Engineering topics

Cheng, A. Y. S.

Publications and source records attributed to Cheng, A. Y. S..

4 records

NASA NTRS1986

A space telescope for infrared spectroscopy of earth-like planets

It is shown here that a space telescope of 16 m diameter, apodized in a new way, could image and measure oxygen n in the thermal infrared spectral of earthlike planets up to 4 pc away. The problems of visible light imaging for this case are discussed, and it is argued that imaging the thermal emission, with greatly reduced requirements for gain and hence surface accuracy, is preferable. The requirements for such imaging are discussed, including the apodization solution.

Angel, J. R. P.↗

NASA NTRS1986

Steps toward 8m honeycomb mirrors. VIII - Design and demonstration of a system of thermal control

Directed jets of ambient temperature air are proposed for the maintenance of low internal temperature gradients and conformity with ambient temperatures in honeycomb-structure borosilicate glass telescope mirrors. The use of greater airflow on thicker sections, to match cooling rates, and the cooling or heating of the internal, back, and edge surfaces of the mirror at the same rate established by convection on the front surface, have been tested on a full scale glass thermal model of a single honeycomb cell from an 8-m diameter mirror. The internal thermal gradient (less than 0.1 C) and ambient-temperature-change lag (less than 0.24 C) ensure minimum image degradation.

Cheng, A. Y. S.↗

NASA NTRS1985

Modelling Epsilon Aurigae without solid particles

Three components can be expected to contribute to the emission of epsilon Aurigae. There is a primary F star. There is an opaque disk which occults it, and there is a gas stream which is observed to produce absorption lines. Evidence that the disk is not responsible for the gas stream lines comes both from the radial velocities, which are too small, and from the IR energy distribution out of eclipse, which shows free-free emission that would produce inadequate optical depth in electron scattering. The color temperature of the IR excess can give misleading indications of low temperature material. Free-free emission at 10,000 K between 10 and 20 microns has a color temperature of 350 K. Attempts to mold the system are discussed.

Cheng, A. Y. S.↗

NASA NTRS1981

Compton losses, Compton rockets

The radiation force on a relativistic plasma is shown to accelerate the plasma to relativistic bulk velocities under certain conditions, thus demonstrating that relativistic bulk motion not only alleviates Compton losses, but can also result from such losses. In order to isolate Compton-rocket effects from hydrodynamical ones, it is assumed that the plasma in its instantaneous rest frame has a temporally constant density and is spatially uniform.

Cheng, A. Y. S.↗