. This facility has been const
 ructed in Lebedev Physical Institute and includes three automatic microsco
 pes. They allow to analyse particles tracks in different kinds of material
 : nuclear photo emulsion\, plastic and minerals (olivine). As a result the
  images of tracks and their geometrical characteristics very differ in var
 ious experiments. This circumstance demands use of various image recogniti
 on methods depending on properties of images and aims of experiment. Durin
 g work in different experiments the PAVICOM group designed numerous algori
 thms of processing particles tracks in complicated events. In this report 
 some of them are represented.\n\nhttps://indico.particle.mephi.ru/event/4/
 contributions/770/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/770/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Background rejection methods for tens of TeV gamma-ray astronomy a
 pplicable to wide angle timing arrays
DTSTART;VALUE=DATE-TIME:20161013T114500Z
DTEND;VALUE=DATE-TIME:20161013T120000Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-757@cern.ch
DESCRIPTION:Speakers: abeer El shoukrofy (SINP MSU- Damanhour university)\
 nA 'knee-like' approximation of Cherenkov light Lateral Distribution Funct
 ions\, which we developed earlier\, now is used for the actual tasks of ba
 ckground rejection methods for high energy (Tens and hundreds of TeV) gamm
 a-ray astronomy. We use our methods basically for HiSCORE wide angle timin
 g array consisting of Cherenkov light detectors with spacing 100 m covered
  0.2 km2 presently and up to 5 km2 in future. However\, it can be applied 
 for other similar arrays. It is shown that application of multivariable ap
 proach (where 4 parameters of knee-like approximation are used) allows to 
 reach a large factor of background rejection but it strongly depends on nu
 mber of hit detectors.\n\nhttps://indico.particle.mephi.ru/event/4/contrib
 utions/757/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/757/
END:VEVENT
BEGIN:VEVENT
SUMMARY:TWO-DIMENTIONAL HYBRID SOLID STATE GAS DETECTOR BASED ON 10B LAYER
   FOR THERMAL AND COLD NEUTRONS
DTSTART;VALUE=DATE-TIME:20161013T120000Z
DTEND;VALUE=DATE-TIME:20161013T121500Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-752@cern.ch
DESCRIPTION:Speakers: Stanislav Potashev (Institute for Nuclear Research o
 f the Russian Academy of Sciences)\nPotashev S.\, Burmistrov Yu.\, Drachev
  A.\, Karaevsky S.\, Konobeevski E.\, Zuyev S.\nInstitute for Nuclear Rese
 arch\, Russian Academy of Sciences\, 117312\, Moscow\, Russia \nE-mail: po
 tashev@inr.ru\n\nTwo-dimensional hybrid solid state gas multiwire detector
  of thermal and cold neutrons [1] is created at the Institute for Nuclear 
 Research. The detector has an active area of 128 x 128 mm2 with double gas
  gap of 2 mm and a 10B converter. The input window is made of a thin alumi
 num layer (3mm) to prevent scattering and absorption of neutrons. The oper
 ation of the detector was studied using W-Be photoneutron source. The phot
 oneutron source (IN-LUE) was created on the base of industrial electron li
 nac LUE-8 operating at electron energy of 7 - 8 MeV\, tungsten electron-ga
 mma convertor\, photoneutron beryllium target and moderator of fast neutro
 ns. The detector is located at a distance of 6 m from the source at an ang
 le of 60 relative to the electron beam axis. The detector efficiency is es
 timated as ~3% at neutron wavelength λ = 1.82 Å and 6% at λ = 8 Å. The
  efficiency of the background detection was less than 0.001% of that for t
 hermal neutrons. The resulting pulse height resolution is 15% and the spat
 ial resolution is 2.5 mm for the X coordinate with gas mixture Ar + 25% CO
 2 + 0.3% CF3Br under standard conditions. The resistive charge-division re
 adout is applied to determine neutron position from pulse height values.\n
 \n    1. Litvin V.S.\, Potashev S.I.\, Razin V.I. and Sadykov R.A. Bull. R
 uss. Acad. Sci. 75\, 229 (2011).\n\nhttps://indico.particle.mephi.ru/event
 /4/contributions/752/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/752/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Detector of the reactor AntiNeutrino based on Solid-state plastic 
 Scintillator (DANSS). Status and first results.
