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Dec 12th, 2011
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  1. [16:38:59] <Gerrit> Does anyone object if I paste 425 lines here?
  2. [16:39:46] <+red-squirrel> go ahead
  3. [16:40:28] <smuckerz> err
  4. [16:40:29] <smuckerz> yeah
  5. [16:40:29] <smuckerz> i do
  6. [16:40:34] <smuckerz> Gerrit
  7. [16:40:36] <smuckerz> pastbin
  8. [16:40:40] <smuckerz> you fimilar with it?
  9. [16:40:51] Faqtotum [~danielg4@gimpelevich.san-francisco.ca.us] has joined ##belz
  10. [16:40:51] ChanServ [ChanServ@services.] has set mode +v Faqtotum
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  13. [16:46:13] <Gerrit> Vanaf video:
  14. [16:46:13] <Gerrit> 1:28 start
  15. [16:46:13] <Gerrit> Thanks for the introduction, my name is Gerrit Holl and I will present my
  16. [16:46:13] <Gerrit> licentiate thesis in the next 30 minutes, welcome all those in the room
  17. [16:46:13] <Gerrit> welcome to tohse connected via internet, while I talk about my thesis, you
  18. [16:46:15] <Gerrit> have printed copies over there or in the e-mail announcement from before.
  19. [16:46:18] <Gerrit> 1:47 frame 2
  20. [16:46:20] <Gerrit> What is it I will talk about? I will start by motivating my thesis
  21. [16:46:23] <Gerrit> project.
  22. [16:46:25] <Gerrit> I will talk about cilmate change, which is the ultimate context of my
  23. [16:46:28] <Gerrit> thesis work.
  24. [16:46:30] <Gerrit> And, the motivation and why we care.
  25. [16:46:33] <Gerrit> And then I'm going to introduce the papers and while I introduce the
  26. [16:46:35] <Gerrit> papers I will also discuss the involved theory behind each paper and
  27. [16:46:38] <Gerrit> (resolve?) the context.
  28. [16:46:40] <Gerrit> So first I will talk about paper 1, paper 2, and finally paper 3, which is
  29. [16:46:43] <Gerrit> it.
  30. [16:46:45] <Gerrit> (...) from the first two papers
  31. [16:46:48] <Gerrit> But always
  32. [16:46:50] <Gerrit> 2:35 frame 3
  33. [16:46:53] <Gerrit> 2:38 frame 4
  34. [16:46:55] <Gerrit> But always the first question, and maybe the most important question
  35. [16:46:58] <Gerrit> why are we doing this, why on Earth, why do we care, for anything
  36. [16:47:00] <Gerrit> 2:48 frame 5
  37. [16:47:03] <Gerrit> For me, the prime motivation of this thesis work is...
  38. [16:47:05] <Gerrit> this is planet Earth, this is a photograph taken by the Apollo astronauts,
  39. [16:47:08] <Gerrit> the last Apollo mission on its way to the moon, but this is not a picture
  40. [16:47:10] <Gerrit> of the moon, but a picture of the Earth. Antarctica is at the top, because
  41. [16:47:13] <Gerrit> that happens to be how the spacercaft was oriented. We are used to see
  42. [16:47:15] <Gerrit> Antarctica at the bottom, but that is pretty random.
  43. [16:47:18] <Gerrit> We all live on Earth, we inhabit this planet, we have only one planet, we
  44. [16:47:20] <Gerrit> need to cherish it. Are we cherishing it?
  45. [16:47:23] <Gerrit> 3:27 frame 6
  46. [16:47:25] <Gerrit> The climate is changing. There is a lot of information in this figure, but
  47. [16:47:28] <Gerrit> teh fact that the climate is changing is hiddin in a small number at teh
  48. [16:47:30] <Gerrit> bottom that is net absorption, 0.9 W m-2, due to humans changing the
  49. [16:47:33] <Gerrit> composition of teh Earth atmosphere.
  50. [16:47:35] <Gerrit> One element of the climate that is difficult to understand, that has a lot
  51. [16:47:38] <Gerrit> of forcings and feedbacks in the climate system, are the clouds.
  52. [16:47:40] <Gerrit> Here, you see, clouds they have an important, complicated feedback,
  53. [16:47:43] <Gerrit> because they reflect incoming solar radiation, they absorb outgoing
  54. [16:47:45] <Gerrit> longwave radiation, they emit radiation, both upward and downward, and
  55. [16:47:48] <Gerrit> sometimes they have a cooling effect, sometimes they have a cooling
  56. [16:47:50] <Gerrit> effect.
  57. [16:47:53] <Gerrit> The net effect from the heating and cooling is a function of the latitude,
  58. [16:47:55] <Gerrit> a function of the altitude, they are important for hydrology, and clouds
  59. [16:47:58] <Gerrit> are actually pretty poorly understood.
  60. [16:48:00] <Gerrit> 4:45 frame 7
  61. [16:48:03] <Gerrit> To get a good understanding of clouds, to get a good quantification of
  62. [16:48:05] <Gerrit> clouds, we need satellite observations.
