86 



Term-Day Observations of Magnetometers, 1844. 



Gottingen 

 Mean time 



of 



Declination 

 Observation 



October 23, 24. 





 5 



10 

 15 

 20 

 25 

 30 

 35 

 40 

 45 

 50 

 55 





 5 

 10 

 15 

 20 

 25 

 30 

 35 

 40 

 45 

 50 

 55 





 5 



10 

 15 

 20 

 25 

 30 

 35 

 40 

 45 

 50 

 55 





 5 

 10 

 15 

 20 

 25 

 30 

 35 

 40 

 45 

 50 

 55 



Declina- 

 tion. 



25 



25 



25 



25 



Bifilar Balance 

 Corrected. Corrected. 



13-52 

 13-69 

 13-67 

 13-57 

 13-72 

 13-43 

 13-67 

 13-52 

 13-66 

 13-69 

 14-20 

 14-40 



14-33 

 13-99 

 13-79 

 14-20 

 13-50 

 13-27 

 13-96 

 13-91 

 13-22 

 13-69 

 13-64 

 12-96 



13-69 

 13-79 

 13-83 

 13-67 

 13-46 

 13-56 

 13-76 

 14-11 

 14-08 

 14-17 

 14-20 



Sc. Div 



18 h . 



5331 



599- 



533-3 



600- 



533-0 



600- 



533-6 



600- 



533-3 



601- 



532-6 



602- 



532-1 



603- 



531-8 



603- 



532-5 



604- 



532-7 



603- 



531-9 



605- 



529-7 



606- 



19 h . 



21 h . 

 527-0 

 527-0 

 526-5 

 525-2 

 525-2 

 525-2 

 525-5 

 524-3 

 5240 

 522-7 

 522-2 

 522-1 



528-6 



607-0 



528-7 



607-5 



529-2 



607-5 



527-9 



609-5 



528-8 



607-2 



530-9 



607-5 



529-8 



607-2 



529-7 



605-3 



531-6 



604-8 



530-4 



605-9 



528-2 



606-1 



528-6 



605-6 



20 h . 





•12 



530-6 



•63 



530-6 



•14 



530-6 



•76 



530-3 



•39 



530-7 



• 20 



528-9 



25 



528-4 



•14 



529-7 



•69 



530-4 



• 13 



529-6 



•97 



528-4 



•76 



527-4 



605-5 

 606-1 

 606-6 

 606-6 

 606-3 

 607-0 

 607-0 

 606-5 

 606-1 

 606-3 

 607-1 

 607-0 



607-4 

 607-7 

 607-7 

 609-4 

 608-9 

 6091 

 509-3 

 609-2 

 609-0 

 610-1 

 611-0 

 610-7 



Declina- 

 tion. 



Bifilar 



Corrected. 



Balance 

 Corrected 



25 



25 





22 h . 



14-41 



521-5 



14-53 



521-0 



14-60 



520-9 



14-80 



520-9 



15-25 



520-9 



15-47 



520-9 



15-54 



520-3 



15-62 



520-6 



15-96 



520-5 



16-03 



520-5 



16-41 



520-9 



16-59 



521-0 



17-09 

 17-39 

 17-42 

 17-73 

 18-23 

 18-27 

 18-52 

 18-63 

 18-84 

 18-90 

 1914 

 19-39 



25 



25 



23 h . 

 521-4 

 521-4 

 520-8 

 521-4 

 521-2 

 520-9 

 521-5 

 521-6 

 521-7 

 522-3 

 5231 

 522-3 





h . 



19-82 



525-2 



20-40 



5250 



20-87 



524-3 



20-67 



5240 



20-89 



525-3 



21-27 



524-9 





525-9 

 525-3 



21-07 



20-58 



525-3 



2106 



5250 



20-45 



525-3 



20-29 



524-5 





l h . 



