Zobrazeno 1 - 6 of 6 pro vyhledávání: '"H. V. Argo"'
1
Observations of solar wind plasma changes across the bow shock
Autor: A. J. Hundhausen, I. B. Strong, H. V. Argo, S. J. Bame, J. R. Asbridge
Publikováno v: Journal of Geophysical Research. 72:1989-1994
The Vela 3 satellites are in nearly circular orbits tilted at 60° to the ecliptic plane at geocentric distances of approximately 18.5 RE (earth radii). Thus the solar wind plasma can be sampled on both sides of the ‘bow shock,’ on both the dawn
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::2fb67d94542973ebd4f60259e7135f62
https://doi.org/10.1029/jz072i007p01989
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2
Absorption ofμ−Mesons inC12
Autor: H. V. Argo, A. D. McGuire, F. B. Harrison, H. W. Kruse
Publikováno v: Physical Review. 114:626-633
It is known that there is a strong similarity between the electron- nucleon and electron-muon weak interactions. This paper is a repont on an experimental investigation of the third leg of the triangle, the muon-nucleon interaction. The absorption of
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::5a64c1ab9454de05aa62a158792f810f
https://doi.org/10.1103/physrev.114.626
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4
16?40 � coronal X-ray emission during the 12 November 1966 eclipse
Autor: S. Singer, J. A. Bergey, W. D. Evans, H. V. Argo
Publikováno v: Solar Physics. 5:551-563
The solar eclipse of 12 November 1966 was used to study the coronal emission near the limbs in selected emission lines between 16 and 40 A. Eight fixed-wavelength, curved crystal spectrometers were carried in each of 3 rocket launches to an altitude
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::a6a0afea81d9eb98e85effc601a47270
https://doi.org/10.1007/bf00147020
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