  63. [16:48:08] <Gerrit> And my thesis is about satellite observations of clouds, in particulary,
  64. [16:48:10] <Gerrit> about ice clouds, and one quantity that I'm focussing on a lot, is the Ice
  65. [16:48:13] <Gerrit> Water Path, which is the column mass density of ice in a cloud, so you
  66. [16:48:15] <Gerrit> might say it's, how much ice is there in a could, might sound like a
  67. [16:48:18] <Gerrit> pretty fundamental thing to know, but even a question like this, as this
  68. [16:48:20] <Gerrit> figure shows, even such a question the estimates vary by one order of
  69. [16:48:23] <Gerrit> magnitude, if you take the extremes, the estimates that are very high,
  70. [16:48:25] <Gerrit> the estimates that are very ligh, the differences are so huge, that we
  71. [16:48:28] <Gerrit> basically don't have a clue how much ice there is in a cloud.
  72. [16:48:30] <Gerrit> Which is a bit of a problem, because we just established that clouds are
  73. [16:48:33] <Gerrit> so important.
  74. [16:48:35] <Gerrit> Well, there are some fundamental reasons that the measurements vary so
  75. [16:48:38] <Gerrit> widely, because some are based on infrared, some are based on microwave,
  76. [16:48:40] <Gerrit> and the physics of the microwave obseravtions or an infrared observation
  77. [16:48:43] <Gerrit> are quite different.
  78. [16:48:45] <Gerrit> For example, microwave radiation, wavelength is large in relation to the
  79. [16:48:48] <Gerrit> ice particle, and therefore, and then there is not so much attenuation,
  80. [16:48:50] <Gerrit> so, ... cloud with small particles is completetly transparent to microwave
  81. [16:48:53] <Gerrit> obseraviotns.
  82. [16:48:55] <Gerrit> On the other hand, infrared observations, they are seeing even the thin
  83. [16:48:58] <Gerrit> clouds, and when a cloud is thick, it's completely opaque, it cannot see
  84. [16:49:00] <Gerrit> through the cloud, so when looking at the cloud, will also see part of the
  85. [16:49:03] <Gerrit> cloud
  86. [16:49:05] <Gerrit> But maybe if we have a combination of both, maybe we can do a better job.
  87. [16:49:08] <Gerrit> And that is what my thesis is about: can we do a better job?
  88. [16:49:10] <Gerrit> 7:03 frame 8
  89. [16:49:13] <Gerrit> So now I will talk about my first paper, whic his considered as a first
  90. [16:49:15] <Gerrit> step toward improving this.
  91. [16:49:18] <Gerrit> As I mentioned, the different components have different strengths, and
  92. [16:49:20] <Gerrit> it's not just me saying that.
  93. [16:49:23] <Gerrit> 7:17 frame 9
  94. [16:49:25] <Gerrit> In April, last year in April, I was at the international workshop of
  95. [16:49:28] <Gerrit> Space-based observations of frozen precipitations, IWSSM, where one
  96. [16:49:30] <Gerrit> recommendation from one of the working groups was that: mathups of
  97. [16:49:33] <Gerrit> spaceborne passive microwave observations with Cloudsat are critical for
  98. [16:49:33] mobile [~Gossamer@h33.55.188.173.dynamic.ip.windstream.net] has quit IRC: Ping timeout: 248 seconds
  99. [16:49:35] <Gerrit> improving the global snowfall detection capabilities of passive
  100. [16:49:38] <Gerrit> instruments.
  101. [16:49:40] r0bby_ [~wakawaka@guifications/user/r0bby] has quit IRC: Remote host closed the connection
  102. [16:49:40] <Gerrit> Say what you need to do is to combine CloudSat, which is an active,
  103. [16:49:43] <Gerrit> scientific radar, with passive, passive microwave, and other passive
  104. [16:49:45] <Gerrit> instruments, so that you can improve the retrievals from the passive ones.
  105. [16:49:48] <Gerrit> They said it in April 2011, already more than, almost a year before, I had
  106. [16:49:50] <Gerrit> a pubilaciotn in Atompsheri Measurement Techniques, on Collocating
  107. [16:49:53] <Gerrit> satellite based radar and radiometer measurements — methodoloy and usage
  108. [16:49:55] <Gerrit> examples.
  109. [16:49:58] <Gerrit> It's my first paper, which is pretty much, closely exactly what is
  110. [16:49:59] r0bby_ [~wakawaka@guifications/user/r0bby] has joined ##belz
  111. [16:50:00] <Gerrit> critically needed according to the workshop, so it's nice to get some independent
  112. [16:50:03] <Gerrit> confirmation that my work is relevant, maybe ...
  113. [16:50:05] <Gerrit> Matchups, I call them collocations, ..., I will come back to this figure
  114. [16:50:08] <Gerrit> later, but a collocation is just different insturments looking at the same
  115. [16:50:10] <Gerrit> place at the same time, might eb at completely different sattelites,
  116. [16:50:13] <Gerrit> different characteristics, but to combine them, synergy, can reach goals
  117. [16:50:15] <Gerrit> that you cannot reach with either satellite alone.
  118. [16:50:18] <Gerrit> 9:24 frame 10
  119. [16:50:20] <Gerrit> This satellite I'm collocating with, this CloudSat, that's a bit of a
  120. [16:50:23] <Gerrit> special satellite.
  121. [16:50:25] <Gerrit> CloudSat is part of a constellation of satellites known as the A-Train.
