<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD JATS (Z39.96) Journal Publishing DTD v1.2d1 20170631//EN" "JATS-journalpublishing1.dtd">
<article xlink="http://www.w3.org/1999/xlink" dtd-version="1.0" article-type="general-sciences" lang="en"><front><journal-meta><journal-id journal-id-type="publisher">IJCRR</journal-id><journal-id journal-id-type="nlm-ta">I Journ Cur Res Re</journal-id><journal-title-group><journal-title>International Journal of Current Research and Review</journal-title><abbrev-journal-title abbrev-type="pubmed">I Journ Cur Res Re</abbrev-journal-title></journal-title-group><issn pub-type="ppub">2231-2196</issn><issn pub-type="opub">0975-5241</issn><publisher><publisher-name>Radiance Research Academy</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">2045</article-id><article-id pub-id-type="doi"/><article-id pub-id-type="doi-url"/><article-categories><subj-group subj-group-type="heading"><subject>General Sciences</subject></subj-group></article-categories><title-group><article-title>SOLAR CONSTANT, SUNSPOTS AND SOLAR ACTIVITY&#13;
</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>.Sumathi</surname><given-names>R</given-names></name></contrib><contrib contrib-type="author"><name><surname>Selvaraj</surname><given-names>R. Samuel</given-names></name></contrib></contrib-group><volume>)</volume><issue/><fpage>36</fpage><lpage>40</lpage><permissions><copyright-statement>This article is copyright of Popeye Publishing, 2009</copyright-statement><copyright-year>2009</copyright-year><license license-type="open-access" href="http://creativecommons.org/licenses/by/4.0/"><license-p>This is an open-access article distributed under the terms of the Creative Commons Attribution (CC BY 4.0) Licence. You may share and adapt the material, but must give appropriate credit to the source, provide a link to the licence, and indicate if changes were made.</license-p></license></permissions><abstract><p>This paper deals with study of sunspot numbers and solar energy since 1755.&#13;
Number of sunspots and solar energy varies for each solar cycle. The duration of solar cycle is&#13;
from 9 to 11 years. It varies every time. Solar cycle is the time interval from a sunspot minimum&#13;
to the next sunspot minimum.&#13;
</p></abstract><kwd-group><kwd>Solar Constant</kwd><kwd> Sunspot Number and Solar activity</kwd></kwd-group></article-meta></front></article>
