Differences between revisions 1 and 47 (spanning 46 versions)
Revision 1 as of 2018-11-03 05:00:06
Size: 161
Comment:
Revision 47 as of 2020-08-28 05:20:39
Size: 4132
Comment:
Deletions are marked like this. Additions are marked like this.
Line 3: Line 3:
 . http://hitran.org keithl@keithl.com on kao3
 
 . https://www.sciencedirect.com/science/article/pii/0022407372900052
-------

=== H density versus altitude ===

||<|16> {{ attachment:geocoronaMarkup.png | | width=600 }} ||<)> '''alt km''' ||<)> '''radius km''' ||<)> '''#/m3''' ||
||<)> 1000 ||<)> 7378 ||<)> 21000e6 ||
||<)> 2000 ||<)> 8378 ||<)> 12000e6 || Constr. perigee ||
||<)> 5000 ||<)> 11378 ||<)> 3100e6 ||
||<)> 10000 ||<)> 16378 ||<)> 820e6 ||
||<)> 20000 ||<)> 26378 ||<)> 180e6 ||
||<)> 30000 ||<)> 36378 ||<)> 67e6 ||
||<)> 35786 ||<)> 42164 ||<)> 45e6 || GEO circular ||
||<)> 40000 ||<)> 46378 ||<)> 35e6 ||
||<)> 50000 ||<)> 56378 ||<)> 22e6 ||
||<)> 60000 ||<)> 66378 ||<)> 14e6 ||
||<)> 69572 ||<)> 75950 ||<)> 11e6 || Constr. apogee ||
||<)> 70000 ||<)> 76378 ||<)> 10e6 ||
||<-3> [[attachment:geocoronaMarkup.png | image source ]] ||

. https://www.sciencedirect.com/science/article/pii/0022407372900052


||<-12> Estimated hydrogen mass per 1000 km height, 1.67e-27kg/H ||
|| Altitude km || 1000 || 2000 || 10000 || 20000 || 30000 || 35786* || 40000 || 50000 || 60000 || 69572* || 70000 ||
|| Radius km || 7378 || 11378 || 16378 || 26378 || 36378 || 42164* || 46378 || 56378 || 66378 || 75950* || 76378 ||
|| Volume km³ || 6.8e11 || 1.6e12 || 3.4e12 || 8.7e12 || 1.7e13 || 2.2e13 || 2.7e13 || 4.0e13 || 5.5e13 || 7.2e13 || 7.3e13 ||
|| #H / m³ || 2.1e10 || 1.2e10 || 8.2e8 || 1.8e8 || 6.7e7 || 4.5e7 || 3.5e7 || 2.2e7 || 1.4e7 || 1.1e7 || 1.0e7 ||
|| H kg || 240000 || 32000 || 4700 || 2600 || 1900 || 1700* || 1000 || 1500 || 1300 || 1300* || 1200 ||

Less than 20 tonnes of hydrogen (and almost nothing else) above GEO, out to the bow shock.


=== 24 hour "Construction" Orbit ===
'''Note:''' 75950 km radius is the apogee of a "24 hour" geosynchronous (but NOT geostationary) orbit with a 8378 km radius (2000 km equatorial altitude) perigee. The same 42164 km semimajor axis as a circular geostationary orbit. This is a High Eccentricity Earth Orbit (HEEO), suggested by space scientist John Lewis at the University of Arizona. Given the high perigee velocity of a launch loop, this orbit is easier to achieve with much less apogee insertion ΔV than a GEO orbit. The perigee velocity of this HEEO orbit is high, and that is an excellent place for a high ΔV thrust into an interplanetary trajectory.

'''Subnote 1:''' due to the J₂ nonlinearity of the Earth's gravity field, this orbit will precess, so an exact synchronous orbit will have a slightly smaller semimajor axis.

'''Subnote 2:''' launchloop launches slows portions of the rotor; restoring rotor position and velocity requires enormous power. Larger vehicles would slow the rotor more, requiring more peak electrical power generation capacity. It is cheaper to assemble large interplanetary vehicles at a permanent orbiting construction station from dozens, perhaps hundreds of daily launches, then launch the propellant to fuel them after they are assembled. Since a launch to an interplanetary Hohmann must occur at a specific time of day for a particular mission, the perigee of the construction orbit must occur at that specific time. This is an annoying constraint for infrequent Mars missions, but less so for missions to many different asteroids.

