NOW 2004 Program:
How does the neutrino "Planisphaerium" appear NOW?

Working Group 1

   =====================================================================

Terra Cognita I: Charting the (\nu_1,\nu_2) land

   Possible topics:
   · SuperKamiokande (solar)
   · SNO
   · Gallium experiments (GNO & SAGE)
   · KamLand, geoneutrinos
   · Low energy experiments (Borexino, KamLand, LowNu etc.)
   · Cross sections of solar interest
   · Solar model(s)
   · Data analysis

=====================================================================

   Possible topics:· SuperKamiokande (atmospheric)
   · K2K
   · Cross sections of atmospheric n interest
   · Cosmic rays of atmospheric n interest
   · Atmospheric fluxes
   · Direct calibration experiments
   · LBL’s and Super Beams (1st phase)
   · Data analysis

=====================================================================

Terra Incognita I: Moving into the (\nu_1,\nu_3) land and beyond

   Possible topics:· Reactor experiments
   · n factories
   · Super Beams (2nd phase) 
   · LSND & MiniBOONE
   · nu electromagnetic properties
   · Sterile neutrinos and nonstandard interactions
   · (Far) beyond standard model (strings, extra dimensions etc.)

Working Group 4

=====================================================================

Terra Incognita II: Exploring and modeling absolute masses

   Possible topics:
   · Neutrino mass models
   · Quantum corrections to neutrino masses
   · b decay
   · 0n2b decay
   · Future direct mass measurement
   · Neutrinos mass from CMB anisotropies
   · Neutrino decay

Working Group 5

=====================================================================

Atlas coelestis: Neutrinos from Heavens

   Possible topics:
   · Supernovae and neutrinos
   · HE neutrino sources
   · Km3 detectors (Antares, NEMO, Amanda & ICE3)
   · Atmospheric Detectors (Auger, EUSO, etc.)
   · Megaton detectors
   · Neutrinos and BBN