1 / 6

Introduction to the Gap Analysis discussion CGMS-41, WG III July 2013

Introduction to the Gap Analysis discussion CGMS-41, WG III July 2013. Jérôme LAFEUILLE (WMO). WMO; OBS/SAT. CGMS baseline for operational/sustained missions. Advanced VIS/IR imagery ) 6 GEO locations IR Sounding (some hyperspectral) ) 6 GEO locations

denali
Download Presentation

Introduction to the Gap Analysis discussion CGMS-41, WG III July 2013

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Introduction to the Gap Analysis discussionCGMS-41, WG III July 2013 Jérôme LAFEUILLE (WMO) WMO; OBS/SAT

  2. CGMS baseline for operational/sustained missions • Advanced VIS/IR imagery ) 6 GEO locations • IR Sounding (some hyperspectral) ) 6 GEO locations • Lightning detection ) 6 GEO locations  • Space Environment Monitoring ) 6 GEO locations • ERB, UV sounding, Solar activitysome GEO locations • Multispectral VIS/IR imagery ) • IR hyper-spectral sounders ) a.m., p.m., e.m • MW sounders ) • MW imagers – some polarimetric ) • Scatterometers 2 orbital planes • Altimeter constellation am,pm +reference mission • Radio occultation (>10,000 occ./day) am, pm + constellation • Broadband Vis/IR radiometer a.m. , p.m • Narrow-band (oc colour, veg, aerolol) a.m. • High Res Vis/IR a.m. constellation • IT dual angle view imagery a.m. • Particle detection, Magnetic field a.m., p.m • Solar monitoring at least two

  3. LEO / early morning : anticipated gap after DMSP expected deployment of a FY-3 satellite LEO / p.m. orbit : risk of gap between SNPP and JPSS GEO: South America coverage after GOES-12 LEO/ERB: to be confirmed (FY3/ERM, JPSS/CERES) Atmospheric composition: limb sounding ? Radio-occultation: threats on COSMIC-2 funding (late 2015 & 2018) Other «gaps» raised by WMO Exec.Council (See WP14) GPM follow-on GEO hyperspectral sounding Space Weather Gaps with respect to the CGMS baseline

  4. Contribution of current COSMIC RO constellationbetween 1000-1800 occultations/day

  5. ~ 1,300 profiles/day 2018 6 satellites polar orbits 2016 6 satellites equatorial orbits ~ 12,000 profiles/day 5 Courtesy of UCAR

  6. To be discussed by WG III • Updating and assessing the list of main risks • Discuss actions/recommendations to mitigate the risk: • Advocacy for no-gap planning • Alternative mission planning • Improved access to or use of, existing/planned alternative sources • Communication to users • ….

More Related