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Version 1.9 Build 1556 |
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Package | utility | |
Module | aipsrcdata |
measures.default: gui measures.precession.d_interval: 0specifies that a measures GUI is started up automatically, and do full calculations on precession always.
measures.default | specify user interface medium | ||
Allowed: | gui or screen | ||
Default: | screen | ||
measures.iau2000.b_use | use the IAU2000 precession/nutation model | ||
Allowed: | true or false | ||
Default: | true | ||
measures.iau2000.b_use2000a | if the IAU2000 precession/nutation model is used, use the high precision nutation | ||
Allowed: | true or false | ||
Default: | false | ||
measures.precession.d_interval | interval in days over which linear interpolation of precession calculation is appropiate | ||
Allowed: | number of days | ||
Default: | 0.1 | ||
measures.nutation.d_interval | interval in days over which linear interpolation of nutation calculation is appropiate | ||
Allowed: | number of days | ||
Default: | 0.04 | ||
measures.nutation.b_useiers | use the IERS Earth orientation parameters tables to calculate nutation | ||
Allowed: | true or false | ||
Default: | false | ||
measures.nutation.b_usejpl | use the JPL DE database (use measures.jpl.ephemeris to specify which one) to calculate nutation | ||
Allowed: | true or false | ||
Default: | false | ||
measures.aberration.d_interval | interval in days over which linear interpolation of aberration calculation is appropiate | ||
Allowed: | number of days | ||
Default: | 0.04 | ||
measures.aberration.b_usejpl | use the JPL DE database (use measures.jpl.ephemeris to specify which one) to calculate aberration | ||
Allowed: | true or false | ||
Default: | false | ||
measures.solarpos.d_interval | interval in days over which linear interpolation of solar position calculation is appropiate | ||
Allowed: | number of days | ||
Default: | 0.04 | ||
measures.solarpos.b_usejpl | use the JPL DE database (use measures.jpl.ephemeris to specify which one) to calculate solar position | ||
Allowed: | true or false | ||
Default: | false |