Differences between revisions 12 and 18 (spanning 6 versions)

pole

Category B

Version 3.0

Description

This program solves for the pole right ascension, declination and rotation rate for a body in principal axis rotation. The rotation rate is calculated in degrees/day while right ascension and declination are calculated in degrees.

Input Files

POLE.TXT - simple text file containing nominal pole RA (deg), DEC (deg), PM (deg), OMEGA (deg/day)
LMRKLIST.TXT - list of landmarks

$/!\$ POLE.TXT and LMRKLIST.TXT must be in the working directory.

POLE.TXT is a single row file that contains the predicted pole RA (deg), DEC (deg), PM (deg), and OMEGA (deg/day). These values are given in the .tpc kernel file for the object. LMRKLIST.TXT contains a list of landmarks.

Using pole

1. Input a time in UTC.

$/!\$ Make sure the time is within the span supported by the kernels.

2018 NOV 16 13:09:54.824

2. Create a POLE.TXT file.

Here is a sample POLE.TXT file:

       86         -65      89.00000000    2010.48945

3. Answer whether you want the rotation rate fixed (y for yes, n for no).

4. Enter

0 if you want to iterate
1 if you want to keep the result (this updates POLE.TXT)
2 if you want the previous result (this is nominal if on the first iteration)

Here is a sample output from the POLE.TXT input:

    86.60062   -65.00002    90.42707  2009.99979311
     0.05176     0.02171                 0.00000001

The first row gives all the new pole parameters for POLE.TXT. The second row shows the change.

================= Testing using the NTE3A data set showed that picking different Epoch times over the time span of the images used (in this case 22 days) resulted in no change of RA, DEC, or rotation rate, and the PM at J2000 only change by 0.07 deg.

(Compiled by KD)

CategoryPrograms

-  ⇤ ← Revision 12 as of 2016-01-28 15:10:53 → 
  Size: 1450
  Editor: DianeLambert
  Comment:
+   ← Revision 18 as of 2018-04-09 15:17:30 → ⇥
  Size: 1958
  Editor: JohnWeirich
  Comment:
-Deletions are marked like this.
+Additions are marked like this.
 Line 2:
-Compiled by KD
+||Category B||Version 3.0||
-Line 6:
+Line 7:
-The program POLE solves for the pole right ascension, declination, and rotation rate for a body in principal axis rotation. The rotation rate is calculated in degrees/day while right ascension and declination are in degrees.
+This program solves for the pole right ascension, declination and rotation rate for a body in principal axis rotation. The rotation rate is calculated in degrees/day while right ascension and declination are calculated in degrees.
-Line 8:
+Line 9:
-For pole to run, POLE.TXT and [[LMRKLIST.TXT]] are required in the working directory. [[LMRKLIST.TXT]] is just a file containing a list of landmarks and POLE.TXT is a single row file that contains the predicted pole RA (deg), DEC (deg), PM (deg), and OMEGA (deg/day). These values are given in the .tpc kernel file for the object.
+== Input Files ==
 * POLE.TXT - simple text file containing nominal pole RA (deg), DEC (deg), PM (deg), OMEGA (deg/day)
 * [[LMRKLIST.TXT]] - list of landmarks
-Line 10:
+Line 13:
-== POLE.TXT Example ==
+'''''' /!\ POLE.TXT and [[LMRKLIST.TXT]] must be in the working directory. 

POLE.TXT is a single row file that contains the predicted pole RA (deg), DEC (deg), PM (deg), and OMEGA (deg/day). These values are given in the .tpc kernel file for the object. [[LMRKLIST.TXT]] contains a list of landmarks. 

----------
== Using pole ==

=== 1. Input a time in UTC. ===
  /!\ Make sure the time is within the span supported by the kernels.
{{{
2018 NOV 16 13:09:54.824
}}}

=== 2. Create a POLE.TXT file. ===

Here is a sample POLE.TXT file:
-Line 15:
+Line 33:
-== Input-Files ==
 * POLE.TXT - simple text file containing nominal pole RA (deg), DEC (deg), PM (deg), OMEGA (deg/day)
 * [[LMRKLIST.TXT]] - list of landmarks
+=== 3. Answer whether you want the rotation rate fixed (y for yes, n for no). ===
-Line 19:
+Line 35:
-== Input stdin ==
 * A time in UTC (make sure it is within the span supported by the kernels)
+=== 4. Enter ===

  * '''0''' if you want to iterate
  * '''1''' if you want to keep the result (this updates POLE.TXT)
  * '''2''' if you want the previous result (this is nominal if on the first iteration)

Here is a sample output from the POLE.TXT input:
-Line 22:
+Line 43:
-NOV 16 13:09:54.824
}}}

 * Determine whether you want the rotation rate fixed ( y for yes, n for no)

 * 0 if you want to iterate, 1 if you want to keep result (updates POLE.TXT), 2 if you want previous result (nominal if on 1st iteration)

== Output ==
 * {{{
-Line 35:
+Line 47:
- * First row is all the new pole parameters for POLE.TXT while the second row is the change.
+The first row gives all the new pole parameters for POLE.TXT. The second row shows the change.

=================
Testing using the NTE3A data set showed that picking different Epoch times over the time span of the images used (in this case 22 days) resulted in no change of RA, DEC, or rotation rate, and the PM at J2000 only change by 0.07 deg.

-----------
''(Compiled by KD)''

CategoryPrograms