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The results presented are a continuation of observing campaigns conducted bya small group of amateur astronomers interested in the Blazhko effect of RRLyrae stars. The goal of these observations is to confirm the RR Lyrae Blazhkoeffect and to detect any additional Blazhko modulation which cannot beidentified from all sky survey data-mining. The Blazhko effect of the twoobserved stars is confirmed, but no additional Blazhko modulations have beendetected.  The observation of the RR Lyrae star AL Pic during 169 nights was conductedfrom San Pedro de Atacama (Chile). From the observed light curve, 49 pulsationmaxima have been measured. Fourier analyses of (O-C), magnitude at maximumlight (Mmax) and the complete light curve have provided a confirmation ofpublished pulsation and Blazhko periods, 0.548622 and 34.07 days, respectively.The second multi-longitude observation campaign focused on the RR Lyrae star FRPsc was performed from Europe, United States and Chile. Fourier analyses of thelight curve and of 59 measured brightness maxima have improved the accuracy ofpulsation and Blazhko periods which are 0.45568 and 51.31 days, respectively.For both stars, no additional Blazhko modulations have been detected.

AL Pictoris and FR Piscis: two regular Blazhko RR Lyrae stars