IGS LEO JASON-1 orbit campaign 2003
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JASON-1 campaign |
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| Centre | ID | Solution description |
| asi | ext | Reduced dynamic solution, external attitude data, GPS |
| int | Reduced dynamic solution, internal attitude model, GPS | |
| cnes | poe | Standard POE for geodetic data record, DORIS+SLR |
| gps | Reduced dynamics solution, GPS | |
| csr_ | _ds | CSR dynamic solution, DORIS+SLR |
| gds | CSR dynamic solution, DORIS+SLR+GPS | |
| deos | grm | DEOS dynamic solution from CalVal campaign using GRIM5-c, DORIS+SLR |
| jgm | DEOS dynamic solution from CalVal campaign, using JGM3, DORIS+SLR | |
| esoc | ds2 | ESOC reduced dynamic solution, DORIS + SLR |
| grgs | _gs | Dynamic solution, undifferenced GPS + SLR |
| gsfc | dyn | GSFC dynamic solution, DORIS+SLR |
| red | GSFC reduced dynamics solution, DORIS+SLR | |
| rex | GSFC reduced dynamics solution, DORIS+SLR+Crossovers | |
| gps | GSFC reduced dynamics solution, GPS | |
| gs4 | GSFC reduced dynamics solution, GPS + SLR | |
| jpl | gps | JPL reduced dynamics solution, GPS |
| poe | Early JPL CalVal orbits | |
| ncl_ | _ds | DORIS / SLR dynamic solution |
Table 1: Solution identifiers used in the comparison results.
: standard fact
sheets per solution are under preparation,
and will provide more detailled
information on the POD methods.
The campaign period runs from day 154 of 2002 (June 3, 2002, MJD 52428, GPS week 1169 day 1) to day 182 of 2002 (July 1, 2002, MJD 52456, GPS week 1173 day 1), both inclusive. This corresponds to the cycles 15, 16 and 17 of JASON-1, with the exclusion of the very last day of cycle 17 which has minor data problems. For day 172 (June 21, 2002, MJD 52446) no attitude quaternions were available, and solutions that use quaternions show reduced precision for that day. Nonetheless, this day has not (yet) been excluded, due to other practical problems that arise from such exclusion.
Participating centers are requested to provide orbit solutions for this period, using satellite identifier L08 for JASON-1. Although SP3 format is preferred, contributions in SP1 format or POE formats can also be processed. Solutions either cover an entire JASON cycle with an overlap of about two orbital revolutions at either end (~ 4 hours), or should be provided in daily files with 2 hour overlap at either end (= 28 hour files starting at 22:00). Deviations from these requirements will probably not lead to significant errors, but an attempt is made to limit file conversions and interpolations as much as possible. Velocity values should be included in the SP3 files, but if these are missing they will be added by an numerical interpolation tool at ESOC. The preferred vector interval is 60 seconds or any smaller step that is in phase with 60 second intervals (i.e. 30, 20, 15, 10 seconds).
For any further questions or comments, please contact Henno.Boomkamp@esa.int .