Far infrared measurement of the solar minimum temperature

Solar Physics ◽  
1969 ◽  
Vol 10 (2) ◽  
pp. 330-341 ◽  
Author(s):  
John A. Eddy ◽  
Pierre J. L�na ◽  
Robert M. MacQueen
1987 ◽  
Vol 35 (10) ◽  
pp. 5334-5336 ◽  
Author(s):  
Z. Schlesinger ◽  
R. L. Greene ◽  
J. G. Bednorz ◽  
K. A. Müller

2017 ◽  
Vol 4 (1) ◽  
pp. 67
Author(s):  
Arjun Kumar Gautam ◽  
Binil Aryal

<p class="Default">We have studied about the evolution of Asymptotic Giant Branch (AGB) stars, mass losses from them and a systematic search of AGB stars in J2000 coordinate system provided by K. W. Shu &amp; Y. J. Kwon (2011) of dust structure in the far infrared range (100 μm and 60 μm). For dust structure IRAS survey was performed using Sky View virtual Observatory. The FITS images downloaded from sky view was processed using software Aladin v 2.5. A cavity like structure (major diameter∼1.93 pc &amp; minor diameter∼ 0.89 pc) lies in the coordinate of R. A. (J2000) 04h 15m 03s and DEC (J2000) 54d 41m 00s was found at the distance∼ 240 pc. We studied the flux density variation and the temperature variation about major diameter, minor diameter and the distance between minimum temperature and minimum flux within the structure. We observed the variation of the temperature is 20.53 K to 21.09 K, with the offset of about 0.56 K, which show the cavity is independently evolved. The mass profile of each pixel of the structure was also calculated using this temperature.</p><p><strong>Journal of Nepal Physical Society</strong><em><br /></em>Volume 4, Issue 1, February 2017, Page: 67-77</p>


2017 ◽  
pp. 48-53
Author(s):  
Arjun Kumar Gautam

A systematic search in the range of J2000 coordinate system provided by K.W. Shu & Y.J. Kwon (2011) of dust structure in the far infrared (100 μm and 60 μm) IRAS (Infrared Astronomical Satellite) survey was performed using Sky View virtual Observatory (1) so that some interesting isolated cavity structures surrounding the cavity structure were expected. The FITS images downloaded from sky view (1) was processed using software Aladin v 2.5. A cavity like structure (major diameter ∼ 3.57 pc & minor diameter ∼ 1.19 pc) lies in the coordinate of R.A. (J2000) 06h 31m 05s and DEC (J2000) 16d 06m 00s was found at the distance ∼ 310 pc (5). We studied the flux density variation and the temperature variation about major diameter, minor diameter and the distance between minimum temperature and minimum flux within the structure. We observed the variation of the temperature is 20.53 K to 21.42 K, with the offset of about 0.89 K, which shows the cavity is independently evolved. The mass profile of each pixel of the structure was also calculated using these temperature.The Himalayan Physics Vol. 6 & 7, April 2017 (48-53)


2010 ◽  
Vol 93 (11) ◽  
pp. 3782-3787 ◽  
Author(s):  
Chun-Hai Wang ◽  
Guang-Hua Liu ◽  
Xi-Ping Jing ◽  
Guang-Shan Tian ◽  
Xiang Lu ◽  
...  

1980 ◽  
Vol 7 (9) ◽  
pp. 704-706 ◽  
Author(s):  
K. V. Chance ◽  
J. C. Brasunas ◽  
W. A. Traub

1973 ◽  
Vol 8 (5) ◽  
pp. 1978-1981 ◽  
Author(s):  
D. B. Tanner ◽  
A. J. Sievers

1987 ◽  
Vol 35 (16) ◽  
pp. 8829-8832 ◽  
Author(s):  
P. E. Sulewski ◽  
A. J. Sievers ◽  
R. A. Buhrman ◽  
J. M. Tarascon ◽  
L. H. Greene ◽  
...  

1985 ◽  
Vol 116 (1) ◽  
pp. 165-172 ◽  
Author(s):  
C. Macris ◽  
B. Petropoulos

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