1 00:00:04,770 --> 00:00:10,019 our solar observatory in space, pointing an array of telescopes into an 2 00:00:10,019 --> 00:00:14,560 environment free of weather conditions and the screening effects of the atmosphere. 3 00:00:14,560 --> 00:00:15,060 Telescopes able to observe several solar features concurrently, such as Sun spots 4 00:00:20,920 --> 00:00:26,880 appearing as relatively cool dark areas on the Sun's disc. their magnetic intensity 5 00:00:26,880 --> 00:00:32,099 is are 10,000 times greater than that of the earth and often associated with 6 00:00:32,099 --> 00:00:37,860 energetic activity the most remarkable fact about sunspot is if you remember an 7 00:00:37,860 --> 00:00:44,940 area are not constant but vary at an 11-year cycle solar flares short-lived 8 00:00:44,940 --> 00:00:49,320 with vigorous burst of light accompanied by intense radiation in the x-ray 9 00:00:49,320 --> 00:00:54,720 ultraviolet and radio parts of the spectrum a large flare releases the 10 00:00:54,720 --> 00:01:00,119 amount of energy a city of three million with used in fifty million year. Flares 11 00:01:00,119 --> 00:01:07,710 usually appear on the white areas bordering sunspots for a more rarefied 12 00:01:07,710 --> 00:01:13,590 gases in the Sun's corona or outer atmosphere. solar black spots 13 00:01:13,590 --> 00:01:18,010 seen an x-ray photos scattered all over the face of the Sun. 14 00:01:18,010 --> 00:01:23,840 prominences - masses of cool, illuminus gas and danced on the corona or shut up out 15 00:01:23,840 --> 00:01:30,350 of the Solar surface has a long magnetic lines go over print wait for turning outward 16 00:01:30,350 --> 00:01:34,700 enormous amount of material hundreds of thousands of tons of weight of the Sun's 17 00:01:34,700 --> 00:01:39,890 outer atmosphere at speeds of up to two million kilometers per hour, reshaping 18 00:01:39,890 --> 00:01:45,860 magnetic field and structural features in large parts of the coronas. Thus from Skylab the light of the is dim. 19 00:01:45,860 --> 00:01:50,649 itself Skylab scientists created the equivalent of thousands of brief 20 00:01:50,649 --> 00:01:56,509 Earth observations or a solar eclipse to study the Sun's corona. Before, it was assumed 21 00:01:56,509 --> 00:02:01,670 this outer atmosphere was fairly stable that changes occur only slowly over long 22 00:02:01,670 --> 00:02:06,920 periods of time but Skylab revealed a much more dynamic corona with many 23 00:02:06,920 --> 00:02:11,980 more changes occurring at faster rates than was thought possible. Including this huge bubble 24 00:02:11,980 --> 00:02:16,880 righted by a magnetic field extending into the outer atmosphere rapidly 25 00:02:16,880 --> 00:02:23,870 growing almost the size of Sun itself. another telescope scanned selected 26 00:02:23,870 --> 00:02:28,459 portions of the Sun recording extreme ultraviolet light from several layers of 27 00:02:28,459 --> 00:02:33,260 atmosphere these layers lying above the visible surface of the Sun the 28 00:02:33,260 --> 00:02:36,350 chromosphere the chromosphere Corona transition zone 29 00:02:36,350 --> 00:02:40,300 and the corona were scanned simultaneously 30 00:02:40,300 --> 00:02:45,160 and a display here using various computer generated color. In this sequence of 31 00:02:45,160 --> 00:02:50,970 ultraviolet photographs, a third is shot out of the chromosphere and into the corona 32 00:02:50,970 --> 00:02:56,350 by means image timed sequences, the flow of energy upward into the corona can 33 00:02:56,350 --> 00:03:01,450 be measured and balanced against the downward flow allowing for the first time an 34 00:03:01,450 --> 00:03:07,810 accurate assessment of a dynamics of the solar atmosphere. For the first time, Skylab 35 00:03:07,810 --> 00:03:12,160 astronauts were able to take the detailed data of a whole Sun and the ultraviolet 36 00:03:12,160 --> 00:03:17,470 region of the spectrum. this picture shows the areas of the sun's atmosphere which are 37 00:03:17,470 --> 00:03:22,960 between 50,000 and 100,000 degrees Kelvin at the time of an eruption that lifted 38 00:03:22,960 --> 00:03:27,730 this twisted sheet of flame off its surface. The eruption is one of the 39 00:03:27,730 --> 00:03:32,410 largest ever recorded and it grown to 40 times the size of the earth when the 40 00:03:32,410 --> 00:03:38,290 photograph was taken. the x-ray telescopes were designed to study the evolution of a hot 41 00:03:38,290 --> 00:03:44,550 atmosphere of the Sun. Here is an example of a rapid change in pressure 42 00:03:51,000 --> 00:03:55,830 this picture was taken at the time when the major reconfiguration took place. at 43 00:03:55,830 --> 00:04:01,200 this time the brightest area with the biggest emitter electric in temperature 44 00:04:01,200 --> 00:04:09,150 was in excess of four million degrees and perhaps 10 million degrees or more. Skylab studies 45 00:04:09,150 --> 00:04:14,190 of corona holes, dark areas on the area on the Sun show that they may be the source of the 46 00:04:14,190 --> 00:04:19,380 solar wind which extends beyond the planet Jupiter coronal holes may also have 47 00:04:19,380 --> 00:04:24,660 strong magnetic boundaries as the Sun rotates, these huge magnetic specters 48 00:04:24,660 --> 00:04:29,370 sleep on earth disturbing the upper atmosphere there are indications that 49 00:04:29,370 --> 00:04:34,130 these disturbances correlate with the formation of low pressure weather centers 50 00:04:34,130 --> 00:04:39,510 Additional astronomy has shown us that the Sun is far more active even violent 51 00:04:39,510 --> 00:04:44,400 than we thought. In the next few years Skylab solar astronomy will tell us even 52 00:04:44,400 --> 00:04:49,680 more about the Sun, but also about our planet Earth a cool island within the 53 00:04:49,680 --> 00:04:55,350 outermost layer of the Sun, Skylab solar study show our space ship Earth in its orbit 54 00:04:55,350 --> 00:05:00,000 around the center of the Sun interacting with a solar wind creating a weight