The On-Orbit Optical Performance of STIS

نویسنده

  • Charles W. Bowers
چکیده

The Space Telescope Imaging Spectrograph (STIS) is a versatile, general purpose instrument installed aboard the Hubble Space Telescope in February, 1997. During the following Servicing Mission Orbital Verification (SMOV) period, STIS has been made operational and aligned, and initial checkout and calibration completed. The overall optical performance goals have largely been achieved and a summary of these results is presented.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The On-Orbit Performance of the STIS Detectors

The Space Telescope Imaging Spectrograph (STIS), successfully installed into the Hubble Space Telescope in 1997 February, achieves its advances over the rst-generation HST spectrographs primarily through the use of modern largeformat, two-dimensional array detectors. The performance of the STIS detectors, two Multi-Anode Microchannel Arrays (MAMAs) and one CCD, has been evaluated on-orbit as pa...

متن کامل

Thermal Motion of the Stis Optical Bench

Various tests have been done of the STIS using internal wavecals to measure thermal motion of the spectral format on the detectors. In most cases, the spectral format moves less than the speci cation not to exceed 0.2 pixels per hour. Primary causes of the motion are 1) changes to the thermal design dictated by the warmer Aft Shroud environment and 2) on-orbit power cycling of MAMA electronics ...

متن کامل

Performance Evaluation of the High-altitude Launch Technique to Orbit Using Atmospheric Properties

The purpose of this paper is to perform the feasibility and performance evaluation of the High-altitude launch technique using high altitude atmospheric Properties to near earth orbits. The current propulsion transportation system from Earth to space has been deemed by many to be expensive, unreliable, and an unnecessarily dangerous means of travel to space. It is suggested in this paper to ana...

متن کامل

ar X iv : a st ro - p h / 96 11 10 9 v 1 1 4 N ov 1 99 6 Submitted to PASP Imaging With STIS : Astronomy at V = 30

In February, 1997, the second Space Shuttle servicing mission to the Hubble Observatory will install the Space Telescope Imaging Spectrograph (STIS). This new instrument will greatly enhance the spectroscopic capabilities of the Hubble Space Telescope by providing a longslit format and CCD detector technology. STIS can also be used as an imager, providing an alternative to the Wide Field Planet...

متن کامل

Determination of the best-fitting reference orbit for a LEO satellite using the Lagrange coefficients

Linearization of the nonlinear equations and iterative solution is the most well-known scheme in many engineering problems. For geodetic applications of the LEO satellites, e.g. the Earth’s gravity field recovery, one needs to provide an initial guess of the satellite location or the so-called reference orbit. Numerical integration can be utilized for generating the reference orbit if a satelli...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1997