  122. [16:50:28] <Gerrit> But I'm focussing on CloudSat, I'm not using the other satellites so much
  123. [16:50:30] <Gerrit> at the current moment, but
  124. [16:50:33] <Gerrit> the A-Train, CloudSat carries a Cloud Profiling Radar, it's an active
  125. [16:50:35] <Gerrit> instrument, it looks only straight down, it sees only a very little bit
  126. [16:50:38] <Gerrit> it's dying, we have some five years of data, but unlike weather
  127. [16:50:40] <Gerrit> satellites, it's not going to get replaced and replaced all the time
  128. [16:50:43] <Gerrit> and because it's an active instrument, because it's designed to profile
  129. [16:50:45] <Gerrit> clouds, not for other things, we have good reasons to believe that the CloudSat ice water path
  130. [16:50:48] <Gerrit> product is the best ice water path product we have.
  131. [16:50:51] <Gerrit> CloudSat is an active instrumente, on the other hand, also close to the
  132. [16:50:53] <Gerrit> A-Train, are weather satellites, that contain passive instruments, but
  133. [16:50:56] <Gerrit> that are operational, that means if this satellite dies, they will
  134. [16:50:58] <Gerrit> replace it, because they are essential for the everyday weather forecast.
  135. [16:51:01] <Gerrit> Those satellites carry instruments, such as passive microwave and
  136. [16:51:03] <Gerrit> infrared, and those are the ones are collocating with the cloudsat
  137. [16:51:06] <Gerrit> But what are all those satellites actually measure?
  138. [16:51:08] <Gerrit> 10:58 frame 11
  139. [16:51:11] <Gerrit> measure, they don't measure ice, they are way above the clouds, below the
  140. [16:51:13] <Gerrit> clouds we also don't measure ice from the ground, so you measure by remote
  141. [16:51:16] <Gerrit> sensing, so the actual quantity that is being measured is electromagnetic
  142. [16:51:18] <Gerrit> radiation, which is emitted by any object at any temperature, for example
  143. [16:51:21] <Gerrit> by the Sun in the visible because it's so hot it's in the visible, the
  144. [16:51:23] <Gerrit> Earth which emits mostly in the infrared, here I'm also showing the
  145. [16:51:26] <Gerrit> microwave.
  146. [16:51:28] <Gerrit> Radiometers, such as the High-resolution Infarred Radiatien Sounder, or
  147. [16:51:31] <Gerrit> the Advanced Very High Resolution Radiomete,r they measuer radiation
  148. [16:51:33] <Gerrit> intensity, in teh infrared such as AVHRR, or in the microwave such as MHS, or
  149. [16:51:36] <Gerrit> actively such as the cloud profiling radar, the CPR.
  150. [16:51:38] <Gerrit> (NOTE: backgrounds not clear on projector)
  151. [16:51:41] <Gerrit> They measure actively such as the cloud profiling radar.
  152. [16:51:43] <Gerrit> And as I said, the passive instruments are carried on operational
  153. [16:51:46] <Gerrit> satellites, the cloud profiling radar is carried on cloudsat, and what I
  154. [16:51:46] <smuckerz> Gerrit
  155. [16:51:46] <smuckerz> Gerrit
  156. [16:51:47] <smuckerz> Gerrit
  157. [16:51:47] <smuckerz> Gerrit
  158. [16:51:48] <Gerrit> do is matching the two, the CloudSat is active, so I need to
  159. [16:51:51] <Gerrit> ONVERSTAANBAAR
  160. [16:51:53] <Gerrit> Microwave we don't see any curve here, because energy-wise the microwave
  161. [16:51:56] <Gerrit> is way way less, orders of magnitude less, than the infrared. But that
  162. [16:51:58] <Gerrit> doesn't matter as long as we can measure it, beacuse it still contains
  163. [16:52:01] <Gerrit> really
  164. [16:52:03] <smuckerz> Gerrit
  165. [16:52:03] <smuckerz> Gerrit
  166. [16:52:03] <Gerrit> valuable information in the context of atmospheric remote sensing, even if
  167. [16:52:04] <smuckerz> Gerrit
  168. [16:52:06] <Gerrit> it's so little radiation in absolute ways
  169. [16:52:07] <smuckerz> hey Gerrit
  170. [16:52:08] <Gerrit> 13:02 frame 12
  171. [16:52:09] <smuckerz> seriously
  172. [16:52:11] <Gerrit> back to those collocations.
  173. [16:52:13] <Gerrit> In this paper I present some statistics from (...) collocations, and
  174. [16:52:14] <smuckerz> why the hell
  175. [16:52:16] <Gerrit> collocation statistics. This was before NOAA-19 was launched. And then I
  176. [16:52:17] <smuckerz> don't you use pastebin?
  177. [16:52:18] <Gerrit> found only NOAA-18 with global collocatoins, which can be explained by the
  178. [16:52:21] <Gerrit> fact that NOAA-18 is close to the A-Train. The collocations, they occur
  179. [16:52:23] <Gerrit> globally, but not all combinations of all angles, due to the, the exact
  180. [16:52:26] <Gerrit> orbit of NOAA-18 and of the cloudsat, collocations occur in ... patterns
  181. [16:52:28] <Gerrit> this shows the latitude and the angle at which collocations occur, so it
  182. [16:52:31] <Gerrit> means that above the equator there are no collocations that occur at
  183. [16:52:33] <Gerrit> exactly the same time exactly then. This is how the orbits are, so there
  184. [16:52:36] <Gerrit> are some boundary conditions in what kind of collocations can we look at
  185. [16:52:38] <Gerrit> 13:58 frame 13
  186. [16:52:41] <Gerrit> The more important issue here is that the satellite have quite different
  187. [16:52:42] <+Faqtotum> smuckerz: he probably pasted that all at once
  188. [16:52:43] <Gerrit> footprints.
