Space solar telescope in soft X-ray and EUV band
نویسندگان
چکیده
In this paper we have reviewed our achievements in soft X-ray and extreme ultraviolet (EUV) optics. Up to now, the research system of soft X-ray and EUV optics has been established, including light sources, detectors, calibrations, optical testing and machining of super smooth mirrors, and fabrications of multilayer film mirrors. Based on our achievements, we have developed two types of solar space telescopes for the soft X-ray and EUV space solar observations. One is an EUV multilayer normal incident telescope array including 4 different operation wavelength telescopes. The operation wavelengths of the EUV telescope are 13.0, 17.1, 19.5 and 30.4 nm. The other is a complex space solar telescope, which is composed of an EUV multilayer normal incident telescope and a soft X-ray grazing incident telescope. The EUV multilayer normal incident telescope stands in the central part of the soft X-ray grazing incident telescope. The normal incident telescope and the grazing incident telescope have a common detector. The different operation wavelengths can be changed by rotating a filter wheel.
منابع مشابه
Soho Eit Observations of Extreme-ultraviolet “dimming” Associated with a Halo Coronal Mass Ejection
A solar flare was observed on 1997 April 7 with the Soft X-ray Telescope (SXT) on Yohkoh. The flare was associated with a “halo” coronal mass ejection (CME). The flaring region showed areas of reduced soft X-ray (SXR) brightness—“dimmings”—that developed prior to the CME observed in white light and persisted for several hours following the CME. The most prominent dimming regions were located ne...
متن کاملAn investigation of Fe XVI emission lines in solar and stellar EUV and soft X-ray spectra
New fully relativistic calculations of radiative rates and electron impact excitation cross sections for Fexvi are used to determine theoretical emission-line ratios applicable to the 251–361 Å and 32–77 Å portions of the extreme-ultraviolet (EUV) and soft X-ray spectral regions, respectively. A comparison of the EUV results with observations from the Solar Extreme-Ultraviolet Research Telescop...
متن کاملLarge-scale Solar Coronal Structures in Soft X-rays and Their Relationship to the Magnetic Flux
We have investigated the relationship between magnetic activity and coronal structures using soft X-ray data from the Yohkoh soft X-ray telescope and magnetic field data from the Kitt Peak Solar Observatory for the period of 1991–2001 and EUV data from the Solar and Heliospheric Observatory EUV Imaging Telescope for 1996–2001. The data are reduced to Carrington synoptic maps, which reveal two t...
متن کاملGrazing incidence telescopes: a new class for soft x-ray and EUV spectroscopy; addendum.
References 1. M. C. Hettrick and S. Bowyer, "Grazing Incidence Telescopes: a New Class for Soft X-Ray and EUV Spectroscopy," Appl. Opt. 23, 3732 (1984). 2. G. Schmidtke, "Infrared-XUV Telescope for Multipurpose Applications," Appl. Opt. 16, 244 (1977). 3. G. Schmidtke, P. Henneberg, K.-H. Hager, F. Busch, and D. Reinhardt, "Parabolic Telescope and Spectrometer Combination," Appl. Opt. 19, 1822 ...
متن کاملResolving Differences in Absolute Irradiance Measurements Between the SOHO/CELIAS/SEM and the SDO/EVE
The Solar EUV Monitor (SEM) onboard SOHO has measured absolute extreme ultraviolet (EUV) and soft X-ray solar irradiance nearly continuously since January 1996. The EUV Variability Experiment (EVE) on SDO, in operation since April of 2010, measures solar irradiance in a wide spectral range that encompasses the band passes (26 - 34 nm and 0.1 - 50 nm) measured by SOHO/SEM. However, throughout th...
متن کامل