Mosaic code update: mapping the kronian magnetosphere

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Presentation transcript:

Mosaic code update: mapping the kronian magnetosphere Henrik Melin Planetary and Space Science Division Space Environment Technologies UVIS Team meeting 09/01/2007

Old and new IDL code a comparison 3367 lines of code Fortran style interface Every instance of a geometric setup a special case 342 lines of code IDL style interface Cache implementation Generalized approach to dealing with geometry by using polygons

Input parameters Length of the side of the square grid Number of grid elements Target, e.g. ‘SATURN’ Flat-field array Files to process Properties of the NCDF files: time, integration time, compression etc from file header.

Output parameters A data cube x, y is spatial coordinates and z is the spectral dimension

INITIAL RESULTS

Cassini pre-SOI system scans 1 2 3 4

Reflected sunlight dataset 1

Reflected sunlight dataset 2

Reflected sunlight dataset 3

Reflected sunlight dataset 4

Lyman Alpha dataset 1

Lyman Alpha dataset 2

Lyman Alpha dataset 3

Lyman Alpha dataset 4

Oxygen (1304Å) dataset 1

Oxygen (1304Å) dataset 2

Oxygen (1304Å) dataset 3

Oxygen (1304Å) dataset 4

Remaining issues  Intensity calibration - flatfielding How do I deal with evil pixels? What is the smallest usable time resolution? What is the optimal grid resolution?