The very long lived M-Regions near the Sunspot Minimum of 1933

Authors

  • ALI M NAQVI
  • J. N. TANDON

DOI:

https://doi.org/10.54302/mausam.v6i3.4482

Abstract

The geomagnetic activity during the years 1930-34 has been analysed, and the earlier conclusions of Naqviand Bhargava for the geomagnetic activity during 1950-53 are confirmed, Three very long sequences of the recurrent type of geomagnetic activity designated as A; B and C have been found.

The difference in the heliographic longitudes of the M -regions responsible for the A and the B sequences is about 1800, for the B and C sequences about 45°, and for the C and the A sequences about 135°, Their respective heliographic latitudes are; above 7°.2 north, below 7°,2 south, and about 4°"8 south respectively.

 

 

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Published

1955-07-01

Issue

Vol. 6 No. 3 (1955): MAUSAM

Section

Shorter Contribution

Categories

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How to Cite

[1]
“The very long lived M-Regions near the Sunspot Minimum of 1933”, MAUSAM, vol. 6, no. 3, pp. 251–253, Jul. 1955, doi: 10.54302/mausam.v6i3.4482.