बिमोडल इसके अंग्रेजी अर्थ का उदाहरण

Analysis gave a well-defined, classically shaped bimodal lightcurve with a rotation period of () hours and a high brightness variation of magnitude ().

Analysis gave a classically shaped bimodal lightcurve with a well-defined rotation period of () hours and a high brightness variation of () magnitude, indicative of its elongated shape ().

Analysis gave a classically shaped, well-defined bimodal lightcurve with a rotation period of hours and a very high brightness variation of magnitude, indicative of an highly elongated shape ().

Analysis gave a bimodal lightcurve with a rotation period of hours and a brightness variation of magnitude ().

Analysis of the classically shaped bimodal lightcurve gave a well-defined rotation period of hours with a brightness variation of magnitude ().

Based on observations taken on September 2004, Brian Warner at his Palmer Divide Observatory , Colorado, published an ambiguous period of and hours with an amplitude of and magnitude, respectively, depending on whether the period solution is derived from a monomodal or from a bimodal lightcurve ().

Analysis gave a classically shaped bimodal lightcurve with a well-defined rotation period of hours and a brightness variation of magnitude ().

Analysis gave a classically shaped bimodal lightcurve with a rotation period of hours and a brightness variation of magnitude ().

Analysis gave a bimodal lightcurve with an exceptionally long rotation period of hours and a brightness amplitude of magnitude ().

Analysis of the classical bimodal lightcurve gave a rotation period of hours with a high brightness amplitude of magnitude, indicative of an irregular, non-spherical shape () .

In July 2014, a rather asymmetric bimodal lightcurve, obtained by a collaboration between American astronomers Frederick Pilcher and Andrea Ferrero, gave a more refine rotation period of 10.

Contrary to the common bimodal shape, the lightcurve for Wallia shows three minima and three maxima.