Author:
White S. M.,Iwai K.,Phillips N. M.,Hills R. E.,Hirota A.,Yagoubov P.,Siringo G.,Shimojo M.,Bastian T. S.,Hales A. S.,Sawada T.,Asayama S.,Sugimoto M.,Marson R. G.,Kawasaki W.,Muller E.,Nakazato T.,Sugimoto K.,Brajša R.,Skokić I.,Bárta M.,Kim S.,Remijan A. J.,de Gregorio I.,Corder S. A.,Hudson H. S.,Loukitcheva M.,Chen B.,De Pontieu B.,Fleishmann G. D.,Gary D. E.,Kobelski A.,Wedemeyer S.,Yan Y.
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference60 articles.
1. Bastian, T.S., Ewell, M.W., Zirin, H.: 1993, The center-to-limb brightness variation of the sun at
lambda
=
850
microns
$\mbox{lambda} = 850~\mbox{microns}$
. Astrophys. J.
415, 364.
DOI
.
ADS
.
2. Brajša, R., Benz, A.O., Temmer, M., Jurdana-Šepić, R., Šaina, B., Wöhl, H.: 2007, An interpretation of the coronal holes’ visibility in the millimeter wavelength range. Solar Phys.
245, 167.
DOI
.
ADS
.
3. Brogan, C.L., Hunter, T.R.: 2014, ALMA Single-Dish Imaging Parameters. NAASC Memo 114 (draft).
4. Broguière, D., Lucas, R., Pardo, J., Roche, J.-C.: 2011, TELCAL: The on-line calibration software for ALMA. In: Evans, I.N., Accomazzi, A., Mink, D.J., Rots, A.H. (eds.) Astronomical Data Analysis Software and Systems XX
CS-442, Astron. Soc. Pacific, San Francisco, 277.
ADS
.
5. Buhl, D., Tlamicha, A.: 1970, The mapping of the Sun at 3.5 MM. Astron. Astrophys.
5, 102.
ADS
.