✦ LIBER ✦

Associating the Solar Wind Measured by Ulysses with its Source at the sun

✍ Scribed by Richard Woo; Shadia Rifai Habbal

Book ID: 110304524
Publisher: Springer Netherlands
Year: 2001
Tongue: English
Weight: 52 KB
Volume: 97
Category: Article
ISSN: 0038-6308
DOI: 10.1023/a:1011822010421

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Solar wind velocity measurements near th

Solar wind velocity measurements near the sun using Ulysses radio amplitude correlations at two frequencies

✍ A.I. Efimov; M.K. Bird; V.K. Rudash; V.E. Andreev; I.V. Chashei; D. Plettemeier; 📂 Article 📅 2005 🏛 Elsevier Science 🌐 English ⚖ 274 KB

Sulfur abundances in the solar wind meas

Sulfur abundances in the solar wind measured by SWICS on Ulysses

✍ C.M. Shafer; G. Gloeckler; A.B. Galvin; F.M. Ipavich; J. Geiss; R. von Steiger; 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 361 KB

Solar wind composition measurements by t

Solar wind composition measurements by the Ulysses SWICS experiment during transient solar wind flows

✍ A.B. Galvin; G. Gloeckler; F.M. Ipavich; C.M. Shafer; J. Geiss; K. Ogilvie 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 356 KB

Solar wind charge states measured by ULY

Solar wind charge states measured by ULYSSES/SWICS in the south polar hole

✍ A. B. Galvin; F. M. Ipavich; C. M. S. Cohen; G. Gloeckler; R. Steiger 📂 Article 📅 1995 🏛 Springer Netherlands 🌐 English ⚖ 356 KB

Observation of the multifractal spectrum

Observation of the multifractal spectrum in solar wind turbulence by Ulysses at high latitudes

✍ Wawrzaszek, Anna; Macek, Wieslaw M. 📂 Article 📅 2010 🏛 American Geophysical Union 🌐 English ⚖ 468 KB

Relationships of quasi-stationary solar

Relationships of quasi-stationary solar wind flows with their sources on the Sun

✍ V. G. Eselevich 📂 Article 📅 1992 🏛 Springer 🌐 English ⚖ 1000 KB

In this paper, by considering an example of four Carrington rotations ( 167 l, 1672, 1681, and 1682), it is shown that there generally exists an exhaustive correspondence between quasi-stationary flows of'fast' and 'slow' solar wind (SW), on the one hand, and their sources on the Sun: coronal holes