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- ...module reached their working temperatures (approximately 50 K on the third V-groove, and 40 K on the reflectors) by passive cooling. This was achieved during t50 KB (7,826 words) - 22:29, 4 February 2015
- 6 KB (921 words) - 17:19, 3 September 2013
- 72 KB (10,038 words) - 08:40, 24 October 2016
- 28 KB (4,415 words) - 18:43, 21 August 2015
- ...ISO, Spitzer, AKARI), could not. Radiative cooling is provided by three [[V-groove]] radiators and a large [[telescope baffle]]. The active coolers are a [[so42 KB (7,697 words) - 16:43, 4 October 2012
- ...provides stray-light shielding and radiative cooling; and three conical “V-groove” baffles that provide thermal and radiative insulation between the warm s ...E, ISO, Spitzer, AKARI), could not. Radiative cooling is provided by three V-groove radiators and a large telescope baffle. The active coolers are a [[LFI_desi14 KB (2,170 words) - 09:29, 21 May 2014
- 34 KB (5,468 words) - 15:34, 4 February 2015
- 14 KB (2,299 words) - 20:58, 17 March 2013
- 24 KB (3,748 words) - 10:02, 26 September 2016
- 6 KB (827 words) - 14:33, 15 April 2015
- 173 KB (25,381 words) - 15:29, 4 June 2014
- 14 KB (2,155 words) - 23:49, 12 November 2014
- 39 KB (5,438 words) - 09:40, 20 May 2014
- 60 KB (9,314 words) - 08:48, 2 January 2015
- 22 KB (2,713 words) - 18:48, 1 March 2013
- 3 KB (487 words) - 17:09, 4 February 2015
- 90 KB (13,248 words) - 13:06, 21 April 2020
- ...provides stray-light shielding and radiative cooling; and three conical “V-groove” baffles that provide thermal and radiative insulation between the warm s ...zer, Akari), could not. Radiative cooling for Planck was provided by three V-groove radiators and a large telescope baffle. The active coolers were a [[LFI_des14 KB (2,136 words) - 09:37, 3 February 2015
- 35 KB (5,146 words) - 17:59, 3 July 2014
- 13 KB (2,128 words) - 15:29, 4 June 2014