4 Final Report - Emits - ESA

4 Final Report - Emits - ESA 4 Final Report - Emits - ESA

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4 Final Report Table 4.5-5: EPS fuel and power consumption and system mass for attitude control over 10 years Deadzone size Fuel consumption [kg] Power consumption [kW] System mass [kg] microHEMPT DZ 1/3 0.7 0.2 61 DZ 1/6 3.9 0.2 64 HEMPT 3050 120 2.3 307 Thrusters active [-] Thrusters active [-] 2 1.5 1 0.5 Thruster activation timeline (DZ: 1/6) 0 1000 1500 2000 2500 3000 Time [s] 3500 4000 4500 5000 Thruster activation timeline (DZ: 1/3) 2 1.5 1 0.5 0 1000 1500 2000 2500 3000 Time [s] 3500 4000 4500 5000 Figure 4.5-9: Thruster activation timelines for dead zone sizes of 1/6 (top) and 1/3 (bottom) of maximum available torque The analysed performance values are • APE 61.1 μrad, AME 11.2 μrad, PDE 0.24 μrad/100ms (all values for 100% probability). A major issue with the EPS based attitude control system is that it is based upon currently nonexistent technology which is believed to be available on the European market within the next five to seven years. No major technological showstoppers are identified for the development of a microHEMPT system but should such a system prove itself to be infeasible for use on Geo-Oculus, other technologies such as microHET and FEEPT thrusters can be considered. 4.5.6.5 Manoeuvre performance One of the key issues for Geo-Oculus is the ability to image multiple locations throughout Europe several times per day. The limiting factor for manoeuvrability is the available torque to perform the manoeuvre in the shortest time possible, and the settling time needed after the manoeuvre to reach the required attitude performance again. Manoeuvrability is only required around the x- and y-axis, to Page 4-62 Doc. No: GOC-ASG-RP-002 Issue: 2 Astrium GmbH Date: 13.05.2009

4 Final Report scan North/South and East/West, respectively. A summary of the manoeuvres required over 24 h is presented in Table 4.5-6. Table 4.5-6: Manoeuvre summary Manoeuvre [deg] Daytime manoeuvres over 9 h [-] Nighttime manoeuvres over 15 h [-] Total manoeuvres over 24 h [-] Manoeuvre time allocation [s] 0.25 27 0 27 70 0.40 27 0 27 70 2.00 324 720 1044 70 All manoeuvre performance data presented in this section are based on one-axis manoeuvres. There are several options for manoeuvre actuators. The MBW option is clear, but also two EPS options, using either the HEMPT 3050 or microHEMPT, have been considered. The MBW option uses the same wheels for attitude control and manoeuvres, as the torque output from one wheel is scaleable from 0 to 400 mNm. The wheel drive electronic quantisation is 55 µNm. The EPS can not throttle its output to the same degree and an additional EPS system is needed for manoeuvres. The first option is to use the HEMPT 3050 thrusters for manoeuvres which can produce a torque of ±85 mNm around each axis. In the EPS analysis another option has been introduced as well. MicroHEMPT for attitude control has a few advantages such as lower fuel and power consumption and system mass, and one obvious drawback: the long resulting manoeuvre time. An overview of the theoretical, time optimal manoeuvre time for the various options are listed in Table 4.5-7. Note that these numbers do not allocate time for a settling period after the completion of the manoeuvre. Table 4.5-7: Theoretical, time optimal manoeuvre times for HEMPT 3050 and microHEMPT based configurations, and duty cycle over 24 h Manoeuvre [deg] HEMPT 3050 (30 mN) MicroHEMPT (2 mN) MicroHEMPT (3 mN) MBW (400 mN) 0.25 24.2 s 132.6 s 108.3 s 9.4 s 0.40 30.6 s 167.8 s 137.0 s 11.9 s 2.00 68.5 s 375.2 s 306.3 s 26.5 s Duty cycle over 24 h 84% 463% 378% 33% Est. fuel consumption 635 kg over 10 years 18 kg 27 kg 0 kg In the following, the complete manoeuvres are assessed which includes the time where the actuators are operated (corresponds to the manoeuvre times of above table) plus the settling time (mainly driven by the solar array) needed to reach the pointing requirements. Only the APE and PDE are evaluated according to the requirements of Table 4.5-3. The absolute measurement error AME shows the same performance before and after a manoeuvre such that this parameter does not need to be checked. From above figures, the EPS options could already be eliminated since the HEMPT solution needs too much fuel (635 kg of noble gas) and the micro HEMPT system is not suitable because of a duty cycle significantly higher than 100% which means that all the required manoeuvres can not be performed in the required time frame. Nevertheless, all of above options are evaluated to give an impression what is feasible with each of the options. MBW performance The MBW option has the most available torque for both the manoeuvres and the stabilizing after the Doc. No: GOC-ASG-RP-002 Page 4-63 Issue: 2 Date: 13.05.2009 Astrium GmbH