  189. [16:52:46] <Gerrit> I will zoom in a bit on part of this figure.
  190. [16:52:48] <Gerrit> Here zie je de green ellipse, which is the footprint from the MHS,
  191. [16:52:51] <Gerrit> microwave humidity sounder; HIRS which is the high-resolution infrared
  192. [16:52:53] <Gerrit> radiation sounder, as showed in an earlier plot, has lots of nice
  193. [16:52:56] <Gerrit> channels, but the footprints is such that it's difficult to use, because
  194. [16:52:58] <Gerrit> here, it doesn't even cololcate with the cloudsat at all.
  195. [16:53:01] <Gerrit> and then those bricks, that's the AVHRR, which has less nice channels than
  196. [16:53:03] <Gerrit> the HIRS, it's approximately the same frequency range, but it's a bit
  197. [16:53:06] <Gerrit> poorer resolution, maybe poorer calibartion as well, but it's my best bet
  198. [16:53:08] <Gerrit> because at least it collocates
  199. [16:53:11] <Gerrit> Now for the MHS collocations with the CloudSat, there are currently two
  200. [16:53:13] <Gerrit> options, either collocate each one pixel with the MHs pixel, each one
  201. [16:53:16] <Gerrit> footprint with the entire MHS footprint, or average them, even if I
  202. [16:53:18] <Gerrit> average the cloudsat, still over a much smaller area than the MHS,
  203. [16:53:21] <Gerrit> something always need to take into account when doing statistics with it.
  204. [16:53:23] <Gerrit> It's a bit easier with AVHRR, because there is only, can just take the
  205. [16:53:26] <Gerrit> closest and if it's too far, it's too far
  206. [16:53:28] <Gerrit> and with the HIRS, sometimes there are cocllocations, but most of the
  207. [16:53:31] <Gerrit> tmie, there actually are not, because those different HIRS-pixel are
  208. [16:53:32] <smuckerz> holy hell
  209. [16:53:33] <Gerrit> pretty far away.
  210. [16:53:36] <Gerrit> The CloudSat looks only at nadir and that's why we don't fill the entire
  211. [16:53:36] <smuckerz> are you fucking serious
  212. [16:53:38] <Gerrit> pixel, also with AVHRR, we can fill the entire MHS pixel, which is
  213. [16:53:39] <smuckerz> Gerrit
  214. [16:53:41] <smuckerz> Gerrit
  215. [16:53:41] <Gerrit> (OVERSTAANBAAR)
  216. [16:53:43] <smuckerz> what
  217. [16:53:43] <Gerrit> 15:58 frame 14
  218. [16:53:44] <smuckerz> the
  219. [16:53:45] <smuckerz> fuck
  220. [16:53:46] <Gerrit> Still, I used collocations between CPR and MHS, and I will present some
  221. [16:53:48] <Gerrit> results from my first paper, from applications from those collocations
  222. [16:53:51] <Gerrit> One application is to collocate CloudSat MHS and just compare the ice
  223. [16:53:53] <Gerrit> water path. In the plot in the introduction, the one from Salomon Eliasson
  224. [16:53:56] <+Faqtotum> smuckerz: frankly, i find this much easier to read than a pastebin
  225. [16:53:56] <Gerrit> and collaborators, I showed a comparison based on the latitudinal average, but
  226. [16:53:58] <Gerrit> here I really compare point by point and of course, yes, they cover
  227. [16:53:59] r0bby_ [~wakawaka@guifications/user/r0bby] has quit IRC: Remote host closed the connection
  228. [16:54:01] <Gerrit> different areas, but still, here we can confirm that the MHS ice water
  229. [16:54:01] <smuckerz> hey red-squirrel
  230. [16:54:02] <smuckerz> hey red-squirrel
  231. [16:54:02] <smuckerz> hey red-squirrel
  232. [16:54:03] <smuckerz> hey red-squirrel
  233. [16:54:03] <Gerrit> path, based on
  234. [16:54:04] <smuckerz> hey red-squirrel
  235. [16:54:04] <smuckerz> hey red-squirrel
  236. [16:54:05] <smuckerz> hey red-squirrel
  237. [16:54:05] <smuckerz> hey red-squirrel
  238. [16:54:06] <Gerrit> a product called MSPPS, has a much much lower ice water path than CloudSat, since we
  239. [16:54:06] <smuckerz> hey red-squirrel
  240. [16:54:07] <smuckerz> hey red-squirrel
  241. [16:54:09] <Gerrit> believe the CloudSat to be correct we arrive that the MSPPS too low, even
  242. [16:54:11] <Gerrit> for the thicker clouds here that it is supposed to be able to see.
