1 00:00:24,370 --> 00:00:21,460 climate scientists have an enormous 2 00:00:28,480 --> 00:00:24,380 challenge which is to understand how or 3 00:00:29,710 --> 00:00:28,490 why climate varies working on Tim and 4 00:00:32,140 --> 00:00:29,720 the glory mission as yet another 5 00:00:34,120 --> 00:00:32,150 dimension to that which is understanding 6 00:00:37,210 --> 00:00:34,130 how the Sun changes and how that affects 7 00:00:39,910 --> 00:00:37,220 climate total solar irradiance is 8 00:00:42,370 --> 00:00:39,920 actually a term that scientists have 9 00:00:44,950 --> 00:00:42,380 begun to use only really in the last 20 10 00:00:48,100 --> 00:00:44,960 years before that it was called the 11 00:00:50,910 --> 00:00:48,110 solar constant so the solar constant is 12 00:00:53,350 --> 00:00:50,920 the integral of all of the energy 13 00:00:56,080 --> 00:00:53,360 radiated by the Sun at all wavelengths 14 00:00:58,960 --> 00:00:56,090 we soon learned that actually this solar 15 00:01:00,760 --> 00:00:58,970 constant varies so therefore we can't 16 00:01:03,700 --> 00:01:00,770 call it the solar constant anymore so we 17 00:01:05,320 --> 00:01:03,710 call it the total solar irradiance which 18 00:01:07,410 --> 00:01:05,330 is really a fancy name for the sun's 19 00:01:10,030 --> 00:01:07,420 brightness 20 00:01:15,050 --> 00:01:13,010 scientists have wondered for hundreds of 21 00:01:17,270 --> 00:01:15,060 years how the sun's radiation changed 22 00:01:20,480 --> 00:01:17,280 there was a series of ground-based 23 00:01:23,510 --> 00:01:20,490 measurements and they couldn't determine 24 00:01:25,670 --> 00:01:23,520 if the changes that they were see were 25 00:01:30,300 --> 00:01:25,680 from the Sun itself or from the 26 00:01:35,069 --> 00:01:32,520 it's important to make measurements of 27 00:01:38,100 --> 00:01:35,079 the solid radiance from space because 28 00:01:40,920 --> 00:01:38,110 it's the only way with a measure the 29 00:01:44,600 --> 00:01:40,930 variability the total irradiance monitor 30 00:01:48,120 --> 00:01:44,610 on glory is at its most basic a 31 00:01:50,340 --> 00:01:48,130 radiometer it looks at the Sun as of 32 00:01:54,060 --> 00:01:50,350 start and measures all that incoming 33 00:01:58,410 --> 00:01:54,070 energy the total irradiance monitor on 34 00:02:02,580 --> 00:01:58,420 glory is state-of-the-art instrument it 35 00:02:04,499 --> 00:02:02,590 has unsurpassed accuracy so that means 36 00:02:06,690 --> 00:02:04,509 we're moving into a new generation of 37 00:02:10,169 --> 00:02:06,700 solar radius measurements with this 38 00:02:12,300 --> 00:02:10,179 higher accuracy and precision we have 39 00:02:14,250 --> 00:02:12,310 recognized that we need to know and 40 00:02:18,240 --> 00:02:14,260 monitor the forces of climate change 41 00:02:22,140 --> 00:02:18,250 over a long period the team measurement 42 00:02:23,970 --> 00:02:22,150 is crucial in continuing this record of 43 00:02:28,020 --> 00:02:23,980 the sun's radiation that we now have 44 00:02:30,479 --> 00:02:28,030 covering almost three solar cycles so 45 00:02:33,080 --> 00:02:30,489 now in a period of what's proving to be 46 00:02:35,550 --> 00:02:33,090 quite a prolonged solar minimum period 47 00:02:37,800 --> 00:02:35,560 the solar minimum period is very 48 00:02:39,960 --> 00:02:37,810 important to measure accurately because 49 00:02:44,160 --> 00:02:39,970 one of the big questions for climate 50 00:02:47,490 --> 00:02:44,170 change is what happens in episodes of 51 00:02:48,960 --> 00:02:47,500 prolonged solar minima the total 52 00:02:52,099 --> 00:02:48,970 irradiance monitor on glory will be 53 00:02:55,020 --> 00:02:52,109 launched at a time to capture this very 54 00:02:56,460 --> 00:02:55,030 uniquely long and low minimum so we're 55 00:02:58,460 --> 00:02:56,470 very excited about what the measurements