WEBVTT FILE 1 00:00:00.060 --> 00:00:04.500 The WISPR instrument is made of two telescopes that are designed to sit 2 00:00:04.500 --> 00:00:09.750 between the two antennae from the FIELDS experiment and image the solar wind and 3 00:00:09.750 --> 00:00:14.219 the corona as we're flying into it so whisper is the latest instrument we've 4 00:00:14.219 --> 00:00:18.930 built before but had really two requirements we wanted to be able to see 5 00:00:18.930 --> 00:00:22.080 far from the spacecraft and then be able to track 6 00:00:22.080 --> 00:00:27.060 the structures that are flowing out from the Sun and then as they passed the 7 00:00:27.060 --> 00:00:31.590 spacecraft we would see them locally at the space path the WISPR instrument is 8 00:00:31.590 --> 00:00:36.059 the only imaging instrument on the Parker Solar Probe and if is looking in the 9 00:00:36.059 --> 00:00:41.100 direction that the spacecraft is traveling and what it sees is light 10 00:00:41.100 --> 00:00:45.960 scattered by the dust that's in orbit about the Sun but then once we remove 11 00:00:45.960 --> 00:00:51.570 that what we see is the light scattered by the electrons in the corona in the 12 00:00:51.570 --> 00:00:56.760 solar wind these measurements that were making from the WISPR instrument have 13 00:00:56.760 --> 00:01:01.320 been made before by other instruments from 1au from the distance of the earth 14 00:01:01.320 --> 00:01:06.330 about 100 million miles from the Sun by getting closer we're increasing then the 15 00:01:06.330 --> 00:01:11.130 ability to see what's really close to the Sun the fact that you're close means 16 00:01:11.130 --> 00:01:16.049 that you you don't have all this this material that's in between you and the 17 00:01:16.049 --> 00:01:20.939 and the object that you really interested in and that contributes to - 18 00:01:20.939 --> 00:01:26.310 background noise and so you're looking at something that's much more pristine 19 00:01:26.310 --> 00:01:28.829 you're looking at just that object all by itself 20 00:01:28.829 --> 00:01:35.400 by going eventually 95% of the way to the Sun we are going to be able to see 21 00:01:35.400 --> 00:01:42.299 what is a dust free region around the Sun that's going to be exciting part so 22 00:01:42.299 --> 00:01:49.290 a probe cannot have any imager that looks at the Sun directly so the WISPR 23 00:01:49.290 --> 00:01:55.320 instrument looks off of the heat shield that protects us from this very intense 24 00:01:55.320 --> 00:02:01.049 heat and so we we sort of peek over the edge of it we use it as a shield to 25 00:02:01.049 --> 00:02:06.119 block out the Sun itself and that allows us to see this very faint glow coming 26 00:02:06.119 --> 00:02:09.349 from the corona that's only observed during the clips 27 00:02:09.349 --> 00:02:14.239 for example we're creating an artificial Eclipse. Eclipses are great but from 28 00:02:14.239 --> 00:02:18.349 the data point of view I like my instruments better they're working 29 00:02:18.349 --> 00:02:23.360 continuously round the clock seven days a week 24 hours a day 365 days a year 30 00:02:23.360 --> 00:02:28.840 sometimes for years.