Zobrazeno 1 - 4
of 4
pro vyhledávání: '"O. L. Lupie"'
Autor:
S. Rosborough, C. W. Freer, L. C. Spalsbury, D. D. Gardner, Fred L. Roesler, Menelaos Sarantos, M. A. Gallant, Ronald J. Oliversen, Edwin J. Mierkiewicz, O. L. Lupie, Nickolas J. Derr, D. C. P. Kuruppuaratchi
Publikováno v:
Journal of Geophysical Research: Planets. 123:2430-2444
We present the first comprehensive set of lunar exospheric line width and line width derived effective temperatures as a function of lunar phase (66° waxing phase to 79° waning phase). Data were collected between November 2013 and May 2014 during s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d257cd206e1fb99a1515c841fc717174
https://doi.org/10.1029/2018je005717
https://doi.org/10.1029/2018je005717
Publikováno v:
Journal of Geophysical Research: Space Physics. 119:4950-4956
We have applied high-resolution Fabry-Perot spectroscopy to the study of the lunar sodium exosphere for the study of exospheric effective temperature and velocity variations. Observing from the National Solar Observatory McMath-Pierce Telescope, we u
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4b6e923bcd2554dc5455d8e4e5ddb9cc
https://doi.org/10.1002/2014ja019801
https://doi.org/10.1002/2014ja019801
Autor:
Frank Scherb, Jeffrey P. Morgenthaler, R. Carey Woodward, Kurt D. Retherford, M. L. Marconi, Ronald J. Oliversen, O. L. Lupie, Melanie E. Freed, William H. Smyth
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:26183-26193
A large database of sunlit Io [O I] 6300 A emission, acquired over the period 1990–1999, with extensive coverage of Io orbital phase angle ϕ and System III longitude λIII, exhibits significant long-term and short-term variations in [O I] 6300 A e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d12bce614299385c1f5bef0a0b42e005
https://doi.org/10.1029/2000ja002507
https://doi.org/10.1029/2000ja002507
Publikováno v:
Publications of the Astronomical Society of the Pacific. 90:154
We examine the kinematics of the known variable DA white dwarfs relative to a sample of observed nonvariable DA white dwarfs in the same color range. The variable DA stars do not form a kinematically distinct group relative to the nonvariable stars.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1d22fb0ca856b7682db6939b234f7e46
https://doi.org/10.1086/130298
https://doi.org/10.1086/130298