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Differences between revisions 16 and 46 (spanning 30 versions)
Revision 16 as of 2020-07-31 17:51:28
Size: 2368
Comment:
Revision 46 as of 2020-08-01 01:14:35
Size: 3754
Comment:
Deletions are marked like this. Additions are marked like this.
Line 20: Line 20:
|| $ d $ || vehicle distance along track || || $ d_e $ || vehicle exit distance || || $ x $ || vehicle distance along track || || $ x_e $ || vehicle exit distance ||
Line 31: Line 31:
 * Assume classical drag heating $ H = \rho v^3 $ proportional to density and velocity cubed.  * Assume classical drag heating $ H = { 1 \over 2 } \rho v^3 $ proportional to density and velocity cubed.
Line 35: Line 35:
$ v ~~=~ a ~ t $ $ v ~~=~ a ~ t  ~~~~~~~~~~~~~~~ t_e ~=~ v_e / a $
Line 37: Line 37:
$ v^2 ~=~ 2 ~ a ~ d $ $ v^2 ~=~ 2 ~ a ~ x ~~~~~~~~~~~~ {v_e}^2 ~=~ 2 ~ a ~ x_e $
Line 39: Line 39:
$ H ~~=~ H_e ~ t / t_e $ Chosen heating rate over the launch run, ramping up proportional to time and velocity:
Line 41: Line 41:
$ H ~~=~ \rho(z) ~ v^3 ~=~ \rho(z) ~ ( 2 a d ) ~ ( a t ) $ $ H ~~=~ H_e ~ t / t_e ~=~ H_e ~ v / v_e $

thus

$ H ~~=~ { 1 \over 2 } \rho(z) ~ v^3 ~=~ { 1 \over 2 } \rho(z) ~ ( 2 ~ a ~ x) ~ ( a ~ t ) ~=~ \rho(z) ~ a^2 ~ x ~ t $
 
$ H = { 1 \over 2 } \rho_e ~ {v_e}^3 ~ t / t_e ~=~ \rho(z) ~ a^2 ~ x ~ t $

$ H_e ~=~ { 1 \over 2 } \rho_e ~ {v_e}^3 \rho(z) ~ a^2 ~ x_e ~ t_e $

FIXME ABOVE, TO GET TO THE BELOW EQUATION:

rearranging:

$ \rho(z) = \rho(z_e) {v_e}^2 / 2 a x $

So, given the exit velocity $ v_e $, the exit density $ \rho(z_e) $, and the distance $ x $ along the track from the starting point, we can compute the (higher) density at distance $ x $, and use that to determine the lower altitude at that point.

This blows up as $ x $ approaches zero, to infinite density. At some point (relatively close to the start) the track angle $ dz / dx $ starts increasing rapidly, where it makes sense to limit the track angle and run at a linear path down to west station, at a lower altitude.

Over a small range of $z$ around $z_0$, the function $ \rho(z) $ will approximate an exponential function:

$ \rho(z) \approx \rho_0 e^{-(z-z_0)/l_0} ~~~~~ $ where $ \rho_0 = \rho(z_0) $ and $ l_0 = { { \Large \rho(z_0) } \over { { { \LARGE \partial\rho(z) } \over { \LARGE z } } } { \large ~at~ z~=~ z_0 } } $, a log-linear fit.

Track Slope

Assume a maximum exit velocity a little larger than Earth escape (11.2 km/s) at 6458 km radius, 80 km altitude, near the equator. At that radius, the Earth's rotation velocity is 0.47 km/s ( 2π × 6458 km / 86414s ), so the maximum atmosphere-relative velocity (ignoring wind and adding drag loss) is 10.8 km/s. We will compute track slope backwards from that.

Loop inclination - the angle to the equator - will probably be between 10 and 30 degrees, To Be Determined.

Atmosphere Density Model

Altitude

Density

Scale Height

Average

km

kg/m3

km

km to 80

80 km

1.85e-5

6.33

6.33

70 km

8.28e-5

7.14

6.7

60 km

3.10e-4

8.02

7.1

50 km

1.03e-3

8.14

7.5

Linear Heating Profile

a

vehicle acceleration

x

vehicle distance along track

x_e

vehicle exit distance

v

vehicle velocity along track

v_e

vehicle exit velocity

H

vehicle heating (relative)

H_e

vehicle exit heating

t

time from start of launch run

t_e

exit time

\rho

atmospheric density

\rho_e

exit atmospheric density

z

vehicle/track altitude

z_e

exit altitude

  • Assume constant 3 gee acceleration ( a = 29.4 m/s²) to earth-relative escape velocity at exit altitude z_e = 80 km ( v_x = 10.8 km/s ), and a heating rate proportional to time on the track.

  • Assume that the track altitude is lower near the beginning of the acceleration run, and is designed to increase with distance (and thus velocity) to produce that heating profile.
  • Assume classical drag heating H = { 1 \over 2 } \rho v^3 proportional to density and velocity cubed.

An escape velocity run to v_e = 10800 m/s will last t_x = 10800/29.4 = 367 seconds. Most launches will be to high earth orbits, a slightly shorter launch run.

v ~~=~ a ~ t ~~~~~~~~~~~~~~~ t_e ~=~ v_e / a

v^2 ~=~ 2 ~ a ~ x ~~~~~~~~~~~~ {v_e}^2 ~=~ 2 ~ a ~ x_e

Chosen heating rate over the launch run, ramping up proportional to time and velocity:

H ~~=~ H_e ~ t / t_e ~=~ H_e ~ v / v_e

thus

H ~~=~ { 1 \over 2 } \rho(z) ~ v^3 ~=~ { 1 \over 2 } \rho(z) ~ ( 2 ~ a ~ x) ~ ( a ~ t ) ~=~ \rho(z) ~ a^2 ~ x ~ t

H = { 1 \over 2 } \rho_e ~ {v_e}^3 ~ t / t_e ~=~ \rho(z) ~ a^2 ~ x ~ t

H_e ~=~ { 1 \over 2 } \rho_e ~ {v_e}^3 \rho(z) ~ a^2 ~ x_e ~ t_e

FIXME ABOVE, TO GET TO THE BELOW EQUATION:

rearranging:

\rho(z) = \rho(z_e) {v_e}^2 / 2 a x

So, given the exit velocity v_e , the exit density \rho(z_e) , and the distance x along the track from the starting point, we can compute the (higher) density at distance x , and use that to determine the lower altitude at that point.

This blows up as x approaches zero, to infinite density. At some point (relatively close to the start) the track angle dz / dx starts increasing rapidly, where it makes sense to limit the track angle and run at a linear path down to west station, at a lower altitude.

Over a small range of z around z_0, the function \rho(z) will approximate an exponential function:

\rho(z) \approx \rho_0 e^{-(z-z_0)/l_0} ~~~~~ where \rho_0 = \rho(z_0) and l_0 = { { \Large \rho(z_0) } \over { { { \LARGE \partial\rho(z) } \over { \LARGE z } } } { \large ~at~ z~=~ z_0 } } , a log-linear fit.

TrackSlope (last edited 2020-08-30 23:40:35 by KeithLofstrom)