✦ LIBER ✦

Distribution of sunspots 1874–1976

✍ Scribed by B. D. Yallop; C. Y. Hohenkerk

Book ID: 104647347
Publisher: Springer
Year: 1980
Tongue: English
Weight: 128 KB
Volume: 68
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00156868

No coin nor oath required. For personal study only.

✦ Synopsis

A diagram of the distribution in latitude of sunspot groups during the period 1874-1976 is given. As an indication of sunspot activity, a diagram of the mean total daily sunspot areas for each synodic rotation is also given.

📜 SIMILAR VOLUMES

Decay rates of sunspot groups from 1874

Decay rates of sunspot groups from 1874 to 1976

✍ V. Martinez Pillet; F. Moreno-Insertis; M. Vázquez 📂 Article 📅 1990 🏛 Springer Netherlands 🌐 English ⚖ 242 KB

Vortical distribution of sunspots

✍ S.-I. Akasofu 📂 Article 📅 1985 🏛 Elsevier Science 🌐 English ⚖ 316 KB

Sunspots and Pressure Distribution.

✍ DEELEY, R. M. 📂 Article 📅 1930 🏛 Nature Publishing Group 🌐 English ⚖ 134 KB

Periodicities in the longitude distribut

Periodicities in the longitude distribution of sunspots

✍ W. Stanek 📂 Article 📅 1972 🏛 Springer 🌐 English ⚖ 734 KB

It is well known to the observer of sunspots that the spots seem not to be randomly distributed on the solar surface but rather occur at an increased rate at distances of 180 ~ of each other on the same hemisphere while northern and southern hemispheres are independent. The following investigation

The distribution of sunspots over the Su

The distribution of sunspots over the Sun

✍ Wahab Uddin; M. C. Pande; V. K. Verma 📂 Article 📅 1991 🏛 Springer Netherlands 🌐 English ⚖ 310 KB

Distribution of sunspots according to th

Distribution of sunspots according to their magnetic fluxes

✍ T. K. Das; M. K. Das Gupta 📂 Article 📅 1982 🏛 Springer 🌐 English ⚖ 130 KB

The occurrence frequency distribution of sunspots in different magnetic flux values has been examined. The number of sunspots decreases as ~b -19 for sunspots with magnetic flux greater than 3 x 102a Maxwell, where q~ is the said flux of a sunspot.