BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:First Aerosol Concentration Measurements at the Auger North Site
DTSTART:20100914T193000Z
DTEND:20100914T200000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1834@events.icecube.wisc.edu
DESCRIPTION:Speakers: Maria Isabel Micheletti\n\nMicheletti\, María Isabe
 l\, Freire\, Martín\, Coco\, Michael\, Wiencke\, Lawrence\, Piacentini\, 
 Rubén \n\nWe performed the first aerosol concentration measurements at th
 e Auger North site at Lamar\, Colorado\, during summer 2010\, with the Gri
 mm 1.109 spectrometer. We evaluate the time evolution –along the hours o
 f the days and the days of the measurement period– of the concentrations
  and their mean and extreme values for particles of sizes bigger than 0.22
  microns.\n\nhttps://events.icecube.wisc.edu/event/30/contributions/1834/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1834/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Measurement of the Aerosol Phase Function by the Central Laser Fac
 ility at the Pierre Auger Observatory
DTSTART:20100914T200000Z
DTEND:20100914T203000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1835@events.icecube.wisc.edu
DESCRIPTION:Speakers: Karim Louedec\n\nIn the Pierre Auger Observatory\, t
 he Central Laser Facility (or CLF) emits all along the night laser shots i
 n the field of view of the four fluorescence buildings. The goal of this t
 alk is to show how it is possible to monitor the aerosols during the night
 . Two obtained quantities should be present: the Aerosol Phase Function (l
 inked to the probability density function of the scattering angles) and th
 e Aerosol attenuation length (linked to the aerosol concentration).\n\nhtt
 ps://events.icecube.wisc.edu/event/30/contributions/1835/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1835/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Identifying Clouds over the Pierre Auger Observatory using Satelli
 te Data
DTSTART:20100914T210000Z
DTEND:20100914T213000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1836@events.icecube.wisc.edu
DESCRIPTION:Speakers: Johana Chirinos\n\nWe describe a new method of ident
 ifying clouds over the Pierre Auger Observatory using infrared data from t
 he Imager instrument on the GOES-12 satellite. For the pixel covering the 
 Central Laser Facility(CLF) we compare cloud identifications with this met
 hod to those made with the Fluorescence Detector observations of CLF verti
 cal laser events. The methods agree. We develop cloud probability maps of 
 the array.\n\nhttps://events.icecube.wisc.edu/event/30/contributions/1836/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1836/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Development of an IR All-Sky Cloud Monitor for the LSST Site
DTSTART:20100914T213000Z
DTEND:20100914T220000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1837@events.icecube.wisc.edu
DESCRIPTION:Speakers: Jacques Sebag\n\nhttps://events.icecube.wisc.edu/eve
 nt/30/contributions/1837/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1837/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Logistics and Overview
DTSTART:20100913T140000Z
DTEND:20100913T143000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1838@events.icecube.wisc.edu
DESCRIPTION:Speakers: Segev BenZvi (University of Wisconsin--Madison)\n\nh
 ttps://events.icecube.wisc.edu/event/30/contributions/1838/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1838/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Breakfast and Registration
DTSTART:20100913T133000Z
DTEND:20100913T140000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1839@events.icecube.wisc.edu
DESCRIPTION:https://events.icecube.wisc.edu/event/30/contributions/1839/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1839/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Towards Poisson-Limited Photometric Precision from Ground-Based Te
 lescopes
DTSTART:20100913T154500Z
DTEND:20100913T161500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1840@events.icecube.wisc.edu
DESCRIPTION:Speakers: Peter Zimmer (University of New Mexico)\n\nGround-Ba
 sed Telescopes supported by lidar and calibrated spectrophotometry can att
 ain levels of precision for all-sky photometry previously only attainable 
 from space-based instruments\, with uncertainties dominated by fundamental
  photon counting statistics and detector noise. Earth’s atmosphere is a 
 wavelength-\, directionally- and time-dependent turbid refractive element 
 for every ground-based telescope\, and is the primary factor limiting phot
