Zobrazeno 1 - 10
of 12
pro vyhledávání: '"P. E. Reichley"'
Autor:
Daniel J. McCleese, David J. Diner, John Theodore Houghton, L. S. Elson, S. E. Bradley, J. T. Schofield, Martha S. Hanner, J. V. Martonchik, Fredric W. Taylor, P. E. Reichley, Andrew P. Ingersoll, J. Delderfield
Orbiter infrared measurements of the Venus atmosphere in the 60- to 140-kilometer region show very small diurnal temperature differences near the cloud tops, increasing somewhat at higher levels. The seasonal (that is, equator to pole) contrasts are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8f475b93e9d92a4d5fed2322e4f0f51
https://ora.ox.ac.uk/objects/uuid:ae4d83e6-2483-45c5-84c3-cedc6d307c76
https://ora.ox.ac.uk/objects/uuid:ae4d83e6-2483-45c5-84c3-cedc6d307c76
Publikováno v:
Icarus. 26:273-312
The Goldstone radar system was used at a wavelength of 12.6 cm to probe the Martian surface during the 1973 opposition. Measurements of range and reflected power were made at least weekly between July 12 and November 24. Surface cells isolated by the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ff90f7083d3328667bfd78d3a016b9af
https://doi.org/10.1016/0019-1035(75)90173-6
https://doi.org/10.1016/0019-1035(75)90173-6
Publikováno v:
Icarus. 33:441-453
The Goldstone radar system was operated at wavelengths of 3.5 and 12.6 cm to probe the Martian surface during the 1975 opposition. Regions studied in detail by range-Doppler techniques are Syrtis Major, Sinus Meridiani, and the crater Schiaparelli. A
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4bf4ec055d2f26c7a21eed805748a3a4
https://doi.org/10.1016/0019-1035(78)90183-5
https://doi.org/10.1016/0019-1035(78)90183-5
Publikováno v:
Icarus. 18:8-21
Taking advantage of the favorable opposition of 1971, the Goldstone radar system, operating at 2388 MHz, was used to scan the Martian surface. Measurements of altitude and reflected power were taken approximately every 3 days. Each measurement repres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::752c81f45ba4b0e4e5e839fb92cdff43
https://doi.org/10.1016/0019-1035(73)90168-1
https://doi.org/10.1016/0019-1035(73)90168-1
Publikováno v:
Nature. 222:1257-1258
Pulsars observed for average energies at centimeter wavelengths, using azimuth elevation antenna
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e8169f243507141c310f3c741bd92718
https://doi.org/10.1038/2221257a0
https://doi.org/10.1038/2221257a0
Autor:
G. S. Downs, P. E. Reichley
Publikováno v:
Nature. 222:229-230
Pulsar PSR 0833-45 period decrease and rate of change in period increased between 24 February-3 March 1969, discussing contraction explanation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c2b3c7d72b5632cd82c5c11d07e14477
https://doi.org/10.1038/222229a0
https://doi.org/10.1038/222229a0
Autor:
J. Delderfield, John V. Martonchik, John C. Gille, Reinhard Beer, J. Leung, M. T. Chahine, David J. Diner, Daniel J. McCleese, R. D. Haskins, Crofton B. Farmer, S. P. Bradley, Fredric W. Taylor, Lucien Froidevaux, John T. Schofield, P. E. Reichley, M. T. Coffey, L. S. Elson
Publikováno v:
Journal of Geophysical Research. 85:7963
The results of the Pioneer Venus orbiter radiometric temperature-sounding experiment are presented with examples of each of the primary data products. The measured temperature field is used to model the dynamics of the middle atmosphere from 60 to 14
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e9f77c53b659616c7b2eab9c8e464261
https://doi.org/10.1029/ja085ia13p07963
https://doi.org/10.1029/ja085ia13p07963
Autor:
G. S. Downs, P. E. Reichley
Publikováno v:
The Astrophysical Journal Supplement Series. 53:169
Monitoring of the behavior of naturally pulsating galactic radio sources, or pulsars, through regularly spaced measurements of pulse arrival times, has been conducted by several laboratories. A tabular presentation is here made of pulse arrival time
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0050e25244ef4f8361872ae1ed0a46f6
https://doi.org/10.1086/190890
https://doi.org/10.1086/190890
Publikováno v:
The Astrophysical Journal. 181:L143
Eleven pulsars were observed and five were detected at 15.1 GHz. Several exhibit strong scintillations at 8.4 GHz. Estimates are made of the spectral indices of five pulsars. Average pulse shapes are presented for the stronger signals.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5b245358fe73b4e31d63eaf7349ec9e5
https://doi.org/10.1086/181202
https://doi.org/10.1086/181202
Autor:
G. S. Downs, P. E. Reichley
Publikováno v:
The Astrophysical Journal. 163:L11
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9b13515b46c460413c40f35ba5243f64
https://doi.org/10.1086/180657
https://doi.org/10.1086/180657