A Satellite in Sun-Synchronous Orbit

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SUMMARY

The discussion focuses on the calculations related to a remote sensing satellite in a sun-synchronous orbit with an inclination of 96.85 degrees. The calculated orbit altitude is 349 km, with a spacecraft coefficient of 200 kg/m² and solar flux F10.7 at 90. Key calculations include a maximum distance to the horizon of 2139 km, a swath width of 12094 km, and a ground speed of 7.3 km/s. The participants seek assistance with atmospheric density for lifetime estimation and communication time based on elevation angles.

PREREQUISITES
  • Understanding of orbital mechanics and satellite dynamics
  • Familiarity with atmospheric models and density calculations
  • Knowledge of trigonometric functions and their applications in satellite visibility
  • Proficiency in using the law of sines for geometric calculations
NEXT STEPS
  • Research atmospheric density models relevant to satellite operations
  • Learn about the law of sines and its applications in satellite communication calculations
  • Explore the impact of solar flux variations on satellite lifetime
  • Study the conversion between degrees and radians in trigonometric calculations
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Aerospace engineers, satellite communication specialists, and students studying orbital mechanics will benefit from this discussion.

ColdFusion85
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Homework Statement


A remote sensing satellite is deployed in a circular sun-synchronous orbit with inclination 96.85 degrees.

A. Calculate orbit altitude. I did this and got 349km.
B. The spacecraft coefficient is 200 kg/m^2. Solar conditions during the spacecraft launch are characterized by the solar flux F10.7 = 90. Is the orbit altitude sufficiently high for the spacecraft to operate through the estimated 2-year life time? What would be the spacecraft approximate lifetime if it is launched during solar maximum?
C. What is the maximum distance from the spacecraft to the horizon? I got 2139 km.
D. What is the maximum possible swath width? I got 12094 km.
E. What is the maximum possible time in view? I got 1560 seconds.
F. What is the ground speed of the subsatellite point? I got 7.3 km/s
G. The ground communications station is located at the satellite ground track. What is the communication time if the local conditions limit spacecraft visibility to elevation angles larger than 18 degrees?



The Attempt at a Solution



Assuming I got A,C,D,E,and F correct, I need help with B and G. For part B, I know the solar flux is related to the atmospheric density. If i get the atmospheric density I can use that, the radius of orbit and the ballistic coefficient to calculate the change in radius per revolution, and can calculate # of revs in a given time period since I know orbital velocity. I just don't know how to find the atmospheric density, rho, in the equation below which relates what I just talked about..

delta R(per rev) = -2*pi*(1/ballistic coeff)*rho*R^2

For part G, I have no clue where to start or what to do.
 
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This picture might help. The elevation angle is epsilon. lambda_0 is the swath angle. rho is not the same as the rho in part B.

http://server6.pictiger.com/img/680776/computer-games-and-screenshots/geometry.jpg
 
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Check your answers for D and E. Do these make sense given your answer for C?

For B, you must have been told to use some atmospheric model. This site, http://modelweb.gsfc.nasa.gov/atmos/atmos_index.html , is a good reference point for a number of atmospheric models.

For G, use the law of sines: sin(A)/a = sin(B)/b = sin(C)/c.
 
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Damn, I don't know what I am doing wrong here. We are given

cos(\lambda_0) = \frac{R_e}{R_e + h} = sin(\rho)

I got sin(\rho) = .9481 using R_e = 6378 km and h = 349 km calculated previously.

So \rho = 71.46 degrees, and D = R_e cos(\rho) = 2139 km

For part D, swath width, S_w = 2 \lambda_0 R_e, and since sin(\rho) = cos(\lambda_0), and since I got sin(\rho) to be .9481, \lambda_0 = arccos(.9481) = 18.54. Now our professor said this was in radians, so does that mean \rho is in radians too? If so, is part C incorrect? However, S_w = 2 \lambda_0 R_e = 2(.9841)(6378 km) = 12094 km. If I used degrees for lambda_0 this number would be absurdly huge. So how would this calculated answer not make sense in light of what I calculated for part C?

And what is wrong with part E? If part D is correct, isn't the time in view just the swath width divided by the speed of the satellite?

Any help with this would be greatly appreciated.
 
The swath width equation S_w = 2 \lambda_0 R_e is valid only if \lambda_0 is in radians. Your result, 18.54, is in degrees. Convert to radians.

Look at your own picture. The length of the circular arc from the subsatellite point to the horizon is half the swath width. How could that distance be three times the distance from the satellite to the horizon? BTW, your picture is a bit exaggerated. The satellite's altitude is 349 km, which is about 1/18 Earth radii.
 

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