 ometric measurement precision. To correct accurately for the transmission 
 of the atmosphere requires direct measurements of the wavelength-dependent
  transmission in the direction and at the time that the supported photomet
 ric telescope is acquiring its data. While considerable resources have bee
 n devoted to correcting the effects of the atmosphere on resolution\, the 
 effects on precision photometry have largely been ignored. We describe the
  facility-class lidar that observes the stable stratosphere\, and a spectr
 ophotometer that creates and maintains NIST absolutely calibrated standard
  stars\, the combination of which enables fundamentally statistically limi
 ted photometric precision. This inexpensive and replicable instrument suit
 e provides the lidar-determined monochromatic transmission of Earth’s at
 mosphere at visible and near-infrared wavelengths to 0.25% per airmass and
  the wavelength-dependent transparency to less than 1% uncertainty per min
 ute. The atmospheric data are merged to create a metadata stream that allo
 ws throughput corrections from data acquired at the time of the scientific
  observations to be applied to broadband and spectrophotometric scientific
  data. This new technique replaces the classical use of nightly mean atmos
 pheric extinction coefficients\, which invoke a stationary and plane-paral
 lel atmosphere and ultimately limit ground-based all-sky photometry to 1% 
 - 2% precision. We demonstrate application of this instrument suite to ste
 llar photometry\, and discuss the enhanced value of routinely provably pre
 cise photometry obtained with existing and future ground-based telescopes.
 \n\nhttps://events.icecube.wisc.edu/event/30/contributions/1840/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1840/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The Astronomical Flux Measurement Problem: Implications for Atmosp
 heric Monitoring
DTSTART:20100913T143000Z
DTEND:20100913T151500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1841@events.icecube.wisc.edu
DESCRIPTION:Speakers: Christopher Stubbs (Harvard University)\n\nI will pr
 ovide an overview of the motivation for direct determination of atmospheri
 c transmission\, from the standpoint of broadband photometric measurements
 . The primary sources of variability (or unpredictability) in transmission
  are clouds\, aerosols and water vapor. I will review our approach to date
 \, and the results we have obtained from initial prototype instruments.\n\
 nhttps://events.icecube.wisc.edu/event/30/contributions/1841/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1841/
END:VEVENT
BEGIN:VEVENT
SUMMARY:General Discussion
DTSTART:20100913T164500Z
DTEND:20100913T171500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1842@events.icecube.wisc.edu
DESCRIPTION:https://events.icecube.wisc.edu/event/30/contributions/1842/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1842/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The NIST Standard Stars Project: Sub-1% Absolute Stellar Photometr
 y
DTSTART:20100913T161500Z
DTEND:20100913T164500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1843@events.icecube.wisc.edu
DESCRIPTION:Speakers: John Woodward (NIST)\n\nNIST has undertaken a campai
 gn to spectrophotometrically calibrate a suite of standard stars for top-o
 f-the-atmosphere flux to a precision of better than 1%. We will describe o
 ur experimental approach and show some preliminary results. In addition to
  high quality spectrophotometric measurements\, this project requires prec
 ise measurements of the atmospheric transmission in both the horizontal di
 rection and along the line of site from the observing telescope to the sta
 r. We are actively seeking input from the astronomical community on both o
 ur experimental approach and useful targets for inclusion in the catalog.\
 n\nhttps://events.icecube.wisc.edu/event/30/contributions/1843/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1843/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Global Atmospheric Model Data for the Pierre Auger Observatory
DTSTART:20100913T194500Z
DTEND:20100913T201500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1844@events.icecube.wisc.edu
DESCRIPTION:Speakers: Bianca Keilhauer (KIT)\n\nB. Keilhauer\, D. Epperlei
 n\, M. Will for the Pierre Auger Collaboration \n\nFor the reconstruction 
 of extensive air showers\, the atmospheric conditions at the site of the o
 bservatory have to be known quite well. This is particularly true for reco
