Search Results - (Author, Cooperation:R. J. Strangeway)
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1G. Paschmann, S. E. Haaland, T. D. Phan, B. U. Ö. Sonnerup, J. L. Burch, R. B. Torbert, D. J. Gershman, J. C. Dorelli, B. L. Giles, C. Pollock, Y. Saito, B. Lavraud, C. T. Russell, R. J. Strangeway, W. Baumjohann, S. A. Fuselier
Wiley-Blackwell
Published 2018Staff ViewPublication Date: 2018-02-16Publisher: Wiley-BlackwellPrint ISSN: 0148-0227Topics: GeosciencesPhysicsPublished by: -
2Staff View
Publication Date: 2018-01-30Publisher: Wiley-BlackwellPrint ISSN: 0094-8276Electronic ISSN: 1944-8007Topics: GeosciencesPhysicsPublished by: -
3A. C. Rager, J. C. Dorelli, D. J. Gershman, V. Uritsky, L. A. Avanov, R. B. Torbert, J. L. Burch, R. E. Ergun, J. Egedal, C. Schiff, J. R. Shuster, B. L. Giles, W. R. Paterson, C. J. Pollock, R. J. Strangeway, C. T. Russell, B. Lavraud, V. N Coffey, Y. Saito
Wiley-Blackwell
Published 2018Staff ViewPublication Date: 2018-01-11Publisher: Wiley-BlackwellPrint ISSN: 0094-8276Electronic ISSN: 1944-8007Topics: GeosciencesPhysicsPublished by: -
4R. E. Denton, B.U.Ö. Sonnerup, C. T. Russell, H. Hasegawa, T. D. Phan, R. J. Strangeway, B. L. Giles, R. E. Ergun, P.-A. Lindqvist, R. B. Torbert, J. L. Burch, S. K. Vines
Wiley-Blackwell
Published 2018Staff ViewPublication Date: 2018-02-22Publisher: Wiley-BlackwellPrint ISSN: 0148-0227Topics: GeosciencesPhysicsPublished by: -
5M. Zhou, J. Berchem, R. J. Walker, M. El-Alaoui, M. L. Goldstein, G. Lapenta, X. Deng, J. Li, O. Le Contel, D. B. Graham, B. Lavraud, W. R. Paterson, B. L. Giles, J. L. Burch, R. B. Torbert, C. T. Russell, R. J. Strangeway, C. Zhao, R. E. Ergun, P.-A. Lindqvist, G. Marklund
Wiley-Blackwell
Published 2018Staff ViewPublication Date: 2018-02-22Publisher: Wiley-BlackwellPrint ISSN: 0148-0227Topics: GeosciencesPhysicsPublished by: -
6M. Akhavan-Tafti, J. A. Slavin, G. Le, J. P. Eastwood, R. J. Strangeway, C. T. Russell, R. Nakamura, W. Baumjohann, R. B. Torbert, B. L. Giles, D. J. Gershman, J. L. Burch
Wiley-Blackwell
Published 2018Staff ViewPublication Date: 2018-02-06Publisher: Wiley-BlackwellPrint ISSN: 0148-0227Topics: GeosciencesPhysicsPublished by: -
7J. L. Burch ; R. B. Torbert ; T. D. Phan ; L. J. Chen ; T. E. Moore ; R. E. Ergun ; J. P. Eastwood ; D. J. Gershman ; P. A. Cassak ; M. R. Argall ; S. Wang ; M. Hesse ; C. J. Pollock ; B. L. Giles ; R. Nakamura ; B. H. Mauk ; S. A. Fuselier ; C. T. Russell ; R. J. Strangeway ; J. F. Drake ; M. A. Shay ; Y. V. Khotyaintsev ; P. A. Lindqvist ; G. Marklund ; F. D. Wilder ; D. T. Young ; K. Torkar ; J. Goldstein ; J. C. Dorelli ; L. A. Avanov ; M. Oka ; D. N. Baker ; A. N. Jaynes ; K. A. Goodrich ; I. J. Cohen ; D. L. Turner ; J. F. Fennell ; J. B. Blake ; J. Clemmons ; M. Goldman ; D. Newman ; S. M. Petrinec ; K. J. Trattner ; B. Lavraud ; P. H. Reiff ; W. Baumjohann ; W. Magnes ; M. Steller ; W. Lewis ; Y. Saito ; V. Coffey ; M. Chandler
American Association for the Advancement of Science (AAAS)
Published 2016Staff ViewPublication Date: 2016-05-14Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
8Staff View
Publication Date: 2018-01-20Publisher: Wiley-BlackwellPrint ISSN: 0148-0227Topics: GeosciencesPhysicsPublished by: -
9O. J. Brambles ; W. Lotko ; B. Zhang ; M. Wiltberger ; J. Lyon ; R. J. Strangeway
American Association for the Advancement of Science (AAAS)
Published 2011Staff ViewPublication Date: 2011-06-04Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
10Kitamura, N., Kitahara, M., Shoji, M., Miyoshi, Y., Hasegawa, H., Nakamura, S., Katoh, Y., Saito, Y., Yokota, S., Gershman, D. J., Vinas, A. F., Giles, B. L., Moore, T. E., Paterson, W. R., Pollock, C. J., Russell, C. T., Strangeway, R. J., Fuselier, S. A., Burch, J. L.