  243. [16:54:14] <Gerrit> Another application I present in the first paper is just to do the statistics,
  244. [16:54:16] <Gerrit> to get the brightness tempearture which, from the MHS, which is a unit of
  245. [16:54:18] <smuckerz> hey red-squirrel
  246. [16:54:19] <Gerrit> radiation intensity and to compare this directly against the ice water
  247. [16:54:19] <smuckerz> hey red-squirrel
  248. [16:54:19] <smuckerz> hey red-squirrel
  249. [16:54:20] <smuckerz> hey red-squirrel
  250. [16:54:20] <smuckerz> hey red-squirrel
  251. [16:54:21] <smuckerz> hey red-squirrel
  252. [16:54:21] <smuckerz> hey red-squirrel
  253. [16:54:21] <Gerrit> path from cloudsat. This is a nice relationship, we can see here for
  254. [16:54:24] <Gerrit> example that the thin clouds below 100 grams per square meter are
  255. [16:54:27] <Gerrit> transparent for microwave radiation, but for thick clouds there is a nice,
  256. [16:54:28] r0bby_ [~wakawaka@guifications/user/r0bby] has joined ##belz
  257. [16:54:29] <Gerrit> also for those clouds, which is actually already above 100 grams per
  258. [16:54:31] <Gerrit> square meter, which is pretty close to the origin on the left figure,
  259. [16:54:34] <Gerrit> on the right hand we have ..., already on 100 grams per square meter it
  260. [16:54:36] <Gerrit> should be possible to measure, when I compare against the simulated
  261. [16:54:39] <Gerrit> datasetso I can confirm that the simulated dataset is mostly correct, there are some small
  262. [16:54:42] <Gerrit> differences, I discuss them in my first paper, but the main conclusion
  263. [16:54:44] <Gerrit> here is, collocations and simulations, they agree pretty well.
  264. [16:54:47] <Gerrit> But the main, what I find the nicest, the most promising application in my
  265. [16:54:49] <Gerrit> first paper, is to actually develop a new product. How do we do that? From
  266. [16:54:52] <Gerrit> the collocations we get a big table of MHS brightness temperatures,
  267. [16:54:54] <Gerrit> radiances, and CloudSat ice water path. And by getting this table, by
  268. [16:54:57] <Gerrit> getting this database, we can train a, in this case I call it an
  269. [16:54:59] <Gerrit> artificial neural network, which is a regression technique that learns to
  270. [16:55:01] <smuckerz> hey red-squirrel
  271. [16:55:01] <smuckerz> hey red-squirrel
  272. [16:55:02] <Gerrit> see patterns, so I show it a lot of combinations of brightness temperatures
  273. [16:55:02] <smuckerz> hey red-squirrel
  274. [16:55:03] <smuckerz> hey red-squirrel
  275. [16:55:03] <smuckerz> hey red-squirrel
  276. [16:55:04] <smuckerz> hey red-squirrel
  277. [16:55:04] <smuckerz> hey red-squirrel
  278. [16:55:04] <Gerrit> and ice water path, then after this I can input new brightness
  279. [16:55:07] <Gerrit> temperatures where I don't hvae collocated ice water path, and
  280. [16:55:09] <Gerrit> (onverstaanbaar)
  281. [16:55:12] <Gerrit> 19:12 frame 15
  282. [16:55:14] <Gerrit> Now this is also still in, still in progress, but this should be pretty promising,
  283. [16:55:17] <Gerrit> and I'm going to continue with that at a later academic point
  284. [16:55:20] <Gerrit> So, in my first paper I had collocations between passive, operational and
  285. [16:55:21] red-squirrel [~rs@unaffiliated/red-squirrel] is now known as rs-afk
  286. [16:55:22] <Gerrit> active, scientific satellites.
  287. [16:55:25] <Gerrit> It's nice.
  288. [16:55:27] <Gerrit> In my second paper, I continue with collocations, but I shift the focus.
  289. [16:55:30] <Gerrit> I shift the focus away from clouds, actually.
  290. [16:55:32] <Gerrit> And look directly at the brightness temperatures of operational
  291. [16:55:35] <Gerrit> satellites.
  292. [16:55:37] <Gerrit> 19:44 frame 16
  293. [16:55:40] <Gerrit> So, second paper.
  294. [16:55:42] <Gerrit> Actually, I'm co-author, it's a paper that was written by Viju John, but I
  295. [16:55:45] <Gerrit> did the collocation part, which is a very important part of the paper, an
  296. [16:55:46] <+Faqtotum> smuckerz: haha
  297. [16:55:47] <Gerrit> essential part.
  298. [16:55:50] <Gerrit> Here it's called, they're called simulateous nadir overpasses, so two,
  299. [16:55:52] <Gerrit> here, two polar orbiting satellites, such as those polar orbiting
  300. [16:55:55] <Gerrit> operational satellites are, there are about six of them, they pass over
  301. [16:55:57] <Gerrit> the pole at each orbit, so pretty frequently they have collocations at the
  302. [16:56:00] <Gerrit> orbit, at the poles sorry.
  303. [16:56:02] <Gerrit> Over the equator, they at a certain point over the equator they pass only once
  304. [16:56:05] <Gerrit> in a couple of weeks, but every orbit they pass ONVERSTAANBAAR
  305. [16:56:07] <Gerrit> what's frequently done is that such collocations at the pole are used to
  306. [16:56:10] <Gerrit> intercalibrate the sensors
  307. [16:56:12] <Gerrit> now, due to orbital drift we actually sometimes have
  308. [16:56:15] <Gerrit> 20:47 frame 17
  309. [16:56:17] <Gerrit> we actually have sometimes have collocations ONVERSTAANBAAR
  310. [16:56:20] <Gerrit> As the figure here on the left shows, that the local time ascending node
  311. [16:56:22] <Gerrit> of the different satellites drifts.
  312. [16:56:25] <Gerrit> The local time ascending node is the time that a sunsynchronous satellite
  313. [16:56:27] <Gerrit> crosses the equator.