 nstructions based on data obtained by the fluorescence technique. For thes
 e data not only the weather conditions near ground are relevant\, most imp
 ortant are altitude-dependent atmospheric profiles. For the Pierre Auger O
 bservatory\, we have investigated the application of “Global Data Assimi
 lation System” (GDAS) data which provide vertical atmospheric profiles f
 or height\, temperature\, and humidity at 23 constant pressure levels ever
 y 3 hours. GDAS data are available for the whole globe with 1° longitude 
 and latitude spacing. These atmospheric data are compared with observation
 s at the sites of the Auger Observatory using meteorological radio soundin
 gs. Finally\, the atmospheric data are included in the reconstruction fram
 ework of the Auger Observatory and effects on reconstruction results of re
 al air shower events are investigated.\n\nhttps://events.icecube.wisc.edu/
 event/30/contributions/1844/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1844/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Atmospheric Temperature and Water Vapor Profiles\, Transmittance C
 alculations\, and Radiative Transfer
DTSTART:20100913T190000Z
DTEND:20100913T194500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1845@events.icecube.wisc.edu
DESCRIPTION:Speakers: Ralf Bennartz (UW-Madison)\n\nThis talk will cover c
 over three areas potentially of interest to the workshop: \n\n* Numerical 
 Weather Forecasting Models estimates of temperature/water vapor profiles f
 rom satellite \n\n* Remote sensing of temperature/water vapor profiles fro
 m satellite. \n\n* Broad-band and monochromatic transmittance calculations
  and radiative transfer in the visible and near-infrared with special emph
 asize on gas absorption.\n\nhttps://events.icecube.wisc.edu/event/30/contr
 ibutions/1845/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1845/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Mesospheric Lidar Studies from Cerro Pachon\, Chile
DTSTART:20100913T211500Z
DTEND:20100913T214500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1846@events.icecube.wisc.edu
DESCRIPTION:Speakers: Gary Swenson (U of Illinois - Champaign Urbana)\n\nT
 he Remote Sensing and Space Science group at the U of I has developed an u
 pper atmospheric observatory on Cerro Pachon\, beginning operation in Sep\
 , 2009. Passive instrumentation includes mesospheric airglow allsky imager
 s of OH (including 16 micron)\, airglow photometers\, a meteor radar\, and
  an Na resonance lidar.\n\nhttps://events.icecube.wisc.edu/event/30/contri
 butions/1846/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1846/
END:VEVENT
BEGIN:VEVENT
SUMMARY:HSRL Lidar
DTSTART:20100913T204500Z
DTEND:20100913T211500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1847@events.icecube.wisc.edu
DESCRIPTION:Speakers: E. Eloranta\n\nE. Eloranta\n\nhttps://events.icecube
 .wisc.edu/event/30/contributions/1847/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1847/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Present and Future Status of LIDAR systems of HESS and CTA
DTSTART:20100913T221500Z
DTEND:20100913T224500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1848@events.icecube.wisc.edu
DESCRIPTION:Speakers: Georges Vasileiadis (LPTA/CNRS)\n\nhttps://events.ic
 ecube.wisc.edu/event/30/contributions/1848/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1848/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Toward Comparison of RAMAN and HSRL LIDAR Technique for CTA-Type A
 tmospheric Monitoring
DTSTART:20100913T214500Z
DTEND:20100913T221500Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1849@events.icecube.wisc.edu
DESCRIPTION:Speakers: Emmanuel Fokitis (Nat Tech Athens)\n\nP. Fetfatzis\,
  E. Fokitis\, V. Gika\, G.Koutelieris\, G.Koutsourakis\, H. Koubli\, S. Ma
 ltezos\, N. Maragos\, A. Aravantinos\,\, M. Kompitsas\n\nThis work describ
 es the HSRL activity at NTUA and the possibility to receive simultaneously
  data with a RAMAN lidar operating at NTUA campus. We believe that such a 
 preliminary study would be a useful study as the hardware for RAMAN LIDAR 
 is already available and operating at NTUA and significant progress has be
 en made in development HSRL prototypes for 532 and 355 nm Fabry-Perot rece
 ivers while the laser transmitters are independent from the ones used for 
 the RAMAN LIDAR system. The Raman LIDAR data have been published in severa
 l Journals and include results in the framework of EARLINET EU funded proj
 ect. The Raman LIDAR has capabilities to record aerosol extinction\, ozon 
