Table of special observation campaigns
2019 Waves Campaign (Oct 17-19, 2019)
GOLD L1B data from this special campaign was analyzed and is discussed in the paper “First comparison of travelling atmospheric disturbances observed in the middle thermosphere by GOLD to travelling ionospheric disturbances seen in ground-based total electron content observations” by England et al. This data is available for download via the link below:
Waves_Campaign_October_2019_L1B_data.tar (6 GB)
2019 Eclipse (July 2, 2019) – Simulations
Simulation steps:
- TGCM runs with (UV attenuation: eclipse condition) and without (non-eclipse condition) an eclipse mask from 16:00 UT on July 2, 2019 to 16:00 UT on July 3, 2019
- Ionospheric and thermospheric parameters from TGCM runs are used as inputs to the GLOW model
- GLOW model estimates of airglow are then mapped onto eclipse’s FOV and LOS effects are taken into consideration
- Finally, percentage difference between eclipse and non-eclipse results are shown in the movies
| Thumbnail | Description | Release date | Format (Size) |
|---|---|---|---|
 |
Percentage difference in OI 135.6 nm emission (GLOW) | May 7, 2019 | MOV (532 KB) |
|
Percentage difference in OI 135.6 nm to LBH emission ratios (GLOW) |
May 7, 2019 | MOV (334 KB) |
 |
Percentage difference in the effective temperature by looking at LBH band structure (GLOW) |
May 7, 2019 | MOV (291 KB) |
 |
Difference in O to N2 ratio (not %) at pressure level -2.15 (not true O/N2 ratio) (TGCM) | May 7, 2019 | MOV (462 KB) |
 |
Difference in electron temperature (in K) at pressure level -2.15 | May 7, 2019 | MOV (564 KB) |
 |
Difference in ion temperature (in K) at pressure level -2.15 | May 7, 2019 | MOV (568 KB) |
 |
Difference in neutral temperature (in K) at pressure level -2.15 | May 7, 2019 | MOV (1 MB) |
All files: Courtesy Saurav Aryal/GOLD