Long Term Observations of Earth's Upper Atmosphere

No abstract availabl

Infrared Radiation in the Thermosphere During Solar Cycle 24

No abstract availabl

Comparison between the Temperature Measurements by TIMED/SABER and Lidar in the Mid-Latitude

Comparisons of monthly-mean nighttime temperature profiles observed by the Sodium Lidar at Colorado State University and TIMED/SABER over passes are made. In the altitude range from 85 km to about 100 km, the two observations are in excellent agreement. Though within each other s error bars, important differences occur below 85 km in the entire year and above 100 km in the summer season. Possible reasons for these difference are high photon noise below 85 km in lidar observations, and less than accurate assumptions in the concentration of important chemical species like oxygen (and its quenching rate) in the SABER retrieval above 100 km. However, the two techniques both show the two-level mesopause thermal structure, with the times of change from one level to the other in excellent agreement. Comparison indicates that the high-level (winter) mesopause altitudes are also in excellent agreement between the two observations, though some difference may exist in the low-level (summer) mesopause altitudes between ground-based and satellite-borne data

Observations of Space Weather and Space Climate Over the Past 15 Years From SABER (And Longer!)

The global infrared (IR) energy budget of the thermosphere has been reconstructed back 70 years (to 1947). IR cooling, integrated over a solar cycle, is relatively constant over the 5 complete cycles (19 -23) studied. Result implies that solar energy (particles and photons) has similar, small (< 7%) variation from one cycle to next. From Earth's upper atmosphere perspective, solar cycles are really more similar than different, over their length. No consistent relationship between peak of IR cooling and sunspot number peak. Results submitted to GRL 8/2016

Stray Light Analysis of the SABER Telescope

The stray light analysis of the sounding of the atmosphere using broadband emission radiometry (SABER) instrument on the thermosphere-ionosphere-mesosphere energetics and dynamics (TIMED) mission is discussed. Relevant mission objectives and operating conditions are stated to define the stray light problem. Since SABER is an earth limb viewing sensor, the telescope must be designed for large off-axis rejection. Described are the key design features which make the instrument well suited for its mission. Representative point source transmittance (PST) curves computed using the commercial stray light program APART are presented. Non-rejected radiance (NRR) values computed using APART generated PST curves and LINEPACK generated curves for the total radiance from the earth aixi the afinosphere are given. A method for computing NRR from the earth and the atmosphere using lineof- sight radiance profiles versus tangent height is described. Computed NRR values demonstrate that the effect of stray light on SABER\u27s measurement capability is negligible

The Spectroscopic Foundation of Radiative Forcing of Climate by Carbon Dioxide

No abstract availabl

Diurnal variations of temperature and winds inferred from TIMED and UARS measurements

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95001/1/jgra18181.pd

Stray Light Analysis of the SABER Telescope

The stray light analysis of the sounding of the atmosphere using broadband emission radiometry (SABER) instrument on the thermosphere-ionosphere-mesosphere energetics and dynamics (TIMED) mission is discussed. Relevant mission objectives and operating conditions are stated to define the stray light problem. Since SABER is an earth limb viewing sensor, the telescope must be designed for large off-axis rejection. Described are the key design features which make the instrument well suited for its mission. Representative point source transmittance (PST) curves computed using the commercial stray light program APART are presented. Non-rejected radiance (NRR) values computed using APART generated PST curves and LINEPACK generated curves for the total radiance from the earth aixi the afinosphere are given. A method for computing NRR from the earth and the atmosphere using lineof- sight radiance profiles versus tangent height is described. Computed NRR values demonstrate that the effect of stray light on SABER\u27s measurement capability is negligible