 and water vapour profiles. The present phase of the work focuses on the st
 udy for the mounting of both the aerosol and molecular channel etalon\, a 
 receiver Newtonian telescope and optical fiber to transmit to the two chan
 nels the collected signal from the scattering volume by the telescope. Pre
 liminary lab results with He-Ne laser with several longitutinal modes anal
 yzed by a 50 mm spacer etalon are discussed. The UV sensitive etalon perfo
 rmance is studied. The mount technique considered for the molecular UV cha
 nnel is of the type of Hansen mount applied to the Dynamics Explorer etalo
 n with 2 mm spacer thickness\, while for the aerosol type we have followed
  the 10 cm hollow Zerodure cylinder spacer . The coating technique for the
  aerosol channel etalon plate pair has been selected to correspond to soft
  coating with proposed reflectance curve peaking at 380 nm (R= 98%)\, whil
 e at 355 nm R=92%.\n\nhttps://events.icecube.wisc.edu/event/30/contributio
 ns/1849/
LOCATION:Old Madison 3rd Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1849/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The Pierre Auger Atmospheric Monitoring program - Status and Futur
 e Plans
DTSTART:20100914T143000Z
DTEND:20100914T150000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1850@events.icecube.wisc.edu
DESCRIPTION:Speakers: Lawrence Wiencke\n\nThe Pierre Auger Observatory use
 s the atmosphere as a giant calorimeter to measure extensive air showers p
 roduced by the highest energy particles known to exist. The Southern hemis
 phere site is operational and includes an array of instruments that monito
 r the troposphere above the 3000 km^2 site. A Northern hemisphere site of 
 20\,000 km^2 is planned. This talk will review the atmospheric monitoring 
 program of the observatory.\n\nhttps://events.icecube.wisc.edu/event/30/co
 ntributions/1850/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1850/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The Atmosphere-Dependent Calculation of Air Fluorescence and its I
 mplementation in the Reconstruction of Air Showers
DTSTART:20100914T140000Z
DTEND:20100914T143000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1851@events.icecube.wisc.edu
DESCRIPTION:Speakers: Maria Monasor\n\nThe fluorescence yield -- the numbe
 r of photons produced per unit of deposited energy by nitrogen fluorescenc
 e as air shower particles move through air -- is a crucial ingredient in t
 he reconstruction of air shower parameters using the fluorescence techniqu
 e.  Several values of the absolute fluorescence yield\, as well as the par
 ameters which determine its dependence on atmospheric conditions (such as 
 humidity and temperature) will be discussed.  We also present a general al
 gorithm for the evaluation of the fluorescence yield\, and its implementat
 ion in the Pierre Auger Observatory offline reconstruction software.  This
  algorithm can be used to estimate the dependence of reconstructed shower 
 parameters on the yield.  We will illustrate the effect of atmospheric con
 ditions on the reconstruction of showers with several examples.\n\nhttps:/
 /events.icecube.wisc.edu/event/30/contributions/1851/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1851/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Atmospheric Simulation Outcomes of The CTA Design Study
DTSTART:20100914T155000Z
DTEND:20100914T162000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1852@events.icecube.wisc.edu
DESCRIPTION:Speakers: Sam Nolan\n\nThe Cherenkov Telescope Array (CTA) is 
 the next generation instrument in ground-based gamma-ray astronomy. It is 
 just coming to the end of a 3 year design study\, and in this talk we will
  discuss the detailed simulation studies performed to assess the need for 
 atmospheric monitoring and the methods by which correction for atmospheric
  variation may be achieved.\n\nhttps://events.icecube.wisc.edu/event/30/co
 ntributions/1852/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1852/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Atmospheric Monitoring for the H.E.S.S. Experiment
DTSTART:20100914T150000Z
DTEND:20100914T152000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1853@events.icecube.wisc.edu
DESCRIPTION:Speakers: Cameron Rulten\n\nA short talk on the atmospheric mo
 nitoring efforts undertaken at the H.E.S.S. site in Namibia and how the da
 ta is used in this ground-based gamma-ray astronomy experiment. Particular
  focus will be given toward single scattering lidars and the extinction of
