Zobrazeno 1 - 10
of 24
pro vyhledávání: '"J. D. Bohlin"'
Autor:
J. D. Bohlin
Publikováno v:
Physics of Solar Planetary Environments: Proceedings of the International Symposium on Solar - Terrestrial Physics, June 7-18,1976 Boulder, Colorado, Volume I
Coronal hole data obtained by Skylab during the period May 1973 to February 1974 are reviewed for the region from the photosphere out through the low corona. Coronal holes have a significantly lower density and temperature than the typical background
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::692d00a80adfe3000b5dd104cfac6563
https://doi.org/10.1029/sp007p0114
https://doi.org/10.1029/sp007p0114
Autor:
W. C. Feldman, J. Anderson, J. D. Bohlin, L. F. Burlaga, R. Farquhar, G. Gloeckler, B. E. Goldstein, J. W. Harvey, T. E. Holzer, W. V. Jones, P. J. Kellogg, S. M. Krimigis, M. R. Kundu, A. J. Lazarus, M. M. Mellott, E. N. Parker, R. Rosner, G. J. Rottman, J. A. Slavin, S. T. Suess, B. T. Tsurutani, R. T. Woo, R. D. Zwickl
Publikováno v:
AIP Conference Proceedings.
The Solar Probe will deliver a 133.5 kg science payload into a 4 R(S) perihelion solar polar orbit to explore in situ one of the last frontiers in the solar system - the solar corona. Using a payload of 12 scientific experiments, it will be possible
Publikováno v:
Solar Physics. 45:363-376
The origin of the material ejected during a white-light coronal transient on August 26 and 27, 1973, is investigated using simultaneous observations of a slowly ascending prominence and the more rapid accompanying coronal transient. Nearly identical
Autor:
J. D. Bohlin
Publikováno v:
Solar Physics. 51:377-398
The disk boundaries of coronal holes have been systematically determined from XUV observations taken during the manned Skylab missions (June 1973-January 1974). The resulting atlas was used to find the sizes, global distributions, differential rotati
Autor:
Richard B. Hoover, Guenter E. Brueckner, Einar Tandberg-Hanssen, J. P. Mc Guire, J. D. Bohlin, Robert M. Wilson, N. R. Sheeley, V. E. Scherrer, A. C. De Loach, J. B. Smith, Richard Tousey, D. M. Speich, J. D. Purcell
Publikováno v:
Solar Physics. 45:377-392
Skylab/ATM observations of a disappearing filament near the center of the solar disk are described using XUV and H-alpha spectroheliograms, X-ray filterheliograms, and photospheric magnetograms. The temperature of the coronal plasma as the filament d
Autor:
J. D. Bohlin, N. R. Sheeley
Publikováno v:
Solar Physics. 56:125-151
Skylab and ground-based observations in the extreme UV range of the spectrum are used to analyze characteristics of coronal holes, and to correlate their development with variations in the solar cycle. The mergence of bipolar magnetic regions (BMR) d
Autor:
Richard Tousey, N. R. Sheeley, V. E. Scherrer, Guenter E. Brueckner, J. D. Purcell, J. D. Bohlin
Publikováno v:
Solar Physics. 40:103-121
Spectroheliograms obtained with the Naval Research Laboratory's Extreme Ultraviolet Spectrograph (S082A) on Skylab are compared with Kitt Peak National Observatory magnetograms. A principal result is the characteristic reconnection of flux from an em
Autor:
L. M. Garrison, J. D. Bohlin
Publikováno v:
Solar Physics. 38:165-179
A general computer program has been developed to numerically integrate the Thomson scattered light from arbitrary inhomogeneous models of the solar corona. Conversion from the observer's to solar coordinates is totally general to eliminate restrictio
Autor:
R. Tousey, J.-D. F. Bartoe, J. D. Bohlin, G. E. Brueckner, J. D. Purcell, V. E. Scherrer, R. J. Schumacher, N. R. Sheeley, M. E. Vanhoosier
Publikováno v:
Symposium - International Astronomical Union. 57:491-495
The Naval Research Laboratory prepared three instruments for ATM and also a series of rocket payloads for purposes of calibration, under the overall direction of R. Tousey, the Principal Investigator. In this preliminary report a summary of results f
Autor:
R. J. Schumacher, J. D. F. Bartoe, N. R. Sheeley, V. E. Scherrer, M. E. Vanhoosier, Guenter E. Brueckner, J. D. Bohlin, J. D. Purcell, Richard Tousey
Publikováno v:
Solar Physics. 33:265-280
Some of the first observations obtained with the Naval Research Laboratory's Extreme Ultraviolet Spectrograph (S082A) during the first Skylab mission are presented and compared with magnetograms and other ground-based data. The instrument is a slitle