  314. [16:56:30] <Gerrit> Those satellites normally are supposed to have a constant time, local time
  315. [16:56:32] <Gerrit> they cross the equator, but due to other gravitational influences this is
  316. [16:56:35] <Gerrit> not really constant, and there is some drift.
  317. [16:56:37] <Gerrit> Thanks to this drift, there are moments that different satellites have the
  318. [16:56:40] <Gerrit> same local time ascending node.
  319. [16:56:42] <Gerrit> (NOTE: looks different?)
  320. [16:56:45] <Gerrit> They have the same local time ascending node, and that means in this
  321. [16:56:47] <Gerrit> period, we actually have global collocations. That means we can compare
  322. [16:56:50] <Gerrit> bias at the equator with the bias at the high latitudes, and do a
  323. [16:56:52] <Gerrit> prediction whether it is right.
  324. [16:56:55] <Gerrit> So there are there pairs of satellites, ... one month, ... two months,
  325. [16:56:57] <Gerrit> where such collocations occur.
  326. [16:57:00] <Gerrit> Most occur between NOAA-19 and NOAA-18, and that is because their orbits
  327. [16:57:02] <Gerrit> were close to each other for a long time.
  328. [16:57:05] <Gerrit> NOAA-19 was just launched, NOAA-18 was just changing the drift, so we can
  329. [16:57:07] <Gerrit> look at some statistics.
  330. [16:57:10] <Gerrit> 22:47 frame 18
  331. [16:57:12] <Gerrit> I show parts of the plot paper by Viju John and me and collobarators,
  332. [16:57:15] <Gerrit> where we compare for different latitudes, in this case look at the bias in
  333. [16:57:17] <Gerrit> MHS, no in AMSU-B, which is also a microwave radiometer, in channel 5 with
  334. [16:57:20] <Gerrit> NOAA-15 and NOAA-16. It is pretty clear here that there is a strong
  335. [16:57:22] <Gerrit> dependence on latitude.
  336. [16:57:24] <smuckerz> hey red-squirrel
  337. [16:57:25] <smuckerz> hey red-squirrel
  338. [16:57:25] <Gerrit> At -90 degrees the bias is much less than at +90 degrees.
  339. [16:57:25] <smuckerz> hey red-squirrel
  340. [16:57:27] <Gerrit> Already, here, if you use only the polar observations, you could already
  341. [16:57:30] <Gerrit> tell that it's not the same.
  342. [16:57:32] <Gerrit> Howeve,r in the next example, MetOp-A/NOAA-17 channel 5, if you use only
  343. [16:57:35] <Gerrit> the polar collocations, you reach the conculsions that there is maybe between 1
  344. [16:57:37] <smuckerz> Faqtotum
  345. [16:57:37] <Gerrit> and 1.5 kelvin in bias
  346. [16:57:40] <Gerrit> If you then correct one of them, down, you would correct it globally,
  347. [16:57:42] <Gerrit> perhaps at the equator, whereas there is actually no bias at all between the two
  348. [16:57:44] <smuckerz> Faqtotum don't you find this shit rediculas
  349. [16:57:45] <Gerrit> because this bias, it depends on latitude, and why does it depend on
  350. [16:57:47] <Gerrit> latitude, because it depends on the scene temperature, and the scene
  351. [16:57:49] <smuckerz> Faqtotum don't you find this shit rediculas and very rude
  352. [16:57:50] <Gerrit> humidity.
  353. [16:57:52] <Gerrit> therefore, we can conclude that it is simply not correct to use only polar
  354. [16:57:55] <Gerrit> SNOs for intercalibration, it is simply too, too simplistic, that is the
  355. [16:57:57] <Gerrit> conclusion from this paper
  356. [16:58:00] <Gerrit> this has also been compared to other metheds
  357. [16:58:02] <Gerrit> 24:36 frame 19
  358. [16:58:03] <smuckerz> Faqtotum, i can't believe he is fucking pasting all this shit in here
  359. [16:58:04] <+Faqtotum> smuckerz: i find it very funny
  360. [16:58:05] <Gerrit> instead, I will proceed, I'm running out of time, but I will proceed
  361. [16:58:07] <Gerrit> my third paper where I shift the focus from collocations to radiative
  362. [16:58:10] <Gerrit> transfer
  363. [16:58:12] <Gerrit> 23:53 frame 20
  364. [16:58:15] <Gerrit> radiative transfer, the modeling, is calculating all those meauruemnts, in
  365. [16:58:16] <smuckerz> Faqtotum, i told his dumbass to use fucking pastebin
  366. [16:58:17] <Gerrit> our case the passive measurements, so we can calculate, we know what the
  367. [16:58:20] <Gerrit> atmosphere is, and then we model other radiation ...