  Cherenkov light due to low-level aerosol populations.\n\nhttps://events.i
 cecube.wisc.edu/event/30/contributions/1853/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1853/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The Rapid Atmospheric Monitoring Program for the Pierre Auger Obse
 rvatory
DTSTART:20100914T165000Z
DTEND:20100914T172000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1854@events.icecube.wisc.edu
DESCRIPTION:Speakers: Martin Will\n\nM. Will\, S. BenZvi\, B. Keilhauer\, 
 M. Prouza and A. Tonachini for the Pierre Auger Collaboration\n\nThe Pierr
 e Auger Observatory measures extensive air showers from interactions of co
 smic rays with Earth's atmosphere. More than 1600 Surface Detectors (SD) s
 ample the secondary shower particles that reach the ground while 27 Fluore
 scence Detectors (FD) constantly scan the night sky for faint fluorescence
  emissions from nitrogen molecules\, excited by the secondary particles. F
 or the reconstruction of air showers from FD data\, information about the 
 current atmospheric conditions is needed. For this purpose\, several monit
 oring systems have been implemented. Five ground-based weather stations an
 d atmospheric soundings provide ground values and altitude-dependent profi
 les of the molecular atmosphere\, four elastic lidars measure the attenuat
 ion of light due to aerosols and scan for clouds\, four cloud cameras at e
 ach of the FDs\, and one photometric robotic telescope (FRAM) also measure
 s the aerosol attenuation. Two aerosol phase function monitors\, a horizon
 tal attenuation monitor and a Raman lidar provide additional information a
 bout aerosol scattering. The atmospheric monitoring program has been upgra
 ded to allow for triggering the monitoring instruments shortly after the d
 etection of high-energy events and other showers of interest. During FD sh
 ifts\, incoming shower data are reconstructed by an automated online analy
 sis. Interesting showers then trigger dedicated measurements by the variou
 s subsystems if they meet certain individualized criteria to obtain detail
 ed information of the atmosphere\, for some subsystems even in the vicinit
 y of the shower track. The data are used to supplement the regular observa
 tions of the atmosphere. In the cases of sparse regular measurements or ra
 pidly changing atmospheric conditions the rapid monitoring data can signif
 icantly improve the accuracy of the reconstruction of showers. We will pre
 sent an overview of the implementation\, performance and first results of 
 the rapid monitoring system.\n\nhttps://events.icecube.wisc.edu/event/30/c
 ontributions/1854/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1854/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Development of a 1.8M Raman LIDAR for CTA
DTSTART:20100914T162000Z
DTEND:20100914T165000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1855@events.icecube.wisc.edu
DESCRIPTION:Speakers: Alicia Lopez Oramas\n\nThe use of a Raman LIDAR toge
 ther with Image Air Cherenkov Telescopes (IACT) would allow to improve the
  duty cycle and reduce systematical uncertainties of the latter. The Raman
  LIDARs allow the monitoring of the atmospheric transmission probability w
 ith a quite good accuracy but the altitude range needed by the IACT is cha
 llenging\, 20 km. A Raman LIDAR is being developed at IFAE for CTA by recl
 ycing an old telescope from the CLUE experiment. The large 1.8 diameter mi
 rror and the use of the most advanced technologies will hopefully allow fu
 lfilling the requirements.\n\nhttps://events.icecube.wisc.edu/event/30/con
 tributions/1855/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1855/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Analysis of Data from the Central Laser Facility
DTSTART:20100914T190000Z
DTEND:20100914T193000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1856@events.icecube.wisc.edu
DESCRIPTION:Speakers: Laura Valore\n\nhttps://events.icecube.wisc.edu/even
 t/30/contributions/1856/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1856/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Atmospheric Monitoring at the Auger North Site
DTSTART:20100914T172000Z
DTEND:20100914T174000Z
DTSTAMP:20260515T023300Z
UID:indico-contribution-1857@events.icecube.wisc.edu
DESCRIPTION:Speakers: David Starbuck\n\nhttps://events.icecube.wisc.edu/ev
 ent/30/contributions/1857/
LOCATION:Class of '24 - 4th Fl E (UNIVERSITY OF WISCONSIN MEMORIAL UNION)
URL:https://events.icecube.wisc.edu/event/30/contributions/1857/
END:VEVENT
END:VCALENDAR