✦ LIBER ✦

Studies of solar magnetic fields

✍ Scribed by Robert Howard

Publisher: Springer
Year: 1974
Tongue: English
Weight: 505 KB
Volume: 38
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00161823

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

✍ Robert Howard 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 692 KB

Solar magnetic flux data accumulated from the magnetograph of the Mount Wilson Observatory are used to infer average east-west field inclination angles for the interval 196%1973. In all latitude zones the total flux (IF +] § measurements indicate that the field is inclined so as to trail the rotatio

Studies of solar magnetic fields

✍ Robert Howard 📂 Article 📅 1976 🏛 Springer 🌐 English ⚖ 274 KB

In order to provide a smooth transition to a smaller aperture for the Mount Wilson daily magnetograms, a 2-step change was made, with two daily observations made using two different apertures covering an interval of several months. A comparison of these observations has made possible a check on the

Studies of solar magnetic fields

✍ Robert Howard 📂 Article 📅 1977 🏛 Springer 🌐 English ⚖ 299 KB

An estimate of the average magnetic field strength at the poles of the Sun from Mount Wilson measurements is made by comparing low latitude magnetic measurements in the same regions made near the center of the disk and near the limb. There is still some uncertainty because the orientation angle of t

Numerical studies of azimuthal modulatio

Numerical studies of azimuthal modulations of the solar wind with magnetic fields

✍ Y. Nakagawa; R. E. Wellck 📂 Article 📅 1973 🏛 Springer 🌐 English ⚖ 771 KB

The evolution of azimuthal modulation of the solar wind is examined by numerical integration of the basic equations governing supersonic, super-Alfv6nic, polytropic one fluid flow in the equatorial plane of the Sun with radial as well as azumuthal magnetic fields. The computations are started by int

Zeeman-doppler imaging: A new option for

Zeeman-doppler imaging: A new option for magnetic field study of Ap and solar-type stars

✍ J. F. Donati; M. Semel 📂 Article 📅 1990 🏛 Springer 🌐 English ⚖ 846 KB

In the task of studying stellar magnetic fields, polarimetric methods have been intensively used in Ap stars. But the observational material classically used to reconstruct stellar magnetic structures (average longitudinal magnetic field as a function of rotational phase) is not rich enough in spati

Dynamic behavior of solar wind as reveal

Dynamic behavior of solar wind as revealed by a correlation study of magnetic fields observed at the Venus and Earth orbits

✍ K. Marubashi 📂 Article 📅 1995 🏛 Elsevier Science 🌐 English ⚖ 361 KB