Estimates of solar wind velocity gradients between 0.3 and 1 AU based on velocity probability distributions from Helios 1 at perihelion and aphelion

Publisher： John Wiley & Sons Inc

E-ISSN： 2156-2202|96|A8|14183-14187

ISSN： 0148-0227

Source： Journal Of Geophysical Research, Vol.96, Iss.A8, 1991-08, pp. : 14183-14187

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

The relationship between recurring cosmic ray depressions and corotating solar wind streams at ≤1 AU: IMP 8 and Helios 1 and 2 anticoincidence guard rate observations

By  

Journal Of Geophysical Research, Vol. 101, Iss. A6, 1996-06 ,pp. : 13483-13496

John Wiley & Sons Inc

Access to resources Recommend Favorite

The solar wind velocity determined from Voyager 1 and 2: Low‐Energy Charged Particle measurements in the outer heliosphere

By  

Journal Of Geophysical Research, Vol. 103, Iss. A1, 1998-01 ,pp. : 267-276

John Wiley & Sons Inc

Access to resources Recommend Favorite

A 16‐moment solar wind model: From the chromosphere to 1 AU

By  

Journal Of Geophysical Research, Vol. 106, Iss. A5, 2001-05 ,pp. : 8217-8232

John Wiley & Sons Inc

Access to resources Recommend Favorite

Electron velocity distribution functions from the solar wind to the corona

By  

Journal Of Geophysical Research, Vol. 104, Iss. A8, 1999-08 ,pp. : 17021-17032

John Wiley & Sons Inc

Access to resources Recommend Favorite

Solar cycle dependence of the solar wind dynamics: Pioneer Voyager, and Ulysses from 1 to 5 AU

By  

Journal Of Geophysical Research, Vol. 101, Iss. A11, 1996-11 ,pp. : 24359-24371

John Wiley & Sons Inc

Access to resources Recommend Favorite