✦ LIBER ✦

The Hale solar sector boundary

✍ Scribed by Leif Svalgaard; John M. Wilcox

Publisher: Springer
Year: 1976
Tongue: English
Weight: 495 KB
Volume: 49
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00221492

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

On the cause of observed solar wind velo

On the cause of observed solar wind velocity variation around hale type sector boundary

✍ T.E. Girish; S.R. Prabhakaran Nayar 📂 Article 📅 1986 🏛 Elsevier Science 🌐 English ⚖ 232 KB

Geomagnetic activity and Hale sector bou

Geomagnetic activity and Hale sector boundaries

✍ H. Lundstedt; P.H. Scherrer; J.M. Wilcox 📂 Article 📅 1981 🏛 Elsevier Science 🌐 English ⚖ 459 KB

On the cause of geomagnetic activity at

On the cause of geomagnetic activity at Hale sector boundary

✍ S.R.Prabhakaran Nayar; P. Revathy 📂 Article 📅 1982 🏛 Elsevier Science 🌐 English ⚖ 258 KB

The relationship between solar flares an

The relationship between solar flares and solar sector boundaries

✍ Phil H. Dittmer 📂 Article 📅 1975 🏛 Springer 🌐 English ⚖ 310 KB

A superposed epoch analysis of [1964][1965][1966][1967][1968][1969][1970] solar flares shows a marked increase in flare occurrence within a day (13 ~ of longitude) of (-- § solar sector boundaries as well as a local minimum in flare occurrence near (+ --)sector boundaries. This preference for (--+)b

Coronal magnetic structure at a solar se

Coronal magnetic structure at a solar sector boundary

✍ John M. Wilcox; Leif Svalgaard 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 660 KB

Solar radio emission at 9.1 cm and secto

Solar radio emission at 9.1 cm and sector boundaries

✍ W. Graf; R. N. Bracewell 📂 Article 📅 1975 🏛 Springer 🌐 English ⚖ 485 KB

A possible connection between solar radio emission from 1.0 to 9.4 GHz and the interplanetary sector boundaries has been previously reported in the literature. The present research does not support the previous work as expected. The 9.1 cm activity appears to be organized around sector boundaries on