2 edition of The SERTS-97 rocket experiment to study activity on the sun found in the catalog.
The SERTS-97 rocket experiment to study activity on the sun
by National Aeronautics and Space Administration, Goddard Space Flight Center, National Technical Information Service, distributor in Greenbelt, Md, [Springfield, Va
|Statement||Marvin Swartz ... [et al.].|
|Series||NASA/TP -- 1999-208640., NASA technical paper -- 208640.|
|Contributions||Swartz, Marvin., Goddard Space Flight Center.|
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This paper describes mainly the version of the Solar EUV Rocket Telescope and Spectrograph (SERTS), a scientific experiment that operated on NASA's suborbital rocket flight GS. Its function was to study activity on the Sun and to provide a cross calibration for the CDS instrument on the SOHO satellite.
Get this from a library. The SERTS rocket experiment to study activity on the sun: flight GS on November [Marvin Swartz; Goddard Space Flight Center.;]. The politics of British foreign policy in the era of Disraeli and Gladstone / Marvin Swartz Macmillan in association with St.
Antony's College, Oxford London Wikipedia Citation Please see Wikipedia's template documentation for further citation fields that may be required. The SOHO instruments are designed for solar studies.
A high spatial resolution is therefore one of the main goals for most of them. Only SEM is a full-Sun instrument and provides the solar irradiance, E Δλ, in its wavelength corresponding observations are shown in Fig.on the other hand, is a full-Sun imager providing the solar radiance, L Δλ, in its spectral bands Cited by: 4.
the rocket payload were carried out in the same facility used for pre-launch calibrations of CDS and EIS. During the ﬂight, EUNIS, SOHO CDS.
the role of velocity redistribution in enhancing the intensity of the He II LINE IN THE QUIET-SUN SPECTRUM A V INCENZO A NDRETTA, 1,2 S TUART D.
J ORDAN,J EFFREY W. B ROSIUS, 3 J OSEPH M. 1), flare activity in several wavelengths (Figure 2), and the liftoff of CMEs from the Sun (Figure 3). Predicting when the flares and CMEs occur is the next step in our effective use of space.
That is one of the goals of NASA’s Living with a Star (LWS) Program, NASA's first program dedicated to studying the causeFile Size: 1MB. Title: VizieR Online Data Catalog: UV spectrum of the quiet Sun above the limb (Warren+, ) Authors: Warren, H. P.; Ugarte-Urra, I.; Landi, E.
yCatW Altcode: First, we compare full-disk mosaics constructed by scanning the EIS slot over the Sun with irradiance observations made by the EUV Variability Experiment (EVE; Woods. The complement of instruments carried by this spacecraft permits the study of the.
entire Sun – from its innermost core out into the heliosphere, beyond the Earth’s orbit. SOHO’s vantage point in a halo orbit around Lagrange point L 1 on the Earth-Sun line, × 10 6 km away from the Earth towards the Sun (Figure 1), is fundamental to. Разработка зеркальной оптики нормального падения для ВУФ диапазона потребовала проведения детальных исследований отражающих свойств зеркал.
Качество зеркал, работающих в рентгеновском и ВУФ диапазонах спектра. explanation blue bibcodes open ADS page with paths to full text Author name code: gopalswamy ADS astronomy entries on author:"Gopalswamy, Nat" Title: The shock driving capability of a CME inferred from multiwavelength observations Authors: Kassa Dagnew, Fithanegest; Gopalswamy, Nat; Belay Tessema, Solomon; Umuhire, Ange Cynthia; Yashiro.
Zhang, Jie, A study of the Sun's corona using EUV and radio observations, Thesis (PhD). University Of Maryland College Park, Source DAI-B 60/12,p.
Слемзин, Владимир Алексеевич. Зеркальные телескопы ВУФ диапазона для внеатмосферной.