4 <strong>Final</strong><br />

<strong>Report</strong><br />

scan North/South and East/West, respectively. A summary of the manoeuvres required over 24 h is<br />

presented in Table 4.5-6.<br />

Table 4.5-6: Manoeuvre summary<br />

Manoeuvre [deg] Daytime manoeuvres<br />

over 9 h [-]<br />

Nighttime manoeuvres<br />

over 15 h [-]<br />

Total manoeuvres<br />

over 24 h [-]<br />

Manoeuvre time<br />

allocation [s]<br />

0.25 27 0 27 70<br />

0.40 27 0 27 70<br />

2.00 324 720 1044 70<br />

All manoeuvre performance data presented in this section are based on one-axis manoeuvres.<br />

There are several options for manoeuvre actuators. The MBW option is clear, but also two EPS<br />

options, using either the HEMPT 3050 or microHEMPT, have been considered. The MBW option uses<br />

the same wheels for attitude control and manoeuvres, as the torque output from one wheel is<br />

scaleable from 0 to 400 mNm. The wheel drive electronic quantisation is 55 µNm. The EPS can not<br />

throttle its output to the same degree and an additional EPS system is needed for manoeuvres. The<br />

first option is to use the HEMPT 3050 thrusters for manoeuvres which can produce a torque of ±85<br />

mNm around each axis.<br />

In the EPS analysis another option has been introduced as well. MicroHEMPT for attitude control has<br />

a few advantages such as lower fuel and power consumption and system mass, and one obvious<br />

drawback: the long resulting manoeuvre time. An overview of the theoretical, time optimal manoeuvre<br />

time for the various options are listed in Table 4.5-7. Note that these numbers do not allocate time for<br />

a settling period after the completion of the manoeuvre.<br />

Table 4.5-7: Theoretical, time optimal manoeuvre times for HEMPT 3050 and microHEMPT based<br />

configurations, and duty cycle over 24 h<br />

Manoeuvre [deg] HEMPT 3050 (30 mN) MicroHEMPT (2 mN) MicroHEMPT (3 mN) MBW (400 mN)<br />

0.25 24.2 s 132.6 s 108.3 s 9.4 s<br />

0.40 30.6 s 167.8 s 137.0 s 11.9 s<br />

2.00 68.5 s 375.2 s 306.3 s 26.5 s<br />

Duty cycle over 24 h 84% 463% 378% 33%<br />

Est. fuel consumption 635 kg<br />

over 10 years<br />

18 kg 27 kg 0 kg<br />

In the following, the complete manoeuvres are assessed which includes the time where the actuators<br />

are operated (corresponds to the manoeuvre times of above table) plus the settling time (mainly driven<br />

by the solar array) needed to reach the pointing requirements. Only the APE and PDE are evaluated<br />

according to the requirements of Table 4.5-3. The absolute measurement error AME shows the same<br />

performance before and after a manoeuvre such that this parameter does not need to be checked.<br />

From above figures, the EPS options could already be eliminated since the HEMPT solution needs too<br />

much fuel (635 kg of noble gas) and the micro HEMPT system is not suitable because of a duty cycle<br />

significantly higher than 100% which means that all the required manoeuvres can not be performed in<br />

the required time frame. Nevertheless, all of above options are evaluated to give an impression what<br />

is feasible with each of the options.<br />

MBW performance<br />

The MBW option has the most available torque for both the manoeuvres and the stabilizing after the<br />

Doc. No: GOC-ASG-RP-002 Page 4-63<br />

Issue: 2<br />

Date: 13.05.2009 Astrium GmbH

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