4 Meteorolagical Observations on Parisnath Hill [No. 1. 



L— Table of\ 





1st April. 



2nd April. 



Time. 



m . Second 

 Temple. Summit. 



Calcutta. 



Time. 



Temple. 



Calcutta. 



h. m. 



Bar. 1 



:her. 



| 

 Bar. 1 



to. 



Bar. 



rher. 



h. m. 



Bar. Ther. 



Bar. 



rher. 



6 



25.963 



21.6 







29.850 



25.7 













„ 30 



7 



25.980 



21.9 





29.875 



260 







22.3 





25.7 



„ 40 



25.999* 22.5* 



25.611 



21.4 



29.892* 



27 .2 + 













8 



26.009* 22.6* 







29.900 



2/.V 













„ 15 



26.016 



22.9 







29.903* 



28.1* 













9 

 „ 30 



26.032 

 26.042 



23.1 



23.8 







29.913 

 29.915* 



29.1 



30.0* 



9 

 „ 15 



25.992 



239 



29.880 



30.1 



10 



26.044 



24.5 







29.918 



30.9 



10 

 „ 15 



26.002 



24.3 



29.877 



31.8 



11 



26.040 



25.8 







29.*902 



32.1 













Noon 



26.021 



27.2 







29.880 



34.0 













1 



26.006 



28.1 







29.842 



34.5 













o 



25.973 



29.1 







29.806 



35.6 













3 



25.951 



28.0 







29 787 



36.1 













4 



„ 40 

 5 



25.928 



27.3* 







29.772 

 29.765* 



36.1 



35.5* 



4 

 „ 55 



25.885 



27.1 



29.716* 



35.6*' 



• • 



9,6 K* 



25.553 



25.4 



29.762 



35.2 



5 



25.884* 



27.0* 



29.715 



35.5 



„ 25 

 6 



25.942 

 25.957 



26.3 

 25.0 







29.762* 

 29.763 



344* 

 33.1 



6 



25.885 



257 



29.716 



33.3| 



7 





24.8* 







29.779 



31.3 













8 



25.964 



# • 



24 6 







29.796 

 • • 



30.0 













Interpolation.— All observations in the table marked with a star, 

 are interpolated. This was done graphically on paper, lithographed 

 for the purpose. A horizontal and a vertical system of straight 

 lines, crossing each other, formed a network of accurately drawn 

 minute squares, each of one millimetre side. By means of this net- 

 work the barometric curve could be designed on any convenient 

 scale, and where the interval of time between two observed points 

 was not greater than one or two hours, a straight line, connecting 



