48th AIAA/ASME/SAE/ASEE Joint Propulsion Conference &Amp;amp; Exhibit 2012
DOI: 10.2514/6.2012-4022
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Performance of Miniature Microwave Discharge Ion Thruster for Drag-free Control

Abstract: Drag-free control systems have been studied to detect gravitational waves by measuring distortions in the fabric of space-time. The purpose of drag-free control is to counteract nongravitational forces such as residual aerodynamic drag or solar radiation pressure. The objective of this study is to use miniature microwave discharge ion thruster, 1, for this propulsion system. In this experiment, the thrust dynamic range was between 7-100 %, and the thrust noise was less than 0.02 N/Hz 1/2 in the frequency ran… Show more

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Cited by 10 publications
(8 citation statements)
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“…Under the conditions of flow rate 0.1 sccm, microwave power 0.5~2.0 W, and acceleration voltage 150~1850 V, the thrust can be continuously adjusted in the range of 1.38~139.18 µN [13]. The microwave ion thruster µ1, designed for the DECIGO pathfinder mission, suppresses the thrust noise in the 0.1~1 Hz band to less than 0.2 µN/Hz 1/2 by means of closed-loop feedback control of the input microwave power [14], which effectively suppresses the low-frequency disturbances but still requires more precise feedback control means.…”
Section: Descriptionmentioning
confidence: 99%
“…Under the conditions of flow rate 0.1 sccm, microwave power 0.5~2.0 W, and acceleration voltage 150~1850 V, the thrust can be continuously adjusted in the range of 1.38~139.18 µN [13]. The microwave ion thruster µ1, designed for the DECIGO pathfinder mission, suppresses the thrust noise in the 0.1~1 Hz band to less than 0.2 µN/Hz 1/2 by means of closed-loop feedback control of the input microwave power [14], which effectively suppresses the low-frequency disturbances but still requires more precise feedback control means.…”
Section: Descriptionmentioning
confidence: 99%
“…LISA, as a pioneer of space-borne GW observatory, has selected four types of thrusterscold gas thruster (CGT), radio frequency ion thruster (RIT), colloidal micro-Newton thruster (CMNT), and high efficiency multipole propulsion (HEMP) [13]. Lots of institutions are interested in these kinds of micro-propulsions and made a series of progress [14][15][16][17][18][19][20][21][22]. Especially, in 2016, LISA pathfinder, as a precursor satellite of LISA, carries the CMNT for providing a thrust dynamic range of 5-30 µN and a resolution of 0.1 µN [23,24].…”
Section: Introductionmentioning
confidence: 99%
“…As a result, the residual differential acceleration of the two TMs in LISA pathfinder is effectively suppressed to be less than 5 fm s −2 at 10 −3 Hz meeting the requirement of LISA [25]. On the other hand, for the Taiji, TianQin, and DECIGO programs, they are tested with RIT, CGT, and electron cyclotron resonance ion thruster (ECRIT) in orbit or on the ground, respectively [20,26,27]. The results of these tests are listed in table 1.…”
Section: Introductionmentioning
confidence: 99%
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“…Hiroyuki Koizumi et al in the Institute of Space and Astronautical Science (ISAS) developed a micro power ECRIT, which was called μ1 [8,9]. The cylinder discharge chamber diameter of μ1 was 2 cm, and the maximum magnetic field intensity was 0.3 T while the minimum magnetic field intensity was 0.05 T. The performances of the thrust, specific impulse, and efficiency with 4 W input power for μ1 were 250 µN, 5500 s, and 32%, respectively.…”
Section: Introductionmentioning
confidence: 99%