Key RO Advances Observation –Lower tropospheric penetration (open loop / demodulation) –Larger...
-
Upload
geraldine-moody -
Category
Documents
-
view
212 -
download
0
Transcript of Key RO Advances Observation –Lower tropospheric penetration (open loop / demodulation) –Larger...
Key RO Advances • Observation
– Lower tropospheric penetration (open loop / demodulation)– Larger number of profiles (rising & setting) – Detailed precision analysis (collocated soundings) – Reduced latency – Ionospheric biases - effect of solar cycle on temp. retrieval
• Atmospheric science – Global maps of ABL height (seasonal variation)– Stratospheric wave detection / Gravity wave– Detailed tropopause studies / double tropopause – Initial climate trend comparisons – Detection of Atmospheric tides– New ionospheric features (caves / bays …) – Pre - seismic ionospheric anomalies ????
Limitations of RO to date
• Too few soundings (limited by # of sats / # transmitters / antenna patterns / firmware / hardware)– Limits impact on weather forecasting– Limited impact at the mesoscale – Lack of resolving power for certain atmos.
features (i.e. in the ABL maps / Water vapor maps)
– Ionosphere coverage still sparse
Limitations of RO up to date (b)
• Limitations in data latency (currently ~80% < 3 hours)– Too slow for space weather (want 10 min) – Too slow for next gen. weather prediction
update cycles (want < 1 hour)
Limitations of RO up to date (c)
• Data quality limitations– Remaining unexplained biases in lower troposphere
• observation noise related
• atmospheric propagation effects
– Biases in stratosphere• ionospheric effects
• orbit / attitude / PCV / multipath limitations
– Height range for climate monitoring is presently limited (8 -25 km)
New Science with COSMIC II• Science at CDAAC
– Improved Quality - what can be done – Increased Quantity - how to maximize– Improved Inversion Algorithms (Weather / Climate /
Ionosphere) – New Products (Level III)
• Science from other groups using these data– Weather / Storm forecasting– Climate monitoring / Model evaluation – Ionospheric forecasting and monitoring– “New phenomena”
COSMIC II Improvements - Quantity
• More satellites (~12)• More transmitters (GPS + Galileo + GLONASS +
BeiDou?)• Better antenna FoV or beam steering• Firmware + Hardware (CPU + RAM) improvements• With 12 satellites we expect: 12*600*2 = 14,400
soundings / day• OSSEs need to be conducted if this is a good number
COSMIC II Improvements - Quality (rx & ant.)
• Better antenna - Beam steering for better gain (LT bias reduction)
• Multiple correlators - maximized signal strength for lower troposphere tracking (LT bias reduction)
• USO - allows zero-differencing (noise reduction in stratosphere)
• Additional Frequencies (L5 + new Galileo bands) potential for improved iono. correction / orbit improvement
COSMIC II Improvements - Quality (s/c)
• Better attitude control & knowledge (reduce satellite velocity errors - better stratospheric data)
• Antenna PCV specification relative to s/c center of mass
• Need to avoid SNR drops observed during COSMIC - not fully understood yet - should monitor antenna temperatures
• Optimize the constellation - 800 km? 12 planes? 6 low-latitude orbit(s) ? Inclination 72 degrees ?
• Additional payloads ? Magnetometer, Langmuir probe, Laser reflector, ….
COSMIC II Improvements - Algorithms
• Weather– Reduce effect of noise and non-spherical irregularities on
retrieved profiles– Alternative initialization maybe develop bending angle
climatology – RH processing in tropopause region?
• Climate– Inverting zonal averaged bending angles– Optimize different initialization for weather and climate
processing
• Ionosphere– Horizontal gradients, localizing scintillation, tomography ..
COSMIC II Improvements - New Data Products (Level III)
• ABL (already done but different approaches + quantity will change the impact of this product)
• Characterization of moist tropospheric convection• Tropopause (Height, Temp, Structure ?) • Scintillation product (S4, lat , lon, height) ?• Dry Turbulence (not yet demonstrated)• Characterization of Gravity waves - in stratosphere and
ionosphere?• E-layer characterization
New Science that we will purse with the improved COSMIC II
observations
– Weather / Storm forecasting– Climate monitoring / Model evaluation – Ionospheric forecasting and monitoring– “New phenomena” – …….