✦ LIBER ✦

Test for detection of fine structure of the solar wind velocity

✍ Scribed by N. A. Lotova; I. V. Chashey

Publisher: Springer Netherlands
Year: 1973
Tongue: English
Weight: 526 KB
Volume: 20
Category: Article
ISSN: 0004-640X
DOI: 10.1007/bf00645601

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

High coronal structure of high velocity

High coronal structure of high velocity solar wind stream sources

✍ J. T. Nolte; A. S. Krieger; E. C. Roelof; R. E. Gold 📂 Article 📅 1977 🏛 Springer 🌐 English ⚖ 698 KB

Testing for multifractality of the slow

Testing for multifractality of the slow solar wind

✍ Wiesław M. Macek; Roberto Bruno; Giuseppe Consolini 📂 Article 📅 2006 🏛 Elsevier Science 🌐 English ⚖ 372 KB

On the bulk velocity of the solar wind α

On the bulk velocity of the solar wind α-particles

✍ G. Moreno; F. Palmiotto 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 139 KB

On the heliographic latitude dependence

On the heliographic latitude dependence of the solar wind velocity

✍ L. Diodato; G. Moreno 📂 Article 📅 1976 🏛 Springer Netherlands 🌐 English ⚖ 301 KB

Azimuthal structure of the solar wind ve

Azimuthal structure of the solar wind velocity andK-corona brightness in the heliospheric current sheet

✍ B. Bala; S. R. Prabhakaran Nayar 📂 Article 📅 1993 🏛 Springer 🌐 English ⚖ 476 KB

A comment on the detection of closed mag

A comment on the detection of closed magnetic structures in the solar wind

✍ J. T. Gosling; E. C. Roelof 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 221 KB

It has recently been suggested that the large scale structure of the interplanetary magnetic field can be deduced solely from solar wind speed measurements. Here it is emphasized that, in addition to speed measurements, direct measurements of the interplanetary field and indirect diagnostics such as