Nomogram for sunspot numbers.

Details Nomogram for sunspot numbers. Nomogram for sunspot numbers.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ijrsp..26..346u&link_type=abstract

Indian J. Radio Space Phys., Vol. 26, No. 6, p. 346 - 353

Physics

Sunspot Numbers

Scientific paper

Nomogram construction using the parabolic relationship f0F2 = a0+a1R12+a2R122 between monthly median f0F2 and running average sunspot number (RASSN) R12 values has been described; here a0, a1 and a2 are the best fit coefficients. The nomogram can give the required local effective sunspot number (LESSN) values corresponding to any observed value of f0F2. Transforming the f0F2-RASSN relation to the form R122+pR12+q = 0 [where p = a1/a2 and q = (a0-f0F2)/a2], a practical method for the preparation of a single nomogram for f0F2-RASSN has been described and the problem of very high and very low values of the variables has also been dealt with successfully. A single nomogram for a large range of variables, namely, f0F2, a0, a1, and a2 has been obtained so that one can easily find LESSN values at any location, season, and time. The nomogram tends to minimize the errors in LESSN calculations at all levels of solar activity.

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