  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: InSight tracking
 Exp. Code:  ed045b  


Schedule Version:       1.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       Dominic Dirxx

Address:  Delft
 
 
          The Netherlands

Phone:    +31 15 27 8886
EMAIL:    d.dirkx@tudelft.nl
Fax:
Phone during observation:

Observing mode: Mk5 at 8 GHz

Notes:    Spacecraft signal on X band
          Single pol RCP
 
 

Schedule for HART      (Code Hh )                                   Page   2
               InSight tracking
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sun  23 Feb 2020   Day  54 ---

 Next scan frequencies:  8400.49  8416.49  8432.49  8448.49
 Next BBC frequencies:    320.49   336.49   352.49   368.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00

02 30 00  J1924-2914   14 30 36  25.5 111.7 -4.9       0.0     0        0   02 30 00
02 33 00  =1921-293    14 33 36  26.2 111.5 -4.9       0.0   180        6   02 30 01

02 33 00  MARS0240     14 33 36  39.0 100.4 -3.8       0.0   -60        6   No stop 
02 35 00  ---          14 35 37  39.4 100.3 -3.7       0.0    60       10   02 33 01

02 35 00  J1820-2528   14 35 37  39.4 102.7 -3.8       0.0   -30       10   No stop 
02 38 00  =1817-254    14 38 37  40.0 102.5 -3.7       0.0   150       15   02 35 01

02 38 00  MARS0240     14 38 37  40.1 100.1 -3.7       0.0   -30       15   No stop 
02 40 00  ---          14 40 37  40.5  99.9 -3.7       0.0    90       19   02 38 01

02 40 00  J1820-2528   14 40 37  40.5 102.4 -3.7       0.0   -30       19   No stop 
02 43 00  =1817-254    14 43 38  41.1 102.2 -3.6       0.0   150       25   02 40 01

02 43 00  MARS0240     14 43 38  41.2  99.7 -3.6       0.0   -30       25   No stop 
02 45 00  ---          14 45 38  41.6  99.5 -3.6       0.0    90       29   02 43 01

02 45 00  J1820-2528   14 45 38  41.6 102.0 -3.6       0.0   -30       29   No stop 
02 48 00  =1817-254    14 48 39  42.2 101.8 -3.6       0.0   150       35   02 45 01

02 48 00  MARS0240     14 48 39  42.3  99.3 -3.5       0.0   -30       35   No stop 
02 50 00  ---          14 50 39  42.8  99.1 -3.5       0.0    90       39   02 48 01

02 51 00  MARS0300     14 51 39  43.0  99.1 -3.5       0.0    39       39   02 51 00
03 10 00  ---          15 10 42  47.2  97.6 -3.2       0.0  1140       75   02 51 01

03 11 00  MARS0320     15 11 43  47.4  97.5 -3.1       0.0    39       75   03 11 00
03 20 00  ---          15 20 44  49.4  96.8 -3.0       0.0   540       93   03 11 01

03 21 00  MARS0340     15 21 44  49.7  96.8 -3.0       0.0    39       93   03 21 00
03 40 00  ---          15 40 47  53.9  95.2 -2.7       0.0  1140      129   03 21 01

03 41 00  MARS0400     15 41 47  54.1  95.2 -2.6       0.0    39      129   03 41 00
04 00 00  ---          16 00 51  58.4  93.6 -2.3       0.0  1140      166   03 41 01


SETUP FILE INFORMATION:
   NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.


 ======== Setup file: sess120.X256
   Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq_RDBE.dat:
     hhsx            Values confirmed by E-mail Jonathan Quick 20140219 (CR)

   Setup group:    3         Station: HART              Total bit rate:   256
   Format: VDIF              Bits per sample: 2         Sample rate: 32.000
   Number of channels:  4    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   8080.00   8080.00   8080.00   8080.00
   Net SB=         U         U         U         U
   IF SB =         U         U         U         U
   Pol.  =      RCP       RCP       RCP       RCP 
   BBC   =         1         2         3         4
   BBC SB=         U         U         U         U
   IF    =        A1        A1        A1        A1

  The following frequency sets based on these setups were used.

   Frequency Set:   3  Setup file default.  Used with PCAL = off
   LO sum=   8400.49  8416.49  8432.49  8448.49
   BBC fr=    320.49   336.49   352.49   368.49
   Bandwd=     16.00    16.00    16.00    16.00
    Matching frequency sets:   3

   Track assignments are: 
    track1=   1,  2,  3,  4
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

   Source                         Source position (RA/Dec)                        Error
                        (B1950)             (J2000)             (Date)            (mas)

 * MARS0240          18 15 41.514224   * 18 18 44.520000     18 19 56.276787       0.00
                    -23 41 23.62156    *-23 40 08.40000     -23 39 34.76969        0.00
                     From catalog imbedded in main SCHED input file.

 * MARS0300          18 15 44.024744   * 18 18 47.030000     18 19 58.786326       0.00
                    -23 41 23.40400    *-23 40 08.00000     -23 39 34.29824        0.00
                     From catalog imbedded in main SCHED input file.

 * MARS0320          18 15 46.525225   * 18 18 49.530000     18 20 01.285882       0.00
                    -23 41 23.28572    *-23 40 07.70000     -23 39 33.92708        0.00
                     From catalog imbedded in main SCHED input file.

 * MARS0340          18 15 49.035747   * 18 18 52.040000     18 20 03.795421       0.00
                    -23 41 23.06817    *-23 40 07.30000     -23 39 33.45564        0.00
                     From catalog imbedded in main SCHED input file.

 * MARS0400          18 15 51.546270   * 18 18 54.550000     18 20 06.304959       0.00
                    -23 41 22.85061    *-23 40 06.90000     -23 39 32.98421        0.00
                     From catalog imbedded in main SCHED input file.

   1817-254          18 17 52.332230   * 18 20 57.848697     18 22 10.574531       0.05
 * J1820-2528       -25 29 37.39982    *-25 28 12.58410     -25 27 34.59171        0.09
   J1820-25          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    656 observations.

   1921-293          19 21 42.234126   * 19 24 51.055953     19 26 04.685816       0.00
 * J1924-2914       -29 20 26.35397    *-29 14 30.12107     -29 12 05.33636        0.01
   J1924-29          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  63480 observations.



SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE

     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.
  Source       Setup file             Frequency sets                  Observing hours
                                   (duplicates not shown)              Scan  Baseline
  MARS0240   sess120.X256          1 2 3 4 5 6                       0.133     2.197
  MARS0300   sess120.X256          1 2 3 4 5 6                       0.317     6.650
  MARS0320   sess120.X256          1 2 3 4 6                         0.150     2.250
  MARS0340   sess120.X256          1 2 3 4 6                         0.317     3.167
  MARS0400   sess120.X256          1 2 3 4 6                         0.317     3.167
  J1820-2528 sess120.X256          1 2 3 4 5 6                       0.150     2.807
  J1924-2914 sess120.X256          1 2 3 4 5                         0.050     0.500


EFFECT OF SOLAR CORONA

  The solar corona can cause unstable phases for sources too close to the Sun.
  SCHED provides warnings at individual scans for distances less than 10 degrees.
  The distance from the Sun to each source in this schedule is:
    Source         Sun distance (deg) 
   MARS0240            59.4
   MARS0300            59.4
   MARS0320            59.4
   MARS0340            59.4
   MARS0400            59.4
   J1820-2528          59.0
   J1924-2914          45.6

  Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes 
  that the Sun will cause amplitude reductions on the  longest VLBA baselines 
  at a solar distance of 60deg F^(-0.6) where F is in GHz. 
  For common VLBI bands, this is: 
       327 MHz        117. deg 
       610 MHz         81. deg 
       1.6 GHz         45. deg 
       2.3 GHz         36. deg 
       5.0 GHz         23. deg 
       8.4 GHz         17. deg 
      15.0 GHz         12. deg 
      22.0 GHz          9. deg 
      43.0 GHz          6. deg 

