Satellite Laser Ranging in 5x5 Spherical Harmonics
<p>This is a variant of the weekly, 5x5 SLR product created at the University of Texas’s Center for Space Research (CSR) which is released alongside the GRACE series:</p> <p>ftp://podaac.jpl.nasa.gov/allData/tellus/preview/L2/deg_5/CSR.Weekly.5x5.Gravity_Harmonics.txt. </p> <p>The version here is averaged monthly, rather than weekly, to make it more directly comparable to the monthly GRACE data. It contains an estimate of C<sub>61</sub>/S<sub>61</sub> (but no other degree-6 harmonics) to avoid skewing the C<sub>21</sub> harmonic due to a lack of sufficient degrees of freedom during the creation of the SLR gravity product (Cheng and Ries, 2017). From January - November 1993, only four satellites were used in its creation (Starlette, Ajisai, and Lageos 1 and 2). After that point, Stella was added as well. Data exists through mid-2017.<br> <br> The layout of the files contains a header section followed by one line containing the date for the following lines, and then 22 lines of spherical harmonic data. The time lines are formatted as: IARC, MAXDEG, NP, IYEAR, IM, XMJD:<br> IARC: the arc number (ie: month number) <br> MAXDEG: spherical harmonic maximum degree/order of the field <br> NP: number of coefficient pairs (Cnm & Snm)<br> IYEAR: year<br> IM: month<br> XMJD: epoch of the arc at the first day in modified Julian date</p> <p>The data lines are formatted as: N, M, Cnm, Snm, Cnm-sigma, Snm-sigma:<br> N: spherical harmonic degree <br> M: spherical harmonic order<br> Cnm: C coefficient <br> Snm: S coefficient<br> Cnm-sig: The formal errors of the C coefficient<br> Snm-sig: The formal errors of the S coefficient<br> </p>
ShareScore
40/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 8
- Harmonization
- 4
- Access
- 20
- Reuse readiness
- 8
- Engagement
- 0