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3 edition of Short-term chromospheric variability in Ü Tauri (K5 III) found in the catalog.

Short-term chromospheric variability in Ü Tauri (K5 III)

Short-term chromospheric variability in Ü Tauri (K5 III)

results from IUE time series observations

by

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  • 20 Currently reading

Published by National Aeronautics and Space Administration in [Washington, D.C .
Written in English

    Subjects:
  • Solar flares.,
  • Time-series analysis.,
  • Stellar chromospheres.

  • Edition Notes

    Other titlesShort term chromospheric variability in Ü Tauri (K5 III) :, Astrophysical journal. 1996.
    StatementManfred Cuntz ... [et al.].
    Series[NASA contractor report] -- NASA-CR-204601., NASA contractor report -- NASA CR-204601.
    ContributionsCuntz, Manfred., United States. National Aeronautics and Space Administration.
    The Physical Object
    FormatMicroform
    Paginationp. 426-433.
    Number of Pages433
    ID Numbers
    Open LibraryOL18120716M


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Short-term chromospheric variability in Ü Tauri (K5 III) Download PDF EPUB FB2

Open Library is an open, editable library catalog, building towards a web page for every book ever published. Short-term chromospheric variability in Ü Tauri (K5 III) Manfred Cuntz Not In Library.

Contribution of x-ray and extreme ultraviolet radiation of solar flare. Results of observations of short-term wind variability in the classical T Tauri stars RW Aur and DR Tau are presented. Since the H CaII emission is absorbed by the absorption component of the H∈ line, which arises in the wind at a radial velocity of about − km/s, the ratio of equivalent widths of the H and K emission lines of ionized calcium is used as an indicator of the line-of-sight Cited by: 1.

Hourly values of the total electron content (TEC-Faraday content) collected at five stations in the northern hemisphere extending from the low Short-term chromospheric variability in Ü Tauri book high latitudes lying in the narrow longitude zone of ( ± 20) °E during Short-term chromospheric variability in Ü Tauri book solar maximum years and respectively of the last 21 and 22nd solar cycles and also during the common solar minimum year are used to study the latitudinal Cited by: 1.

chromosphere (krō`məsfēr') [Gr.,=color sphere], layer of rarefied, transparent gases in the solar atmosphere; it measures 6, mi (9, km) in thickness and lies between the photospherephotosphere, luminous, apparently opaque layer of gases that forms the visible surface of the sun or any other star.

The photosphere lies between the dense interior. Short term variability in Be stars and binaries. 3 short-term variability by using PDM and FT+CLEAN algorithm methods. Un-der these conditions we find that 13 Be stars present short-term photometric variability (P. changes of the tw hydrae bright spot 1 C.

Batalha, 2 N. Batalha, 3 S. Alencar, 4 D. Lopes, 2 and E. Duarte 2 Received April 8; accepted July PDF | We obtained high-resolution, high-quality VLT/UVES spectra to reconstruct the two-dimensional surface structure of the rapidly-rotating classical | Find, read and cite all the research.

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G.; Nielsen, K. E.; Kober, G. V.; Ayres, T. R.; Wahlgren, G. M.; Rau, G. Stellar model chromospheres. IX - Chromospheric activity in dwarf stars. NASA Technical Reports Server (NTRS) Kelch, W. L.; Worden, S. P.; Linsky, J. ISIS-2 digital topside ionogram (apparent range vs.

frequency f) illustrating: ¥ p la s m a r e s o n a n c e s ¥ ionospheric penetration freq. f x F 2 ¥ ionospheric reflections when f. Linear Polarization Measurements of Chromospheric Emission Lines. NASA Technical Reports Server (NTRS) Sheeley, N. R., Jr.; Keller, C. We have used the Zurich Imagi.

Highway long short-term memory rnns for distant speech recognition. In ICASSP, [Zhou et al., ] Peng Zhou, Zhenyu Qi, Suncong Zheng, Jiaming Xu, Hongyun Bao, and Bo Xu. Text classi-cation improved by integrating bidirectional lstm with two-dimensional max pooling. arXiv preprint arX-iv, Cited by: 7.

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