SSRT: First results of millisecond spike observations

We present the results of the first observations of spike-like phenomena with the Siberian Solar Radio Telescope (SSRT) in the one-dimensional mode at the frequency of 5.7 GHz with high spatial and temporal resolutions.     

An adaptive controller for current-fed induction motor

A model reference speed adaptive controller for a current-fed induction motor drive is proposed. It uses a proportional-plus-integral (PI) adaptation to satisfy the hyperstability condition for taking care of the load and machine parameter changes of the drive. The available information on the states and output of the reference model as well as the plant output are all that are required for the control; no explicit parameter identification is needed. The controller can be designed by using a reduced reference model to simplify the design without much degradation of the performance, so that it is relatively easy to implement practically     

Digital control algorithms for multi-degree-of-freedom microgravity isolation systems

Two general methodologies have been developed to design digital controllers for multi-degree-of-freedom microgravity isolation systems such that the desired transmissibility matrix is achieved. The absolute accelerations and relative displacements are used as feedback signals. Absolute acceleration signals are used to provide proportional damping in the system whereas relative displacement signals are used to achieve the desired transmissibility. In the first method, the closed-form expression of the controller transfer function metrix for the relative displacement feedback is obtained directly in the Z-domain. The controller transfer function matrix is first obtained in the S-domain and then discretized in the second method. The discrete-time controller transfer function matrices and numerical results are presented for a three-degree-of-freedom system with attractive electromagnetic actuators.     

Missile Guidance Based on Kalman Filter Estimation of Target Maneuver

A fourth-order extended Kalman filter is developed to estimate target maneuvers, and a guidance law using these estimates is implemented.     

Highlights of the 1975 URSI/COSPAR workshop on the IRI

Some of the presentations made at the IRI Workshop held at Louvain in 1985 have not appeared in the Proceedings. Some discussions which took place during the workshop could be of interest in future work. This article tries to highlight the IRI modelling aspects in the four principal height regions of the ionosphere.     

The influence of pressure on combustion intensity

The influence of pressure in the range of 3–15 kgf/cm² on combustion intensity is studied experimentally in a medium-sized rig. The apparatus is described and temperature measurements by different thermocouple techniques are discussed; gas composition was monitored by gas chromatography. The experiments were performed at different cross sections allowing to map temperatures and gas concentrations. The results show that temperature and carbon dioxide concentration increase more rapidly as the pressure is raised. Carbon monoxide appears as an intermediate and is concentrated near the combustion axis. The combustion zone becomes shorter with increasing pressure and the combustion intensity increases correspondingly.     

The composition of heavy ions in solar energetic particle events

We review recent advances in determining the elemental, charge-state, and isotopic composition of 1 to 20 MeV per nucleon ions in solar energetic particle (SEP) events and outline our current understanding of the nature of solar and interplanetary processes which may explain the observations.The composition within individual SEP events may vary both with time and energy, and will in general be different from that in other SEP events. Average values of relative abundances measured in a large number of SEP events, however, are found to be roughly energy independent in the 1 to 20 MeV per nucleon range, and show a systematic deviation from photospheric abundances which seems to be organized in terms of the first ionization potential of the ion.Direct measurements of the charge states of SEPs have revealed the surprisingly common presence of energetic He⁺ along with heavy ions with typically coronal ionization states. High-resolution measurements of isotopic abundance ratios in a small number of SEP events show these to be consistent with the universal composition except for the puzzling overabundance of the SEP ²²Ne/²⁰Ne relative to this isotopes ratio in the solar wind. The broad spectrum of observed elemental abundance variations, which in their extreme result in composition anomalies characteristic of ³He-rich, heavy-ion rich and carbon-poor SEP events, along with direct measurements of the ionization states of SEPs provide essential information on the physical characteristics of, and conditions in the source regions, as well as important constraints to possible models for SEP production.It is concluded that SEP acceleration is a two-step process, beginning with plasma-wave heating of the ambient plasma in the lower corona, which may include pockets of cold material, and followed by acceleration to the observed energies by either flare-generated coronal shocks or Fermi-type processes in the corona. Interplanetary propagation as well as acceleration by interplanetary propagating shock will often further modify the composition of SEP events, especially at lower energies.     

Power Converter Design Optimization

Utilizing the demonstrated capability of nonlinear programming algorithms, a practical design optimization approach for power converters is established which allows conception of a design to meet all power-circuit performance requirements and concurrently optimize a defined quantity such as weight or losses. In addition to facilitating a costeffective design, the computer-aided approach provides a means to readily assess 1) the weight-efficiency tradeoff, 2) impacts of converter requirements and component characteristics on a given design, and 3) optimum powersystem configurations.     

Cos-B X-ray observations of Cyg X-3; An indication for apsidal motion

Results are presented of three 40 d COS-B X-ray observations of Cyg X-3. The shape of the 4.8 h light curve showed variations on all observational time scales. An 20 d periodicity was found in the arrival time of the minimum of the light curve, interpreted as apsidal motion of an orbit with an eccentricity of 0.03.