  368. [16:58:22] <Gerrit> this is governed by the radiative transfer equation and I will go through
  369. [16:58:25] <Gerrit> step-by-step, starting with the clear-sky parts, which is absorption, and
  370. [16:58:27] <Gerrit> actually we can consider extinction, since it is just scattering out, we
  371. [16:58:30] <Gerrit> just need to know how much scattering there is, I will focus on the
  372. [16:58:32] <Gerrit> absorption and the emission of gases, so the arrow reperesnts the
  373. [16:58:35] <Gerrit> atmospheric radiation
  374. [16:58:37] <Gerrit> on the left hand of the equation where you have a change in radiation
  375. [16:58:40] <Gerrit> intenisty along the line of sight
  376. [16:58:42] <+Faqtotum> smuckerz: the drama is rather entertaining
  377. [16:58:42] <Gerrit> and then there is extinction, which is absorption plus scattering
  378. [16:58:45] <Gerrit> and there is emission, eh, and as I'll show extinction causes radiation
  379. [16:58:47] <Gerrit> along the line of sight to get less, but emission causes it to get more
  380. [16:58:50] <Gerrit> so later I will focus on the 3rd term, which is related to scattering, but
  381. [16:58:52] <Gerrit> can be considered more complicated
  382. [16:58:55] <Gerrit> but with those ingredients we can
  383. [16:58:57] <Gerrit> 26:08 frame 21
  384. [16:59:00] <Gerrit> do clear-sky simulations. what is shown on the figure in the top, then we can
  385. [16:59:02] <Gerrit> actually calculate it
  386. [16:59:05] <Gerrit> I'll show the parts, part of this figure, I will zoom in on the part I draw in
  387. [16:59:07] <Gerrit> red here
  388. [16:59:10] <Gerrit> show a zoom
  389. [16:59:12] <Gerrit> so I show between, the next plot shows just the different results from
  390. [16:59:15] <Gerrit> radiative transfer between 10 and 13 micrometer
  391. [16:59:17] <Gerrit> 26:40 frame 22
  392. [16:59:20] <Gerrit> ehm, for each atmospheric gas, ro for all atmospheric gases together, we
  393. [16:59:22] <Gerrit> can calculate the opacity or the optical depth, which is just a measure for how
  394. [16:59:25] <Gerrit> opaque it is
  395. [16:59:27] <Gerrit> the higher the opacity, the more radiation is blocked
  396. [16:59:30] <Gerrit> that's a function of wavelength and of species
  397. [16:59:32] <smuckerz> Faqtotum, i find it impressive that someone would do this
  398. [16:59:32] <Gerrit> so here we take some ingredients in the atompsehire
  399. [16:59:35] <Gerrit> we take water vapour, ozone, co2, n2o, etcetera
  400. [16:59:37] <Gerrit> that's the clear-sky part
  401. [16:59:40] <Gerrit> with this we can calculate clear-sky radiation
  402. [16:59:42] <Gerrit> which is by comparison to the cloudy simulation simple
  403. [16:59:43] <+Faqtotum> smuckerz: indeed
  404. [16:59:45] <Gerrit> but my thesis focusses on clouds, so I want to calculate clouds
  405. [16:59:47] <Gerrit> 27:25 frame 23
  406. [16:59:50] <Gerrit> that's why the 3rd term here becomes importan,t which is the scattering
  407. [16:59:52] <Gerrit> source term
  408. [16:59:55] <Gerrit> as radiation meets cloud particles, it can be scattered away, but it can
  409. [16:59:57] <Gerrit> also be scattered into the line of sight, and that's what's reperesented
  410. [17:00:00] <Gerrit> by the 3rd term, which starts with the phase function.
  411. [17:00:02] <Gerrit> 27:47 frame 24
  412. [17:00:05] <Gerrit> the phase function describes the photon
  413. [17:00:07] <Gerrit> the photon meets an ice particle and gets scattered, then it changes the
  414. [17:00:10] <Gerrit> direction of the radiation
  415. [17:00:12] <Gerrit> now in this figure, the photon gets scattered twice and in the end it's
  416. [17:00:15] <Gerrit> more or less, going it's in a very similar direction as when it started
  417. [17:00:17] <Gerrit> so it's important really, necessary to consider the scattering
  418. [17:00:20] <Gerrit> the scattering phase function is the probability density function in
  419. [17:00:22] <Gerrit> describing in what direction the radiation gets scattered
  420. [17:00:25] <Gerrit> unlike the photon in this animation, not every photon gets scattered in
  421. [17:00:27] <Gerrit> the same way
  422. [17:00:30] <Gerrit> one way to model this, is to really follow each photon step by step
  423. [17:00:32] <Gerrit> it's a slow method, slightly faster than this photon, but still a slow
  424. [17:00:35] <Gerrit> method that we can directly apply a scattering phase function such as the
  425. [17:00:37] <Gerrit> two examples in the figure
  426. [17:00:40] <Gerrit> and this scattering phase function, and also the scattering cross section,
  427. [17:00:42] <Gerrit> which determines how likely it is that a scatetring event occurs
  428. [17:00:45] <Gerrit> depends strongly on the size of the, on the wavelength in relation to the
  429. [17:00:47] <Gerrit> size of the particle
  430. [17:00:50] <Gerrit> in the figure there is an example, there's an infrared phase function,
  431. [17:00:52] <Gerrit> which nonlinear for a 50 micrometer particle, an infrared phase function
  432. [17:00:55] <Gerrit> wavelength is much smaller than the size of the particle, then most of the
  433. [17:00:57] <Gerrit> radiation goes, even if it gets scattered it goes straight ahead,
  434. [17:01:00] <Gerrit> whereas in the microwave, it's much more, in this case it's a similar
  435. [17:01:02] <Gerrit> size, size of particle is similar to the size of the wavelength,
  436. [17:01:05] <Gerrit> and it's more scattered in all directions, the phase function
  437. [17:01:07] <Gerrit> so knowing this, we can
  438. [17:01:10] <Gerrit> 29:50 frame 25
  439. [17:01:12] <Gerrit> solve now single frequency, which is, including the clear-sky part, and
  440. [17:01:15] <Gerrit> the cloudy part.