=== Collision cross section table ===

|| Gas || (nm)² || (nm)² with H₂ ||
|| H₂ || 0.27 || 1.02 ||
|| He || 0.21 || 0.99 ||
|| Ar || 0.36 || 1.06 ||
|| O₂ || 0.40 || 1.07 ||
|| N₂ || 0.43 || 1.08 ||
|| CH₄ || 0.46 || 1.09 ||
|| CO₂ || 0.52 || 1.11 ||
|| Cl₂ || 0.93 || 1.22 ||

The second column is the combined collision cross section with an H₂ molecule ... the square of the sum of the square roots.

from [[ https://chem.libretexts.org/Bookshelves/Physical_and_Theoretical_Chemistry_Textbook_Maps/Supplemental_Modules_(Physical_and_Theoretical_Chemistry)/Kinetics/Modeling_Reaction_Kinetics/Collision_Theory/Collisional_Cross_Section | libretexts ]]

-----

 . http://hitran.org . . . . . . . . . k*l at k*l dot com on kao3

Propellant Plume Gas Scattering


H density versus altitude

geocoronaMarkup.png

alt km

radius km

#/m3

1000

7378

21000e6

2000

8378

12000e6

Constr. perigee

5000

11378

3100e6

10000

16378

820e6

20000

26378

180e6

30000

36378

67e6

35786

42164

45e6

GEO circular

40000

46378

35e6

50000

56378

22e6

60000

66378

14e6

69572

75950

11e6

Constr. apogee

70000

76378

10e6

image source

. https://www.sciencedirect.com/science/article/pii/0022407372900052

Estimated hydrogen mass per 1000 km height, 1.67e-27kg/H

Altitude km

1000

2000

10000

20000

30000

35786*

40000

50000

60000

69572*

70000

Radius km

7378

11378

16378

26378

36378

42164*

46378

56378

66378

75950*

76378

Volume km³

6.8e11

1.6e12

3.4e12

8.7e12

1.7e13

2.2e13

2.7e13

4.0e13

5.5e13

7.2e13

7.3e13

#H / m³

2.1e10

1.2e10

8.2e8

1.8e8

6.7e7

4.5e7

3.5e7

2.2e7

1.4e7

1.1e7

1.0e7

H kg

240000

32000

4700

2600

1900

1700*

1000

1500

1300

1300*

1200

Less than 20 tonnes of hydrogen (and almost nothing else) above GEO, out to the bow shock.

24 hour "Construction" Orbit

Note: 75950 km radius is the apogee of a "24 hour" geosynchronous (but NOT geostationary) orbit with a 8378 km radius (2000 km equatorial altitude) perigee. The same 42164 km semimajor axis as a circular geostationary orbit. This is a High Eccentricity Earth Orbit (HEEO), suggested by space scientist John Lewis at the University of Arizona. Given the high perigee velocity of a launch loop, this orbit is easier to achieve with much less apogee insertion ΔV than a GEO orbit. The perigee velocity of this HEEO orbit is high, and that is an excellent place for a high ΔV thrust into an interplanetary trajectory.

Subnote 1: due to the J₂ nonlinearity of the Earth's gravity field, this orbit will precess, so an exact synchronous orbit will have a slightly smaller semimajor axis.

Subnote 2: launchloop launches slows portions of the rotor; restoring rotor position and velocity requires enormous power. Larger vehicles would slow the rotor more, requiring more peak electrical power generation capacity. It is cheaper to assemble large interplanetary vehicles at a permanent orbiting construction station from dozens, perhaps hundreds of daily launches, then launch the propellant to fuel them after they are assembled. Since a launch to an interplanetary Hohmann must occur at a specific time of day for a particular mission, the perigee of the construction orbit must occur at that specific time. This is an annoying constraint for infrequent Mars missions, but less so for missions to many different asteroids.

Collision cross section table

Gas

(nm)²

(nm)² with H₂

H₂

0.27

1.02

He

0.21

0.99

Ar

0.36

1.06

O₂

0.40

1.07

N₂

0.43

1.08

CH₄

0.46

1.09

CO₂

0.52

1.11

Cl₂

0.93

1.22

The second column is the combined collision cross section with an H₂ molecule ... the square of the sum of the square roots.

from libretexts


GasScatter (last edited 2020-08-28 17:21:33 by KeithLofstrom)