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--- atmos:citation:research:research:iccp-cloudprobe2024_instructions [2024/06/28 19:36] – delene
+++ atmos:citation:research:research:iccp-cloudprobe2024_instructions [2024/06/28 20:22] (current) – delene
@@ Line 29: / Line 29: @@
     - Complete and partial images ''(Assume sum of the above two''
   - Number distribution functions before corrections for particle size (we will use counts per bin per second so that assumptions about the sample volume dependence on maximum dimension don't affect the results).
-    - Use 1-second resolution for generating counts;
+    * Use 1-second resolution for generating counts;
-    - Bins should have widths corresponding to 1 pixel
+    * Bins should have widths corresponding to 1 pixel
-    - Entries should correspond to number of counts in that bin for given second (should be integer)
+    * Entries should correspond to number of counts in that bin for given second (should be integer)
-    - Files should cover entire length of time in synthetic data files
+    * Files should cover entire length of time in synthetic data files
-    - Should include complete and partial images
+    * Should include complete and partial images
       * UPDATE: In order for these size distributions to be comparable, we need to use the same definition of dimension. I suggest that we use maximum particle dimension so that we are all using the same definition (Note that there still may be some differences because there are different algorithms for defining maximum dimension).  Note also that the simulations have a constant PSD over the full minute, so it is probably easier to aggregate everything into a single distribution rather than breaking down by the second.  However, we can handle data submitted either way.
   - Number distribution function after corrections for particle sizes (we will specify a priori the sample volume)