|
Detailed Reference Information |
Cummings, A.C., Stone, E.C. and Webber, W.R. (1993). Estimate of the distance to the solar wind termination shock from gradients of anomalous cosmic ray oxygen. Journal of Geophysical Research 98: doi: 10.1029/93JA01173. issn: 0148-0227. |
|
The radial gradient of anomalous cosmic ray oxygen measured instantaneously between Voyager 2 and Pioneer 10 during 1985--1988 is correlated with the inferred tilt of the heliospheric neutral sheet. This is consistent with a simple model in which the radial gradient is related to the length of the neutral sheet between the two spacecraft. With this model we show that the radial gradient and the tilt of the neutral sheet near the solar wind termination shock can be inferred rom the Voyager and Pioneer observations. By comparing the time history of the inferred tilt with that derived from solar observations, we estimate that the termination shock was at 62+5-7 AU at solar minimum in 1987. At solar maximum the shock should be located at ~90 AU due to the increased pressure of the solar wind. ¿ American Geophysical Union 1993 |
|
|
|
BACKGROUND DATA FILES |
|
|
Abstract |
|
|
|
|
|
Keywords
Interplanetary Physics, Cosmic rays, Interplanetary Physics, Heliopause and solar wind termination, Interplanetary Physics, Interstellar gas, Interplanetary Physics, Solar wind plasma |
|
Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
|
|
|