Inertially fixed pitch stabilization of satellites by solar radiation pressure

Utilization of solar radiation pressure to stabilize the pitch attitude of an unsymmetrical satellite along an inertially-fixed orientation is investigated. A controller employing two rotatable highly reflective control surfaces is proposed and a control strategy involving both nominal and feedback controls is synthesized. Accounting for the apparent annual motion of the Sun, the validity of the concept throughout the year is established through a stability analysis of the system. The influence of the Earth's shadow on the controller performance is also analyzed. The speed of response as well as the pointing accuracy capabilities of the system appear to be quite acceptable for long-life scientific missions.     

Solar flares,CMEs and solar energetic particle events during solar cycle 24

We present here a study of Solar Energetic Particle Events (SEPs) associated with solar flares during 2010–2014 in solar cycle 24. We have selected the flare events (≥GOES M-class), which produced SEPs. The SEPs are classified into three categories i.e. weak (proton intensity?≤?1?pfu), minor (1?pfu?<?proton intensity?<?10?pfu) and major (proton intensity?≥?10?pfu). We used the GOES data for the SEP events which have intensity greater than one pfu and SOHO/ERNE data for the SEP event less than one pfu intensity. In addition to the flare and SEP properties, we have also discussed different properties of associated CMEs.     

On optimal aerodynamic attitude control of spacecraft

Attitude control of spin-stabilized satellites by means of aerodynamic forces is investigated. A controller employing two rotatable control surfaces is proposed to control the roll-yaw motions of the spacecraft spin-axis. Optimal control theory is applied to synthesize a feedback control law for the control surface rotations which leads to asymptotically stable controller operation. The system response is interpreted in terms of performance criteria such as the maximum control surface excursions, the speed of response and the associated orbital energy loss due to drag. Even with a moderate size, the controller appears quite effective in maintaining the spacecraft attitude against external disturbances.     

Solar Pressure Attitude Stabilization of Earth-Pointing Spacecraft

The development of a solar pressure control system for three-axis attitude control of Earth-oriented spacecraft is presented. A controller configuration consisting of two rotatable mirrorlike surfaces, representing the minimum hardware implementation, is considered. Optimal control theory is applied to synthesize a feedback control law directly governing the differential rotation of the control surfaces. The system performance is evaluated through the response analysis of a satellite subject to destabilizing gravity gradient torques as well as external disturbances. Even under such adverse conditions, the results indicate a moderately sized controller to be quite effective in maintaining the desired Earth-pointing spacecraft orientation. The validity of the optimal control law is established for all times of the year, and the feasibility of implementing suboptimal control policies is also examined.     

Semipassive Pitch Attitude Control of Satellites by Solar Radiation Pressure

Pitch attitude control of earth-pointing satellites by solar radiation pressure is investigated. Development of a controller that is simple to implement and yet promises asymptotic stability of the system is presented. The analysis establishes the capability of the solar controller in stabilizing even the gravitationally unstable equilibrium orientation. The semipassive nature of the system promises an increased operational lifetime for the satellite.