American Association for the Advancement of Science (AAAS)
Published 2018Staff ViewPublication Date: 2018-09-07Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyGeosciencesComputer ScienceMedicineNatural Sciences in GeneralPhysicsKeywords: Geochemistry, Geophysics, Planetary SciencePublished by: -
11Staff View
Publication Date: 2018-12-21Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyGeosciencesComputer ScienceMedicineNatural Sciences in GeneralPhysicsKeywords: Geochemistry, Geophysics, Physics, Planetary SciencePublished by: -
12Zhang, T. L. ; Delva, M. ; Magnes, W. ; Strangeway, R. J. ; Wei, H. Y. ; Russell, C. T.
[s.l.] : Nature Publishing Group
Published 2007Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] The occurrence of lightning in a planetary atmosphere enables chemical processes to take place that would not occur under standard temperatures and pressures. Although much evidence has been reported for lightning on Venus, some searches have been negative and the existence of lightning has ...Type of Medium: Electronic ResourceURL: -
13Staff View
ISSN: 1572-9052Keywords: Time series ; Bayesian approach ; outlier detection ; smoothing ; nonlinear modelingSource: Springer Online Journal Archives 1860-2000Topics: MathematicsNotes: Abstract In the measurements of VLF electric fields with the Pioneer Venus spacecraft in sunlight, spin synchronized signals often dominate over the naturally generated emissions. We present a method to separate natural emissions from the several possible sources of noise. Our major objective by this method is not to remove all spin modulation, but to effectively subtract the background noise caused by the identifiable noise sources. Examination of the data shows that the background spin synchronized noise is quite sensitive to ϑ(n), the angle between the sense axis and the solar direction. We model the observed data asy(n)=w(n)t(n)f(ϑ(n))+x(n), wheref(ϑ) represents the phase response of the background noise andx(n) is the estimated natural emissions.t(n) andw(n) are the long-term trend component and time- and phase-independent component of the intensity of the background noise, respectively. The method to decomposey(n) is based on the Bayesian approach which has been recently applied to various inversion problems such as nonstationary time series modeling and image reconstruction. In this procedure, the estimated parametersw(n),t(n),f(ϑ), andx(n) can be determined automatically. We will describe the Bayesian scheme and its application to the Pioneer Venus VLF electric field data.Type of Medium: Electronic ResourceURL: -
14Staff View
ISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsType of Medium: Electronic ResourceURL: -
15Staff View
ISSN: 1573-093XSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract Solar wind data from the Ames experiment aboard the Pioneer Venus Orbiter, coincident with a period of unprecedented solar activity that began at the end of May, 1991, within the highly active earlier portion of 1991, are summarized and discussed. Some comparison is made with corresponding data from Earth. Some particularly large, strong shocks and solar ejecta were observed at Venus. The solar longitude of Venus, relative to associated flares, varied over a wide range, for a series of flares that produced X-rays that saturated the GOES X-ray counters. Some of the disturbances at Venus must be due to CMEs with longitudinal extents up to ∼40–50 deg.Type of Medium: Electronic ResourceURL: -
16Staff View
ISSN: 1572-9672Source: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract Many significant wave phenomena have been discovered at Venus with the plasma wave instrument flow on the Pioneer Venus Orbiter. It has been shown that whistler-mode waves in the magnetosheath of the planet may be an important source of energy for the topside ionosphere. Plasma waves are also associated with thickening of the ionopause current layer. Current-generated waves in plasma clouds may provide anomalous resistance resulting in electron acceleration, possibly producing aurora. Ion-acoustic waves are observed in the bow shock, and appear to be a feature of the magnetotail boundary. Lastly plasma waves have been cited as evidence for lightning on Venus.Type of Medium: Electronic ResourceURL: