RE: Confusing satellites

Ted Molczan (molczan@neocom.ca)
Thu, 9 Nov 1995 14:17:55 -0500

Walter Nissen quoted the following from Russell Eberst:

> It is very easy to confuse satellites what with the multitude 
> of objects in orbit. I try to fit in observations of as many 
> satellites as possible, as consistent with being accurate. This 
> of course involves a compromise and often completing obs on one 
> satellite, with only a minute or so before the next is due. 
> So I get the predicted R.A. and Dec and check if the azimuth and 
> elevations are increasing or decreasing i.e. if it's going 
> left to right or right-to-left and if its going up or down. 
 
> Grabbing the binoculars, I point them where the predicts 
> indicate, and look for something going up (or down) and l>r or 
> r>l. If an object is seen that doesn't fit the expectation then 
> it is ignored, and I wait for one that does fit.

Russell describes a challenge faced by all intensive observers.
In the late 80's, I did some fairly intensive observing, that is
to say, I tried to obtain at least two accurate time/position
measurements per object, tracking objects as little as 5 minutes
apart in time. That kind of activity puts a real premium on
such skills as organization, map reading, "star hopping",
perception and memory. Even with well developed skills, it is
always a challenge to keep up with the parade of satellites.
Often I found my self fighting the clock, trying to adequately
document my last obs (sufficient for later detailed reduction
of position and time) while leaving sufficient time to acquire 
the next target. 

Russell's comments about checking whether or not the expected
object will be moving up or down or left to right describe exactly
the process I followed. The only problem, is that it takes precious
time, so I found a way to automate the process, as the following
sample ephemeris shows. In particular, I draw your attention to
the column labeled "FE":

 9/11/95  18:05 - 23:05 ST   J2000.0  EL > 15  40 Pleasant Blvd.
Radarsat       95059A   23710   Bull =  17     Ted Molczan
SGP4   Age =   2.1 d   Unc =    0 s ( 25%)     416-921-1564 (h/w)

  TIME      %I   Mv     AZ  EL    R.A.   DEC   FE   VANG  RANGE   ALT
--------    --  ----   ---  --   -----  -----  --   ----  -----  -----
17:58:17    42   6.6   178  15   21:01  -31.5   7   0.11   2016    787
17:59:24    41   6.2   182  23   20:45  -22.9   7   0.16   1603    788
18:00:11    40   5.8   187  31   20:30  -14.6   7   0.22   1337    788
18:00:45    39   5.5   193  39   20:16   -6.6   7   0.28   1165    788
18:01:12    38   5.3   200  45   20:02    1.3   7   0.34   1048    789
18:01:34    37   5.2   209  52   19:48    8.9   7   0.40    970    789
18:01:53    37   5.1   220  57   19:34   16.2   8   0.44    919    789
18:02:10    36   5.0   233  61   19:19   23.2   8   0.47    888    789
18:02:26    36   5.0   249  63   19:02   30.0   9   0.49    874    790
18:02:41    36   4.9   266  63   18:43   36.3   9   0.49    873    790
18:02:56    37   5.0   281  61   18:22   42.3  10   0.48    886    790
18:03:12    37   5.0   294  57   17:55   48.1  10   0.45    913    790
18:03:29    38   5.1   305  53   17:21   53.3  10   0.42    956    790
18:03:47    39   5.2   313  48   16:41   57.6  11   0.37   1015    791
18:04:07    40   5.3   319  42   15:53   60.7  11   0.33   1094    791
18:04:30    40   5.5   324  37   14:57   62.5  11   0.28   1200    791
18:04:57    41   5.7   328  31   13:59   62.7  11   0.23   1338    791
18:05:30    42   6.0   332  25   13:03   61.3  11   0.18   1523    792
18:06:11    43   6.3   335  19   12:16   58.6  11   0.14   1767    792
18:07:03    44   6.6   338  13   11:37   54.8  11   0.11   2093    793

To understand FE, picture the field of view you see through your
binoculars as the face of a clock. The FE is the closest hour of the
clock face at which the object will enter your field of view, assuming
you are centred on the RA and DEC of the ephemeris point. So an FE of
6 means the object will move from bottom to top; an FE of 9, means it
will move from left to right. I simply note the FE beside each point
I plot in my star atlas when I prepare for an observing session. No muss, 
no fuss.

In addition to reducing the risk of tracking the wrong object, the FE
is helpful when looking for very faint objects, because it helps one to 
focus his/her gaze at the points where the object is most likely to
pass.

Computing the FE is not particularly difficult, as long as you are 
good at vector algebra. I have long ago forgotten most of the vector 
algebra I learned in school, but I have been able to count on some of my 
younger friends to help me out. If anyone wants the formulas in the 
form of BASIC statements, compatible with SGP/SGP4, I will be pleased 
to dig them up and post them.

bye for now