STEREO-related JOPS and CIPS

• Joint Observing Programs (combined with SOHO)
  • JOP Guidelines
  • JOP 186: Atmospheric Seismology
  • JOP 187: Stereoscopic Observations of Coronal Structures
  • JOP 188: Prominence Mass Composition and Variability Study
  • JOP 190: Temperature, density and 3-D structure of active region loops
  • JOP 191: 3-D structure and evolution of filaments/prominences
  • JOP 192: Chromospheric heating - signatures of waves and reconnection
  • JOP 193: Coronal holes boundaries evolution
  • JOP 194: Filament/Cavity-CME-ICME IHY-CIP campaign
  • JOP 196: Detection of waves in the solar atmosphere
  • JOP 197: Multi-wavelength observations of coronal hole plumes at solar minumum
  • JOP 199: The magnetic structure of macrospicules
  • JOP 200: Multi-point, high cadence EUV (and complementary) observations of the dynamic solar corona
  • JOP 201: Linking the Corona to the solar wind at Ulysses -- WHI
  • JOP 202: Origin of the slow solar wind -- WHI
  • JOP 203: Coronal hole boundary and Low-latitude Coronal Holes -- WHI
  • JOP 204: Characterizing the Energetics and Dynamics of the Quiet Sun -- WHI
  • JOP 205: Active Regions -- WHI
  • JOP 206: Low-latitude Coronal Holes -- WHI
  • JOP 214: Quiescent prominence structure and dynamics with Hinode and La Palma
  • JOP 216: Multi-wavelength Observations of Oscillations in Polar Plumes
  • JOP 217: Velocity fields at the base of polar coronal holes
  • JOP 219: Connection between photospheric vortex flows and transition region and coronal heating
  • JOP 222: Detecting the Origin of Shock-Accelerated Solar Energetic Particles
  • JOP 224: Solar Tomography with Minimal Solar Rotation
  • ICAL 01: Intercalibration 1 (EUV)
  • ICAL 14: HERSCHEL Sounding Rocket Intercomparisons
• International Heliophysical Year Coordinated Investigation Programs
  • CIP 7: 3-D Structure of EUV CMEs in the inner corona
  • CIP 21:Investigating Coronal Filament Cavities
  • CIP 23: Formation and Evolution of Filaments
  • CIP 51: Filament activation and its relation to CMEs

Last Revised: Thursday, 11-Jun-2009 14:17:22 EDT
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