2021
DOI: 10.1016/j.ast.2021.107150
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Collinear artificial equilibrium point maintenance with a wrinkled solar sail

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Cited by 23 publications
(8 citation statements)
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“…where a c is the spacecraft characteristic acceleration, that is, the acceleration magnitude induced by the solar sail when its nominal plane is perpendicular to the Sun-spacecraft line at a distance r = r ⊕ 1 au, and α ∈ [−90, 90] deg is the sail pitch angle measured counterclockwise from the Sun-spacecraft line; see Figure 5. The solar sail is here described through an augmented ideal force model [24,25] without degradation [26][27][28] or wrinkles [29]. In this context, the sail is assumed to maintain a flat surface, and the direction of the propulsive acceleration vector is normal to the sail nominal plane in the direction opposite to the Sun.…”
Section: Mission Optimizationmentioning
confidence: 99%
“…where a c is the spacecraft characteristic acceleration, that is, the acceleration magnitude induced by the solar sail when its nominal plane is perpendicular to the Sun-spacecraft line at a distance r = r ⊕ 1 au, and α ∈ [−90, 90] deg is the sail pitch angle measured counterclockwise from the Sun-spacecraft line; see Figure 5. The solar sail is here described through an augmented ideal force model [24,25] without degradation [26][27][28] or wrinkles [29]. In this context, the sail is assumed to maintain a flat surface, and the direction of the propulsive acceleration vector is normal to the sail nominal plane in the direction opposite to the Sun.…”
Section: Mission Optimizationmentioning
confidence: 99%
“…Therefore, this model is often referred to as "ideal" SRP acceleration model. Unlike other models that take into account the optical properties of the sail film material [1,[25][26][27] or more complex sail shapes [28][29][30][31], the ideal SRP acceleration model allows for a straightforward definition of the SRP acceleration, which becomes a function of the sailcraft attitude only and can be conveniently expressed in the sail-fixed reference frame O S as [1]: a SRP,S = νa c cos 2 α nS (8) where ν ∈ [0, 1] is the shadow factor and a c denotes the sailcraft characteristic acceleration defined as [1]:…”
Section: Solar Radiation Pressure Accelerationmentioning
confidence: 99%
“…. , n * O ,NBH,16(30) which is then used to find the final interpolated normal direction, n * O , as:2 When performing the normalization, two of the three Cartesian components of the λ direction are considered instead of the spherical coordinates θ and φ to avoid dealing with discontinuous variables in the interpolation process.n *O =…”
mentioning
confidence: 99%
“…In terms of attitude control, although there exists a variety of conventional attitude control methods such as reaction wheels, control moment gyroscopes (CMGs) and thrusters, these methods cannot effectively control the attitude of solar sails due to the mass limitation and the required long mission lifetime [1,3,11]. Currently, several methods for attitude control for solar sails exist [17], including the control vane method [18], gimbaled masses method [19,20], sliding masses method, shifted wings method, tilted wings method and billowed wings method for rigid solar sail and sail film with controllable reflectivity method for non-rigid solar sail [3,[21][22][23]. Qu et al also proposed a control method utilizing individually controllable elements to control each sail [24].…”
Section: Introductionmentioning
confidence: 99%