20-40 



524-2 



2015 



524-1 



20-16 



523-6 



19-75 



523-0 



19-79 



522-5 



19-41 



521-8 



19-56 



523-3 



19-86 



524-5 



19-56 



523-6 



19-78 



524-5 



19-98 



524-5 



19-73 



525-9 



6110 

 611-6 

 611-2 

 611-4 



610-9 



610-1 



611-1 

 611-5 



612-1 

 612-1 

 611-7 

 611-0 

 610-5 



610-5 



609-8 

 610-9 

 613-2 



615-9 

 616-9 

 616-5 



619-8 



620-0 

 621-2 



623-4 

 6250 



Declina- 

 tion. 



Bifilar 

 Corrected. 



25 



25 



25 



25 



1502 

 14-78 

 14-55 

 14-24 

 14-20 

 1415 

 14-04 

 13-81 

 13-69 

 13-47 

 13-76 

 13-76 



Sc. Div. 



5 h . 



Balance 



Corrected, 





2 h . 



19-91 



526-8 



20-02 



528-1 



19-95 



527-8 



19-88 



528-2 



19-51 



527-8 



19-62 



527-7 



19-55 



527-6 



19-42 



528-2 



19-48 



529-2 



19-41 



529-9 



19-44 



529-7 



19-55 



528-5 



Mic. Div. 



625-2 



630-2 



631-3 





3\ 



19-26 



528-2 



1910 



528-2 



18-77 



527-6 



18-10 



527-4 



18-05 



527-8 



17-76 



528-1 



17-34 



527-9 



17-36 



529-2 



17-07 



529-5 



16-57 



530-4 



16-48 



531-8 



16-45 



532-4 





4 h . 



16-30 



532-9 



16-23 



5331 



16-21 



533-2 



16-10 



533-5 



1610 



533-5 



1601 



533-7 



15-76 



533-8 



15-39 



533-7 



15-24 



534-2 



15-27 



535-2 



15-14 



534-6 



15-04 



534-3 



534-9 



622- 



535-2 



622- 



5350 



622- 



534-9 



622- 



535-2 



622- 



535-3 



621- 



535-1 



620- 



535-4 



621- 



535-5 



620-. 



535-6 



620-, 



535-3 



620-: 



5350 



619- 



633-9 



634- 1 

 6320 



632-4 

 630-9 

 631-8 

 631-3 

 629-9 

 629-8 



629-6 



629-1 

 628-9 

 628-3 

 6270 

 626-5 

 625-8 

 6260 

 625-0 

 624-5 

 623-8 



Declina- 

 tion. 



Bifilar 

 Corrected 



25 13 

 13 

 13 

 13 

 13 

 14 

 14 

 14 

 14 

 13 

 13 

 13 



25 



25 



13-88 

 13-88 

 13-96 

 13-99 

 13-93 

 13-86 

 13-84 

 13-83 

 13-86 

 13-79 

 13-81 

 13-84 



25 



Sc. Div. 



6\ 



•74 



534-8 



•94 



534-2 



•90 



534-2 



•97 



533-9 



•93 



534-3 



•17 



534-3 



•13 



534-2 



•13 



534-6 



•10 



534-2 



•96 



534-8 



•99 



534-7 



■83 



534-7 



7 h . 



534-8 



535-0 



535-4 



535-3 



535-1 



5351 



535-2 



535-4 



535-5 



535-2 



5351 



535-2 





8\ 



13-72 



535-3 



13-72 



535-1 



13-76 



535-0 



13-72 



5350 



13-69 



5350 



13-66 



535-1 



13-59 



535-2 



13-61 



5350 



13-57 



534-9 



13-57 



534-9 



13-56 



534-5 



13-50 



534-3 





9 h . 



13-47 



534-4 



13-52 



534-6 



13-48 



534-6 



13-47 



534-9 



13-49 



5351 



13-56 



534-7 



13-56 



534-7 



13-56 



534-5 



13-54 



534-5 



13-52 



5341 



13-59 



534-1 



13-49 



533-5 



Bifilar. Observed 2™ after the Declination, £=0-000140. 



Balance. Observed 3™ after the Declination, £=0-0000085. 



The temperature of the bifilar and balance magnets, and the observers' initials, will be found at the corresponding hours in the Hourly 

 Observations of Magnetometers. 



When double commas („) occur in the column for the balance magnetometer, the needle was examined, and no change from the previous 

 observation being appreciable, the micrometers were not altered. 



