CEDAR Support of the TIMED Initiative
Under an agreement with APL, the CEDAR Database (DB) at HAO/NCAR is
responsible as one of the sites for data from the Ground-Based
Investigators (GBI) of the TIMED program who have instrumental
or model data. The data from the
Ground sites
can be obtained through the Data Services/ Get/Plot Data menu to the left.
-
TIMED web page
-
TIMED/GUVI (Global Ultraviolet Imager) data web page (?)
-
TIMED/SABER (Sounding of the Atmosphere using Broadband Emission Radiometry) data web page
-
TIMED/SEE (Solar Extreme Ultraviolet Experiment) data web page (?)
-
TIMED/TIDI (TIMED Doppler Interferometer) data web page (?)
-
SuperDARN (Super Dual Auroral Radar Network) data web page
- CEDAR (Coupling, Energetics and Dynamics of Atmospheric Regions) data web page
-
MLTR (Mesosphere and Lower Thermosphere Radar) data web page
-
LT-ISR (Lower Thermosphere - Incoherent Scatter Radar) data web page (?)
Some GBI instruments show plots of their data, and in some cases links to get
the data. Often, these are automated sites so the data include all data,
including optical night-time data during cloudy periods or whatever. In some
cases, only the good data are passed onto the CEDAR DB.
- Socorro, NM Keogram imager slices in
the E-W and N-S. Click to 'Socorro' location and to 'All Sky Imager' istrument.
-
Poker Flat, AK 4 channel photometer data and estimated auroral and [O] parameters.
-
Fort Yukon, AK 4 channel photometer data and estimated auroral and [O] parameters.
-
Inuvik, Canada vertical [O] 557.7 nm (~97 km) Fabry-Perot winds and temperatures
There are 4 instruments on the TIMED satellite:
GUVI, SABER, SEE, and TIDI. SEE is the only instrument which
does not measure the same thing as GBIs. Of the other three,
this is an estimate about possible calibrations, validations or collaborations.
- GUVI - Ne from ISRs, auroral [O] variations from 4 Channel Photometers,
Tn > 100 km from red line FPSs (Poker Flat), auroral species ratios
from CCDSs.
- SABER -
SABER Observations (pdf file) and
SABER Validation Products (pdf file).
- Ti (or Tn) from ISRs day and night >~90km
- Tn at night from near OH peak ~87 km from MIs, CCDSs, FPSs (using OH filter)
-- all every several min, and narrowband temperature lidars using OH filter over the night
- Tn at night from near O2 peak ~93 km from MIs, FPSs and narrowband temperature lidars (using O2 filters)
- Tn at night from near OI 557.7 nm peak ~97 km from FPSs (using OI 557.7 nm filter)
- Tn profile at night (mostly) from sodium lidars from ~75-110 km, ~1 hr, ~1 km
- Tn profile at night (mostly) from ozone lidars from ~15-50 km (see also
http://www.ndsc.ws)
- Tn profile at night (mostly) from Rayleigh lidars from ~45-85 km, ~1 hr, ~0.1 km
- neutral density profile at night from Rayleigh lidars from ~45-95 km, ~1 hr, ~0.1 km,
with fixed density (like MSIS) at some altitude (like 50 km)
- [O3] from ~15-50 km from ozone lidars (see also
http://www.ndsc.ws)
- [O] ~100-150 km compared to MSIS profile from 4-channel photometers
at night during aurora
- [NO] from ~90-130 km from ground microwave at Kitt Peak
- [H2O], [O3], [O2] from ~50-70 km from ground microwave at Kitt Peak
- TIDI - winds between 70-100 km from MLT radars, lidars, ISRs, and FPSs;
Tn from lidars, ISRs, FPIs, MIs, CCDSs, and narrowband temperature imagers;
gravity waves from imagers; some intercomparison of radiances with ground
stations.
- Revised 08 Feb 2008 by emery@ucar.edu