  441. [17:01:17] <Gerrit> But this is rather expensive, unfortunately.
  442. [17:01:20] <Gerrit> If we want, for example, to simulate an entire channel for AVHRR channel
  443. [17:01:22] <Gerrit> 5, you would need about 5000 calculations, which is too many to do
  444. [17:01:25] <Gerrit> practically, certainly if one wants to cloudy radiative transfer
  445. [17:01:27] <Gerrit> but this can be optimised, even in the cloudy case, and that is what my
  446. [17:01:30] <Gerrit> 3rd paper is about
  447. [17:01:32] <Gerrit> 30:26 frame 26
  448. [17:01:35] <Gerrit> Simulation cloudy thermal infrared radiances with an optimised frequency
  449. [17:01:37] <Gerrit> grid in the radiative transfer model ARTS
  450. [17:01:40] <Gerrit> It's a ... sentenec, but what it means that instead of 5000 frequencies,
  451. [17:01:42] <Gerrit> to simulate this channel, you can do with only five
  452. [17:01:44] r0bby_ [~wakawaka@guifications/user/r0bby] has quit IRC: Remote host closed the connection
  453. [17:01:45] <Gerrit> this is a continuation of work presented by
  454. [17:01:47] <Gerrit> 30:47 frame 27
  455. [17:01:49] mrmist [~mrmist@freenode/staff/pdpc.active.mrmist] has joined ##belz
  456. [17:01:50] <Gerrit> Stefan Buehler and collaborators in 2010 it was published, called
  457. [17:01:52] <Gerrit> simulated annealing, and it's a numerical method to give the same channel
  458. [17:01:55] <Gerrit> radiance, in this application, as the large number of frequencies
  459. [17:01:57] <Gerrit> now this paper was focussing directly on clear-sky radiation, but I
  460. [17:02:00] <Gerrit> and ... and derived for clear-sky, applying this method,
  461. [17:02:02] <Gerrit> 31:19 frame 28
  462. [17:02:05] <Gerrit> I get five channels, five frequencies with associated weights, all inside
  463. [17:02:07] <Gerrit> AVHRR channel five, and the daring part here, is that I'm actually
  464. [17:02:10] <Gerrit> applying it to cloudy simulations
  465. [17:02:12] <Gerrit> 31:32 frame 29
  466. [17:02:15] <Gerrit> does it work? how do we know it works.
  467. [17:02:17] <Gerrit> We can test it, and what do we see?
  468. [17:02:20] <Gerrit> ... it works
  469. [17:02:22] <Gerrit> we have the references brightness temperature here
  470. [17:02:25] <Gerrit> where we used only one photon per frequency for 5000, more than 5000
  471. [17:02:27] <Gerrit> frequencies, which took about 20 times longer to run than the fast setup,
  472. [17:02:30] <Gerrit> that is on the y-axis here, where I used 1000 photons times five
  473. [17:02:32] <Gerrit> frequencies
  474. [17:02:35] <Gerrit> the total number of photons is similar, but the reference is more than 20
  475. [17:02:37] <Gerrit> times faster
  476. [17:02:39] r0bby_ [~wakawaka@guifications/user/r0bby] has joined ##belz
  477. [17:02:40] <Gerrit> now I have a setup that I can use for whatever I'm going to do in the
  478. [17:02:42] <Gerrit> future
  479. [17:02:45] <Gerrit> 32:17 frame 30
  480. [17:02:47] <Gerrit> which is, among other things, a cloudy study of radiances through clouds,
  481. [17:02:48] <smuckerz> hello mrmist
  482. [17:02:49] <mrmist> Gerrit: you seem to be posting a novel here. I'd suggest using pastebin
  483. [17:03:01] <smuckerz> he was already told
  484. [17:03:04] <smuckerz> to use pastebin
  485. [17:03:24] rs-afk [~rs@unaffiliated/red-squirrel] is now known as red-squirrel
  486. [17:03:26] <smuckerz> 23 minutes ago
  487. [17:03:30] <smuckerz> to be precise
  488. [17:03:32] <+Faqtotum> it seems to have stopped
  489. [17:03:36] <+Faqtotum> idk why
  490. [17:03:45] <mrmist> it does.funny how that happens sometimes.
  491. [17:04:00] <smuckerz> hmm...
  492. [17:04:03] <+Faqtotum> maybe he crashed irssi
  493. [17:04:09] <smuckerz> what's the term...
  494. [17:04:09] <+Faqtotum> happens sometimes
  495. [17:04:10] <smuckerz> shun?
  496. [17:05:07] <+Faqtotum> afk
  497. [17:07:17] <smuckerz> mrmist, thank you
  498. [17:07:26] <mrmist> np
  499. [17:07:44] <smuckerz> no clue if you did anything
  500. [17:07:49] <smuckerz> but you did show up
  501. [17:07:49] <smuckerz> :)
  502. [17:07:50] <mrmist> I joined
  503. [17:08:07] robbyoconnor [~wakawaka@guifications/user/r0bby] has joined ##belz
  504. [17:08:14] <smuckerz> yup :)
  505. [17:08:19] <smuckerz> that was something :)
  506. [17:08:27] Bateau [~Ghost@unaffiliated/section9] has joined ##belz
  507.  
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