Zobrazeno 1 - 10
of 48
pro vyhledávání: '"J L Innis"'
Autor:
R. J. Sica, M. R. M. Izawa, K. A. Walker, C. Boone, S. V. Petelina, P. S. Argall, P. Bernath, G. B. Burns, V. Catoire, R. L. Collins, W. H. Daffer, C. De Clercq, Z. Y. Fan, B. J. Firanski, W. J. R. French, P. Gerard, M. Gerding, J. Granville, J. L. Innis, P. Keckhut, T. Kerzenmacher, A. R. Klekociuk, E. Kyrö, J. C. Lambert, E. J. Llewellyn, G. L. Manney, I. S. McDermid, K. Mizutani, Y. Murayama, C. Piccolo, P. Raspollini, M. Ridolfi, C. Robert, W. Steinbrecht, K. B. Strawbridge, K. Strong, R. Stübi, B. Thurairajah
Publikováno v:
Atmospheric Chemistry and Physics, Vol 8, Iss 1, Pp 35-62 (2008)
An ensemble of space-borne and ground-based instruments has been used to evaluate the quality of the version 2.2 temperature retrievals from the Atmospheric Chemistry Experiment Fourier Transform Spectrometer (ACE-FTS). The agreement of ACE-FTS tempe
Externí odkaz:
https://doaj.org/article/ab01851b5ca34d07bb3dd0ead09407c1
Publikováno v:
Annales Geophysicae, Vol 20, Pp 1987-2001 (2002)
Thermospheric mean vertical winds from high-resolution Fabry-Perot Spectrometer observations of the l630 nm emission (from ~ 240 km altitude), over a four year interval 1997–2000, from Mawson (67.6° S, 62.9° E, Inv 70.5° S) and Davis (68
Externí odkaz:
https://doaj.org/article/7caef804720e4ae4a94687b163092b50
Publikováno v:
Annales Geophysicae, Vol 19, Pp 533-543 (2001)
Zenith-directed Fabry-Perot Spectrometer (FPS) and 3-Field Photometer (3FP) observations of the λ630 nm emission (~240 km altitude) were obtained at Davis station, Antarctica, during the austral winter of 1999. Eleven nights of suitable data wer
Externí odkaz:
https://doaj.org/article/a9b93767d8b54ac5904c210c1ff297d7
Publikováno v:
Annales Geophysicae, Vol 19, Iss 3, Pp 359-365 (0000)
Annales Geophysicae, Vol 19, Pp 359-365 (2001)
Annales Geophysicae, Vol 19, Pp 359-365 (2001)
We present observations of the hydroxyl (6–2) airglow lines from ~ 87 km altitude obtained at Davis station, Antarctica, in the austral winter of 1999. Nine nights of observations were made of the P-branch near λ840 nm with a Czerny-Turner scannin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb32c68c4bdbc79b95954d99dad9117f
https://www.ann-geophys.net/19/359/2001/
https://www.ann-geophys.net/19/359/2001/
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 420:2539-2545
Bayesian statistical methods of Gregory-Loredo and the Bretthorst generalization of the Lomb-Scargle periodogram have been applied for studying activity cycles of the early K-type subgiant star CF Oct. We have used a ~45 year long dataset derived fro
Autor:
Mark Conde, J. L. Innis
Publikováno v:
Geophysical Research Letters. 28:3847-3850
Large-scale distribution of thermospheric vertical wind activity was studied using observations from the Wind and Temperature Spectrometer on the Dynamics Explorer-2 satellite. We calculated the vertical velocity standard deviation, σ(Vz), within a
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 63:1571-1584
Neutral wind upwelling events are well documented in both the northern and southern high latitude ionosphere. The vertical winds in the F-region frequently exceed 100 m / s , and winds in excess of 200 m / s have been observed. These upwelling events
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:15489-15499
Five years of photometric data of the λ630 nm oxygen auroral/airglow emission (∼240-km altitude) over Davis, Antarctica (Λ=−74.6°), are searched for evidence of periodic oscillations due to atmospheric gravity waves. Data were selected for int
Autor:
J. L. Innis
Publikováno v:
Geophysical Research Letters. 27:3813-3816
This letter explores the hypothesis that gravity wave drag may account for the observed deceleration of the thermospheric anti-sunward wind near the nightside auroral oval, which at times has been seen to reduce to near zero in a horizontal distance
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 310:377-386
The Wilson–Devinney program is used to model 27 light curves (our own and others) for CF Tuc. We find new parameters for the binary system, and estimate the longitudes and radii of the spots on the cooler secondary star. We also find a strong tende