DTSTART;VALUE=DATE-TIME:20161013T101500Z
DTEND;VALUE=DATE-TIME:20161013T103000Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-707@cern.ch
DESCRIPTION:Speakers: Igor Alekseev (ITEP)\nA detector of the reactor anti
 neutrino based on a cubic meter of plastic scintillator is installed below
  3.1 GW industrial reactor. The detector is placed on a movable platform w
 hich allows to change the distance from the reactor core center in the ran
 ge 10.7-12.7 m. 2500 scintillator strips are readout individually by SiPMs
  and in groups of 50 by PMTs. In addition to the overburden by the reactor
  (~50 m w.e.) the detector has multilayer passive shielding and active muo
 n-veto.\n\nInverse beta-decay count rate of about 5000 events per day in t
 he fiducial volume (78% of the detector) with bout 5% of cosmic background
  has been reached. DANSS is sensitive to sterile neutrino in the most inte
 resting region of mixing parameter space.\n\nThe talk will cover the detec
 tor status and performance\, as well as the first results.\n\nhttps://indi
 co.particle.mephi.ru/event/4/contributions/707/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/707/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Polarized proton and antiproton beams for the SPASCHARM experiment
  at U-70 accelerator
DTSTART;VALUE=DATE-TIME:20161013T110000Z
DTEND;VALUE=DATE-TIME:20161013T111500Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-595@cern.ch
DESCRIPTION:Speakers: Vladimir Rykov (National Research Nuclear University
  MEPhI)\nThe design\, layout and parameters of the polarized-beam facility
  at U-70 proton synchrotron of IHEP\, Protvino\, are presented. The polari
 zed proton and antiproton beam line 24A is currently under development at 
 IHEP. It will serve as a main playground for carrying out the rich program
  of the SPASCHARM experiment for comprehensive studies of spin phenomena i
 n a wide variety of hadronic reactions in the beam energy range of ~10-45 
 GeV.\n\nhttps://indico.particle.mephi.ru/event/4/contributions/595/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/595/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Tagging system for the polarized beams at U-70 accelerator
DTSTART;VALUE=DATE-TIME:20161013T111500Z
DTEND;VALUE=DATE-TIME:20161013T113000Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-564@cern.ch
DESCRIPTION:Speakers: Pavel Semenov (IHEP\,  MEPhI)\nA beam line of polari
 zed protons and antiprotons\, obtained from decays of Λ (anti-Λ)-hyperon
 s for SPASCHARM experiment at U-70 accelerator is under development at IHE
 P\, Protvino.  For precise asymmetry measurements one needs to know beam p
 olarization with a relatively low error. Tagging of the beam particle prov
 ides a possibility to perform measurements for both polarizations of the b
 eam at the same time to reduce systematic errors and increase statics.\nBe
 am tagging station will measure both polarization and beam particle moment
 a on-line. The correlation between the position of the proton (antiproton)
  with respect to the channel axis and the value of its polarization is use
 d to measure the relative polarization.  The system of detectors with good
  spatial resolution designed for those measurements as an integral part of
  the beam line of polarized particles is discussed in the report\n\nhttps:
 //indico.particle.mephi.ru/event/4/contributions/564/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/564/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Universal Main Magnetic Focus Ion Source: A New Tool for Laborator
 y Research of Astrophysics and Tokamak Microplasma
DTSTART;VALUE=DATE-TIME:20161013T104500Z
DTEND;VALUE=DATE-TIME:20161013T110000Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-480@cern.ch
DESCRIPTION:Speakers: VLADIMIR OVSYANNIKOV (Dresden MaMFIS Group)\nA novel
  room-temperature ion source for the production of  ions with charges from
  $2^{+}$ up to $80^+$ in electron beam within wide ranges of electron ener
 gy $E_e$ (500 eV $\\leq E_e \\leq 60$ keV) and current density $j_e$ ($10$
  A/cm$^2 \\leq j_e \\leq 20$ kA/cm$^2$) is developed. Due to combination o
 f two methods of sequential ionization of atoms\, the device can operate b
 oth as conventional Electron Beam Ion Source/Trap (EBIS/T) and novel Main 
 Magnetic Focus Ion Source (MaMFIS). In EBIS/T\, ions confined in the poten
 tial well are stored in the smooth electron beam going through a few drift
  tubes with positive potentials applied at the edge sections. In MaMFIS\, 
 the local ion traps with extremely high electron current density are forme
 d in crossovers of the rippled electron beam in a thick magnetic lens [1\,
 2].  The device is suitable for generation of both the low- and high-densi
 ty microplasma in steady state\, which can be employed for investigation o
 f a wide range of physical problems in an ordinary university laboratory\,
  in particular\, for astrophysics and Tokamak microplasma simulation. For 
 the electron beam characterized by the incident energy $E_e = 10$ keV\, th
 e current density $j_e \\sim 20$ kA/cm$^2$ and the number density $n_e \\s
 im 2 \\cdot 10^{13}$ cm$^{-3}$ were achieved experimentally [1-3]. For $E_
 e \\sim 60$ keV\, the value of electron number density $n_e \\sim 10^{14}$
  cm$^{-3}$ is feasible. The efficiency of MaMFIS for laboratory astrophysi
 cs significantly exceeds that of the existing warm EBIT at the National As
 tronomical Observatory of China and superconducting EBITs at the Lawrence 
 Livermore National Laboratory and the Harvard-Smithsonian Center for Astro
 physics.\n\n\nReferences\n\n[1] V. P. Ovsyannikov and A. V. Nefiodov\, Nuc
 l. Inst. Meth. B **367**\, 1 (2016). \n\n[2] V. P. Ovsyannikov and A. V. N
 efiodov\, Nucl. Inst. Meth. B **370**\, 32 (2016).\n\n[3]  A. Borovik\, Jr
 \, J. Dreiling\, R. Silwal\, E. Takács\, J. Gillaspy\, R. Lomsadze\, \nV.
  Ovsyannikov\, K. Huber\, S. Schippers\, A.  Müller\, and Yu. Ralchenko\,
  \n18th Int. Conf. on the Physics of Highly Charged Ions\, 2016\, Kielce\,
  Poland\, \nBook of Abstracts\, p. 44.\n\nhttps://indico.particle.mephi.ru
 /event/4/contributions/480/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/480/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Silicon-Gas Pixel Detector
DTSTART;VALUE=DATE-TIME:20161013T103000Z
DTEND;VALUE=DATE-TIME:20161013T104500Z
DTSTAMP;VALUE=DATE-TIME:20260814T154359Z
UID:indico-contribution-82-479@cern.ch
DESCRIPTION:Speakers: GEORGY BASHINDZHAGYAN (Lomonosov Moscow State Univer
 sity)\nThe proposed device combines the advantages of Silicon and Gas-pixe
 l detectors.\n7 micron space resolution and down to 0.2 degree both angles
  measurements\n are inside 10 mm thick and very low material detector.\nBi
 nary readout\, advanced data collection and preliminary analysis logic all
 ow to obtain \nall the information in less than 1 microsecond and to use i
 t for the fast trigger generation.\n\nhttps://indico.particle.mephi.ru/eve
 nt/4/contributions/479/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/479/
END:VEVENT
END:VCALENDAR
